Observations of Nebulae and Clusters of Stars, Made at Slough, with a Twenty-Feet Reflector, between the Years 1825 and 1833

XIX. Observations of Nebulæ and Clusters of Stars, made at Slough, with a Twenty-feet Reflector, between the years 1825 and 1833. By Sir John Frederick William Herschel, Knt. Guelp. F.R.S. &c. Received July 1,—Read November 21, 1833. The following sheets contain the results of observations begun about the year 1825, and prosecuted with more or less assiduity from that time up to the commencement of the present year, in pursuance of a design to review the nebulæ and clusters of stars discovered by my father; and perhaps, in so doing, to add to their number, and to extend in some degree our knowledge of the nature and physical construction of that mysterious and interesting class of bodies. It was my original intention to have deferred the publication of these observations until I should have been able to have presented their results to the Royal Society in the more complete form of a general catalogue of nebulæ and clusters visible in this latitude; in which all my father's nebulæ should have been included, and their places determined by at least two observations. To have done this, however, would have required several years' additional work; and the want of an extensive list of nebulæ arranged in order of right ascension, having, since the recent improvements in the achromatic telescope, and the increased assiduity of astronomers in the detection and observation of comets, become continually more pressing, and the deficiency more and more complained of, I have thought it on the whole a preferable course to supply that deficiency so far as I am able, not by the production of a catalogue pretending to a precision and a completeness I am unable yet to give it, but by simply stating the individual results of such observations as I have hitherto made; with no other preparation than that of reducing them all to a common epoch, arranging them in order of right ascension, and bringing together, in every case where the same object has been more than once observed, all the observations of it which occur. By so doing, two distinct ends are accom- plished. In the first place, the series of observations thus arranged can be used, as a catalogue, for reference, and may serve the purposes of one, until a more perfect one can be produced—(valeat quantum). In the next place, the results so stated, carry with them their own weight and evidence. Where several observations of one and the same object occur, their agreement or disagreement will enable every one to assign to them their proper degree of credit,—to appreciate the amount of error, both accidental and inherent, to which the system of observation adopted is liable; and being thus impressed with a due notion of the degree of latitude with which each result is to be interpreted, he will readily perceive what reliance can be placed on single observations, unchecked by the context. My mode of observing,—the general character of the instrument employed, and the principal sources of error to which its determination of the places of objects is liable, are stated in considerable detail in my five catalogues of double stars discovered with it, published in the Memoirs of the Astronomical Society. To these, therefore, I will refer for the particulars in question: but it will be right here to mention, that a much greater latitude of error must unavoidably subsist in observations of nebulae than in those of stars. Many of these objects present a large and ill-defined surface, in which it is not always easy to say where the centre of greatest brightness is situated. Vast numbers of them are so extremely faint as to be with difficulty discerned at all, or not until they have been some time in the field of view, or are even just about to quit it. In such cases the observations become hurried and uncertain; and this peculiar and fertile source of error and mistake is greatly increased by their excessively irregular distribution over the heavens,—crowded together in some places so as to allow hardly any interval between their transits,—while in others whole hours elapse without a single nebula occurring in the zone of the heavens under examination. In these crowded parts of the heavens, it is not only the number, but the variety and interest of the objects which distract attention and render it scarcely possible to proceed with that methodical calmness and regularity which is necessary to ensure numerical correctness, especially when the observer has continually present to his mind the rarity of his opportunities. It is only in the months of March, April, and May that the richer parts of the heavens can be advantageously observed, and then only in the complete absence of the moon, and of twilight. When to these conditions we add those which arise from the variable and uncertain nature of our climate, it will be seen that a number of circumstances by no means frequently concurring, is necessary to produce a night in which it is possible to make any great progress in a review of nebulæ; and that in fact there is hardly any branch of astronomy which has a greater tendency to create a sense of hurry, of all things the most fatal to exact observation. The observations which are here registered comprise, more or less, about 2500 nebulæ and clusters of stars, which is the number of those observed by my father; but of the two collections, only about 2000 are common to both, the remaining 500 of mine being new. It may serve to show the close and rigorous nature of my father's scrutiny, when I state, that among these 500 I can call to mind only one very conspicuous and large nebula, and only a very few entitled to rank in his first class, or among the "bright nebulæ." By far the greater proportion of them are objects of the last degree of faintness, only to be seen with much attention and in good states of the atmosphere and instrument. This is so far satisfactory, that it shows pretty evidently our knowledge of the nebulous contents of the northern hemisphere to be at length nearly complete, and that to make a further step, the powers of an instrument like the 40-feet reflector will be required. It has generally been my practice to make some kind of sketch or drawing; sometimes more, sometimes less elaborate, of any nebula at all remarkable which presented itself. In many instances careful drawings have been made and repeatedly compared, at distant intervals, with the objects they have been intended to represent. The difficulty of making satisfactory representations of such objects is, however, extreme; and of those which accompany this paper, as specimens of the various classes of objects which the heavens present, I am rather disposed to apologize for the incorrectness than to vaunt the accuracy. General resemblance, however, I can vouch for; and where fidelity in details has been attempted, I should hope that glaring departures from nature will hardly be found to subsist. Among the figures will be found representations of some very extraordinary objects, which have not hitherto been sufficiently pointed out to the notice of astronomers, and of which indeed some of the most remarkable peculiarities have escaped every former observer. These are briefly noticed in the descriptions appended to each observation, and more distinctly and at large in the explanations of the plates. Meanwhile it is only necessary for any reader to cast his eye over the figures, to be satisfied that many of these mysterious objects possess a symmetry of parts, and a unity of design, which, singular as their constitution must appear, strongly mark them as systems of a definite nature, each complete in itself, and subservient to some distinct purpose of which it is in vain for us to conjecture the nature. The manner in which the observations are presented in the following pages requires little explanation. The first column contains a general number for convenience of future reference; the second, the number or name under which each nebula is to be found, either in my father's catalogues (in which case his class and number is set down,) or in the brief but important list furnished by Messier in the Mémoires de l'Académie des Sciences for 1771, and the Connoissances des Temps for 1783 and 1784, which are indicated by the letter M. When no previous mention of a nebula or cluster could be found in the writings of former observers, it is designated as Nova. A very few are due to Struve. These are noted by Σ. The third column contains the right ascension, and the fourth the north polar distance, for 1830°0. The manner in which these elements are obtained from the rough observations, or the process of reduction employed throughout the work, will be fully stated in an Appendix annexed to the observations, as well as other matters of detail which may be advantageously deferred. Under the head of each nebula, as above mentioned, all its observations are brought together, and for distinctness' sake, the hour and minute in AR, and the degree in N.P.D. are only once set down for each, viz. in the upper line, or that which contains the earliest AR of each. When the subsequent observations in AR fall into the next minute, the seconds are counted on beyond 60; and when those in polar distance pass into the next degree, the same contrivance, i.e. counting the minutes beyond 60, is resorted to, to avoid doubling the initial entries and so misleading the eye. When no AR or no P.D. has been observed, the fact is indicated by dotted lines. When only a rough approximation has been obtained (a case unfortunately too common), or when, none having been procured, the necessary datum has been taken from the working list book, this is indicated by the sign ±. What is here meant by the working list will be explained in the Appendix. The column headed "Description and Remarks" contains the abbreviated description taken down, at the time of observation, from the sweeping book. The following is the system of abbreviation used. | B | denotes | Bright. | |-----|---------|---------| | b | | brighter. | | br | | broad. | | c | | considerably. | | Cl or cl | | cluster. | | comp | | compressed. | | D or d* | | double star. | | E | | extended, elliptic, or elongated. | | e | | extremely, excessively. | | F | | Faint. | | f | | following. | | fig | | figure. | | g | | gradually. | | i or irr | | irregular. | | L | | large. | | l | denotes | long or little. | |-----|---------|-----------------| | M | | in the middle. | | m | | much. | | N | | nebula. | | neb | | nebulous or nebulosity. | | n | | north. | | p | | pretty, preceding. | | pos | | angle of position. | | R | | round. | | r | | resolvable. | | S | | small. | | s | | south, suddenly. | | st | | star, stars. | | sc | | scattered. | | v | | very. | * Star. Moon above the horizon. Moon very troublesome. Globular cluster. In all the descriptions the following order is, or ought to be, adhered to. First the degree of brightness is mentioned, characterized by eB, vB, pB, B, pF, F, vF, eF. Next, the size, generally indicated by L and S with their adverbial adjuncts e, v, p. Thirdly, the general form, as R, E, mE, &c. Fourthly, the degree and rate of condensation, as bM, sbM, vg1bM, &c. If the nebula be resolvable, it is next expressed by r. After these come more distinct numerical particulars, as the estimated diameter, indicated by the number of seconds it was judged to subtend; the measured, or estimated length, breadth, or position with the meridian, &c.; and any other remarks which may have appeared desirable to note at the time. Clusters are characterized as Rich, or poor, or compressed, loose, or scattered, &c. For example:— "v B; v L; l E; v g p m b M; 50''1; 45'' br; pos 29°3 by microm. a ≈ 9 m 45° n p dist 80'." Which expanded runs thus: "Very bright; very large; little extended; very gradually pretty much brighter in the middle; 50'' long; 45'' broad; angle of position (reckoned always from the north, and from a meridian, in the direction north, following, south, preceding,) measured 29°3 by the micrometer. A star of the ninth magnitude is situated 45° north preceding the centre of the nebula, and at a distance from it of 80", (both by estimation)." Measured angles are always marked as above, in degrees and decimals. Finally, the last column contains the sweep in which the observation occurs, numbered regularly on in order of time up to sweep 427, with only one inter- ruption of the order, viz. that the sweeps marked 43, . . . . 49 precede sweep 1 in order, having been written down on separate sheets in the year 1823, before the commencement of my more regular plan of observation, and mislaid. ## Observations of Nebulae and Clusters of Stars. | No. | Synonym | \( \mathcal{R} \) 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------------|--------------|------------------------|-------| | 1 | III. 868 | h m s 0 0 1·6 | 86 19 58 | Very Faint (v F); Large (L); very gradually a little brighter in the middle (v g l b M); 40" in diameter (40'). | 95 | | | | | 2·5 19 21 | Bright (B); Small (S); very suddenly much brighter in the middle (v s m b M); 12" long; much extended (m E); a star precedes. | 300 | | 2 | III. 866 | 0 0 2·0 | 57 30 40 | No description | 102 | | | | 4·7 30 51 | | Small stars and nebulosity. | 104 | | 3 | II. 591 | 0 0 3·0 | 75 8 37 | e F; R; b M; a star 10 m, n p, dist. 5' | 174 | | | | 3·6 7 41 | | e F; R; v g v l b M; 40" | 175 | | | | 7·5 7 23 | | F; R; v g b M; 60". | 11 | | | | | | v F; R; l b M | 1 | | 4 | Nova? | 0 0 19·6 | 63 13 29 | p B; R; b M; 20" (? if not IV. 15) | 172 | | 5 | IV. 15 | 0 1 50± | 63 15 0 | A star 15 m with a burr \( \mathcal{R} \) from Cat | 178 | | 6 | II. 853 | 0 1 58·5 | 57 35 27 | p B; p L; irreg fig; (very clear sky). | 106 | | | | 59·8 35 33 | | p B; E | 100 | | 7 | III. 861 | 0 3 32·6 | 59 54 15 | No description | 102 | | | | 36·9 53 31 | | p F; L; R; (very foggy) | 104 | | | | ... 54 30 | | e F; S; R | 178 | | 8 | IV. 58 | 0 3 52·5 | 18 25 17 | A * 10 m with strong neb atmosph 15" diameter. Exactly R and p suddenly fading away makes a D * class 5 with a * preceding. | 378 | | | | 55·5 25 24 | | The L * of a D * strongly affected with a neb burr. Pos 241°·4; \( \Delta \mathcal{R} = 25°; 10 and 12 m. | 380 | | | | 59·4 25 43 | | A star 11 m with a luminous atm 30 or 40" diam. | 228 | | 9 | Nova. | 0 4 12·4 | 60 1 48 | e F; has * 12 m 45" dist; pos 325°? | 100 | | 10 | Nova. | 0 4 26·5 | 59 39 22 | e F; v S; not to be seen but in the clearest night | 106 | | 11 | III. 183| 0 6 23± | 72 24 21 | v F; S; E | 92 | | 12 | Nova. | 0 6 36·4 | 78 30 ± | About this place a considerable space seems affected with nebulosity. | 14 | | 13 | II. 241 | 0 6 45·4 | 73 36 50 | B; S; s b M | 92 | | 14 | III. 428| 0 7 42·6 | 97 15 48 | F; R; p s b M; 15" | 186 | | 15 | V. 16 | 0 9 32·8 | 60 52 10 | An extr F cluster with neb 5' diam. Several * s 15...18 m. Seen distinctly, but there is also unresolved neb. | 178 | | 16 | Nova. | 0 12 21·6 | 68 34 46 | F; S; R; p s b M; 15" | 166 | | 17 | Nova. | 0 12 32·1 | 68 29 16 | E; perhaps bicentral; makes trapezium with three B stars. | 166 | | 18 | Nova. | 0 13 36·8 | 61 11 30 | F; R; g b M; 15" | 178 | | 19 | II. 257 | 0 13 37·2 | 80 27 49 | v F; p L; R; g b M | 15 | | 20 | Nova. | 0 16 0·2 | 29 36 39 | A p S, p compressed cl; 3' diam st 11...18 m in 2 or 3 principal branches. If this be VI. 35, there must be a mistake in my father's obs or mine of 6m in \( \mathcal{R} \). | 216 | MDCCCXXXIII. | No. | Synonym. | AR 1830°. | N.P.D. 1830°. | Description and Remarks. | Sweep. | |-----|----------|-----------|---------------|-------------------------|-------| | 21 | III. 148 | h m s | 0 17 5'4 | Not v F; p L; R; b M; 40''. Seen in moonlight ........ | 114 | | | | | | p B; R; p s b M; 20'' .................................. | 178 | | 22 | Nova. | | 0 17 36'6 | A v loose, p rich cl; *s 9...12 m; * 9 m in M taken .... | 378 | | 23 | III. 869 | | 0 20 6'5 | v F; S; close to a d *. The s p of two .................. | 95 | | | | | | F; S; b M; n f a d *; the s p of two neb ................ | 93 | | 24 | VIII. 79 | | 0 20 27'1 | A * 9 m about M of a v L, coarse sc rich cl of * s 9...13 m which more than fills field. | 213 | | 25 | II. 854 | | 0 20 31'5 | p B; 1 E in meridian; the n f of two .................... | 95 | | | | | | B; E; b M; 20'' ......................................... | 93 | | 26 | II. 855 | | 0 21 27'3 | p B; R; b M; C, yet a p good obs ....................... | 108 | | | | | | e F; b M; has a s * 3' dist; pos 150°± .................. | 110 | | | | | | p F; R; 1 b M; 25''; a good obs ....................... | 113 | | | | | | Excess F C and haze. P D no reliance; much past meridian when taken, and wanting a great correction. | 93 | | 27 | Nova. | | 0 23 5'8 | F; p L; R; v g l b M; 30...40''; has a * 8.9 m, dist 5'; pos 75°± | 186 | | 28 | Nova. | | 0 23 31'7 | A loose cl; * s 11 and 12 m; 10' diam; place that of a double * (h 1033) whose AR is erroneously stated in my 4th Catalogue. | 219 | | 29 | Nova. | | 0 23 53'3 | v F; v L; irr R; 4...5' diam; loses itself insensibly; has a * 11 m in centre. | 207 | | 30 | II. 478 | | 0 25 26'2 | v F; p L; E; v g l b M; 60'' ................................ | 310 | | 31 | III. 467 | | 0 25 43'0 | e F; S; R; 15 or 16'' .................................. | 373 | | 32 | III. 476 | | 0 27 8'6 | Has a * 7 m, 5' dist; pos of neb from * 195°5 ........... | 166 | | 33 | III. 871 | | 0 28 28'6 | e F; a doubtful observation ............................. | 112 | | | | | | v F; R; b M; 20''. A star 11 m pos 225°±, dist = 80'' .. | 113 | | 34 | Nova. | | 0 29 13'5 | Cl v L p Rich 150...200 st 10...18 m; more than fills the field | 381 | | 35 | II. 707 | | 0 29 33'1 | p B; L; R; g b M; full 60'' diam ........................ | 390 | | 36 | Nova. | | 0 29 58'5 | Cl L; p rich; irreg R; 8' diam; straggling; *s 11...15 m .. | 219 | | 37 | Nova. | | 0 30 17± | v F; L; close to a * 15 m. AR by III. 595, which this precedes 25°5. | 95 | | 38 | II. 479 | | 0 30 22'2 | v F; R; sky rather dull ................................ | 310 | | 39 | III. 872 | | 0 30 29'2 | p F; p s b M; 25'' ..................................... | 113 | | | | | | The s p of two, and probably a third. Cloudy ........... | 112 | | | | | | p B; p m E; b M; 40'' l. ................................ | 371 | | | | | | F; R; b M; C, but certainly seen ...................... | 108 | | | | | | F; p L; R; b M ........................................ | 110 | | 40 | II. 856 | | 0 30 33'2 | p B; S; R; b M ......................................... | 95 | | 41 | II. 860 | | 0 30 33'8 | p B; R; b M; 30'' ..................................... | 371 | | | | | | F; R; p s m b M; 30'' .................................. | 113 | | | | | | F; R; b M; C, but certainly seen; a stellar centre .......... | 108 | | | | | | v F; R; 1 b M; 40''; the n f of 2; hazy ................ | 112 | | 42 | III. 595 | | 0 30 42± | p B; R; the f of 2. Δ AR = 25°5; Δ PD = 2' ............ | 95 | | No. | Synonym | AR 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|-------------|----------------|------------------------|--------| | 43 | III. 873 | h m s | 90° 4′ 37″ | v F; L; E; 60″. The last of 3 on the parallel of the first ... | 113 | | | | | 50° 7′ | v F; E; v g l b M; 60″ | 371 | | 44 | V. 18 | 0 31 8′1 | 49 14 45 | p B; v L; m E; pos 160...170°; 15′ l; 7′ br; a faint suspicion of a nucleus; ζ. | 183 | | 45 | V. 36 | 0 31 10′7 | 50 11 30 | A very large space filled with neb | 180 | | 46 | II. 452 | 0 32 1′2 | 104 48 51 | B; R; p s b M; 25″ | 307 | | | | | 1′5 | B; R; p g b M | 373 | | | | | 2′7 | p B; R; p s b M; (a thick haze) | 308 | | 47 | II. 209 | 0 32 30′4 | 65 25 47 | p B; R; g b M; 25″ | 172 | | | | | 26 15 | p F; R; g b M; 20″ | 392 | | 48 | II. 480 | 0 32 59′2 | 100 56 56 | not v F; S; g b M; 10...15″ | 310 | | 49 | III. 244 | 0 32 59′2 | 111 58 54 | e F; 1 E, n f to s p | 293 | | 50 | M. 31 | 0 33 26′3 | 49 39 40 | The great nebula in Andromeda | 180 | | 51 | M. 32 | 0 33 27′8 | 50 4 7 | The companion of the great nebula. e B; p L; s b M to a * 10 m; 40″; a small star follows it 11°5.5. | 183 | | | | | | Viewed. v B R; p s b M; 30″; a * 13 m follows 11°0 | 180 | | 52 | VIII. 78 | 0 33 35′5 | 29 8 37 | A fine L, loose cl; stars 9.10 m on a dark ground; no small stars. Place that of a D (h 1046). | 219 | | 53 | Nova. | 0 33 47′9 | 58 20 49 | e F; S; R; has a * 13 m to s, dist 20″ | 106 | | 54 | III. 146 | 0 34 29′2 | 60 20 26 | not v F; R; b M; 15″ | 177 | | | | | 29′4 | F; R; 1 b M; 30″; ζ ζ, yet distinctly seen | 114 | | 55 | III. 485 | 0 37 14′9 | 106 30 51 | v F; S; R; has * 10 m 3′s | 307 | | 56 | V. 25 | 0 38 30′5 | 102 48 36 | v F; diffused neb involving stars | 373 | | | | | 31′2 | A small constellation in a v diffused neb | 308 | | 57 | V. 20 | 0 38 44′8 | 111 40 49 | e F; v L; v m E; v g l b M; 10′1; pos 172°0. Has no B * in it, but a * 8.9 m at some dist n p. | 293 | | 58 | III. 204 | 0 38 54± | 71 19 40 | v F; R; follows a * 6.7 m 40° and is 1½′ n of it. It is near 2 v s st. If this be III. 204, my father's P D is 5′ wrong AR by working list. | 312 | | 59 | II. 609 | 0 38 55′4 | 63 18 17 | F; R; b M. A coarse D * precedes | 114 | | | | | 57′5 | p B; R; s b M; 15″ | 178 | | | | | 57′6 | v F; R; b M; 15″ | 392 | | | | | 57′7 | p B; R; p s b M; 20″ | 172 | | 60 | II. 611? | 0 39 3′4 | 63 18 6 | Not v F; R; b M; 15″. Query if not the same as II. 609 | 177 | | 61 | V. 1 | 0 39 11′7 | 116 12 55 | A v L, m E, v B neb. (See figure 52.) Observed also in sweep 292, but no place taken. | 306 | | 62 | II. 472 | 0 39 12′9 | 102 24 31 | v F; L; R; g b M; 30″ | 373 | | 63 | Nova. | 0 39 24′0 | 93 47 14 | e F, (through fog.) Makes obtuse-angled triangle with 2 st | 97 | | 64 | II. 621 | 0 39 24′4 | 93 42 32 | F; E; 30″1; barely seen through fog | 96 | | 65 | III. 153 | 0 40 36′2 | 58 39 26 | F; S; R; b M; has a * 8 m nearly s, 4 or 5′ dist | 104 | | | | | 36′4 | p B; p L; R; p s b M; has * 9 m, s f, dist 3′ | 100 | | | | | 37′0 | p B; E; b M; has * 7 m 3′5 f, 4′ s | 106 | | | | | 37′6 | p B; S; R; b M; a * 8 m to s, dist 5′ | 102 | | No. | Synonym. | AR 1830-0. | N.P.D. 1830-0. | Description and Remarks. | Sweep. | |-----|----------|------------|----------------|-------------------------|--------| | 66 | III. 463 | h m s | 96° 7′ 37″ | Very doubtful; ζ | 40 | | | | 0 41 28′8″ | | | | | | | | 31° 1′ | No description | 186 | | 67 | II. 446 | 0 42 2′5″ | 92 49 50 | Not v F; R; ps1b M; 30″; a * 8°9 m follows rather to s Δ | 371 | | | | | | AR = 5°5. | | | 68 | III. 955 | 0 42 7± | 99 35 1 | F; S; R. AR from my father's obs | 310 | | | | | | | | | | | | 36° 0 | v F; R; p g b M | 315 | | 69 | III. 429 | 0 42 25′7″ | 97 58 53 | A fine double neb; the preceding only seen by my father. | 186 | | | | | | | | | | | | | p B; S; s m b M. The f is v F; S; R; pos = 60° (30° n f); dist of centres 40″. The neb join at borders. | | | 70 | Nova. | 0 42 28′0″ | 97 59 13 | The prec p B; the foll v F. They form a double nebula, which is described by my father only as an extended single one. | 187 | | | | | | | | | 71 | I. 159 | 0 42 29′6″ | 43 22 6 | B; S; R; vg1b M; 20″. Approaching to planetary; makes a v obtuse-angled triangle with 2 st 10 m. | 390 | | 72 | III. 477 | 0 43 24′6″ | 66 34 36 | e F; R; has a * 15 m f dist = 30″ | 166 | | | | | | | | | | | | 35 51 ± | e F; S; has a * near | 172 | | 73 | III. 439 | 0 43 27′4″ | 93 9 5 | v F; S; R; b M; seen, but hardly discernible | 96 | | | | | | | | | | | | 28° 0 | Not e F; S; R; g b M | 97 | | 74 | VI. 20 | 0 43 50′7″ | 117 30 30 | (nisi AR = 44m 25°7.) A fine rich, not v comp L cluster | 292 | | 75 | Nova. | 0 44 14′9″ | 58 26 49 | e F; S; R. The faintest object imaginable; (night wonderfully clear.) | 106 | | 76 | Nova. | 0 47 25′7″ | 78 50 39 | A small cluster of p closely scattered stars | 15 | | 77 | Nova. | 0 47 53′2″ | 92 41 15 | p F; S; E; 15″ | 371 | | 78 | Nova. | 0 48 18′3″ | 60 38 30 | p B; R; g b M; 10″ | 178 | | | | | | | | | | | | 18° 8 | F; v S; R; b M; 6″ | 177 | | 79 | II. 210 | 0 48 33′4″ | 60 34 57 | p B; R; g b M; has * 9 m 45° s f, dist. 3′ | 114 | | | | | | | | | | | | 34° 3 | B; R; ps b M; 20″ | 178 | | | | | | | | | | | | 35° 3 | B; p L; g b M; 25″ | 177 | | 80 | II. 433 | 0 51 15′3″ | 98 29 36 | F; L; E; 50″. Sky not very clear | 186 | | | | | | | | | | | | 15° 4 | Not v F; L; E; gl b M; has * 10 m 20°5 f in the parallel. | 187 | | 81 | III. 191 | 0 53 32′0″ | 95° 9′ 41″ | v F; S | 96 | | | | | | | | | | | | 35° 9 | Precedes by 1m 37s a star 8.9 m; a * 10 m between | 97 | | 82 | II. 434 | 0 54 45′4″ | 97 15 35 | F; R; s b M, to * 13 m; 20″; a * 14 m 10° n f 20″ dist | 187 | | | | | | | | | | | | | F; S; r | 40 | | | | | | | | | | | | | p B; R; 20″; hazy | 186 | | 83 | Nova. | 0 55 54′8″ | 28 43 47 | A small cl 2′ in diam. Place that of the D * h 1070 whose AR in my 4th Catal is 2m wrong. | 219 | | 84 | II. 215 | 0 57 52′6″ | 58 23 50 | p B; R | 100 | | | | | | | | | | | | 54° 0 | p B; not v S; b M | 106 | | | | | | | | | | | | 54° 2 | F; R | 104 | | 85 | II. 216 | 0 57 54′6″ | 58 27 ± | p B; R | 100 | | | | | | | | | | | | 56° 0 | p B; S; s b M | 106 | | | | | | | | | | | | 56° 2 | F; p L; R; b M | 104 | | No. | Synonym | R 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 86 | II. 217 | h m s | 0 58 0'2 | F; R; b M; 5 or 6' s of II. 216 .................................. | 104 | | | | | | p B; R; P D requires an uncertain correction, being taken much out of the meridian. | | | 87 | II. 218 | 0 59 0'6 | 57 46 50 | p B; p L; g b M....................................................... | 106 | | 88 | I. 54 | 0 59 0'6 | 51 15 8 | p F; S; R; s b M. It is bright 3rd or F 2nd class (sky perfectly clear), and = * 14 m. One of a group of 5 or 6 st 15 m. | 188 | | 89 | II. 224 | 0 59 58'9| 55 12 6 | v F; v S; 1E; g b M; 10''. Allowing for the C &c. this cannot be a 1st class neb; no other near it. | 183 | | 90 | III. 154| 1 2 46'6 | 58 46 50 | B; R; g b M; 30''...................................................... | 105 | | 91 | III. 592| 1 4 9'2 | 91 12 44 | p B; R; p g b M; 30''.................................................. | 168 | | 92 | III. 593| 1 4 14'4 | 91 13 59 | p B; S; R; b M........................................................... | 102 | | 93 | II. 447 | 1 4 19'7 | 91 8 59 | v F; R; s b M............................................................ | 113 | | 94 | Nova. | 1 4 35'6 | 30 46 28 | No desc. Place estim from II. 447 .................................. | 113 | | 95 | Nova. | 1 4 36'4 | 57 11 26 | A star 8 m the chief of a small loose cluster........................ | 213 | | 96 | Nova. | 1 6 50'1 | 59 52 16 | F; S; v s b M............................................................. | 106 | | 97 | VII. 42 | 1 8 33'1 | 32 34 8 | v F; E; a * 9 m n p and a S * n f at the extremity of the nebula a D * 10 m, pos 324°5, dist 12'', in the midst of a p rich L cl which fills the field. The stars are 10 m; one of 7 and 1 of 8 m in the s f part. | 106 | | 98 | Nova. | 1 10 22'8| 58 11 27 | v F; e S; stellar...................................................... | 106 | | 99 | III. 250| 1 10 23'9| 87 34 48 | No description .................................................................. | 95 | | 100 | III. 577| 1 11 37'1| 50 23 49 | e F; S; R; v g l b M; 15''; C........................................ | 183 | | 101 | Nova. | 1 12 13'7| 83 52 32 | e F; p L; R; has a red * 7.8 m 45° s p.............................. | 118 | | 102 | III. 156| 1 12 25'5| 57 27 ± | v F; so that I had difficulty in finding it again when it had quitted the field. | 100 | | 103 | III. 252| 1 12 57'7| 85 37 58 | p B; L; R; b M; 30''.................................................... | 95 | | | | 58'2 | 37 51 | B; L; s v m b M, and losing itself imperceptibly; r in centre with 320; * 7 m in parallel 1m f. | 300 | | 104 | Nova. | 1 13 23'8| 57 42 47 | v F; E; has a D * to s .................................................. | 106 | | 105 | III. 594| 1 13 27'2| 89 56 36 | v F; L; E; pos by diag 60°0 ±; 1 b M; 90'' 1 .................... | 113 | | 106 | III. 158| 1 13 38'5| 57 26 20 | p B; p L; R; through fog............................................... | 102 | | | | 39'5 | 26 9 | p B; R; b M. N.B. nebulae numerous hereabouts .................... | 100 | | 107 | Nova. | 1 13 56'±| 57 46 ± | It precedes III. 159 by about 10', and is half a field to the south of it | 106 | | 108 | III. 159| 1 14 6'1 | 57 38 17 | p B; p L; b M .............................................................. | 106 | | | | 8'7 | 37 56 | e F; R ............................................................................. | 104 | | 109 | III. 160| 1 14 8'4 | 57 36 21 | v F; pos from III. 159 = 15°0; dist = 2'±.......................... | 106 | | 110 | Nova. | 1 14 26'9| 56 59 21 | v F; v S ............................................................................ | 105 | | 111 | III. 169| 1 14 53'5| 57 5 56 | F; S .................................................................................. | 105 | | 112 | II. 252 | 1 14 58'4| 77 59 19 | v L; irr R; v g l b M; by diagram at least 3' in diameter; a remarkable object. Is closely followed by the D * h 13; see fig 38. | 15 | | | | 63'0 | 57 57 | e F; L; R; 60''; has a * 9 m 20° s f, dist 100''. (N.B. This place and the former description to be preferred.) | 173 | | No. | Synonym | AR 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 113 | III. 167 | h m s | 1 15 4'5: | 57 26 5" | Precedes III. 168, and is 2' north | 102 | | 114 | III. 168 | | 1 15 8'0: | 57 28 5 | p B; R | 102 | | 115 | II. 461 | | 1 15 43'4 | 89 9 52 | B; p L; R; b M | 110 | | | | | 51'7 | 9 44 | v F; R; b M. This or the AR of sweep 110 mistaken 10° | 113 | | 116 | III. 253 | | 1 15 46'5 | 87 4 43 | p B; E like a comet, pos 135°0 ±; 60" 1 | 95 | | 117 | I. 151 | | 1 15 52'5 | 81 21 17 | v B; p L; R; p s m b M; 60"; 4 st near | 118 | | 118 | Nova. | | 1 16 3'2: | 56 10 58: | p B; v S; s b M. The preceding of two | 105 | | 119 | III. 556 | | 1 16 25± | 81 38 57 | Not v F; L; R; b M. 40". AR brought up from my father's obs not having been taken. | 118 | | 120 | III. 171 | | 1 16 43'2 | 56 11 28 | p B; p L; g b M; the following of two | 105 | | 121 | II. 462 | | 1 16 46'4 | 89 7 33 | Barely, but certainly seen; Ç | 108 | | | | | 47'8 | 7 30 | B; p L; R; b M | 110 | | 122 | II. 463 | | 1 17 59'2 | 88 52 9 | p F; R; p s b M; 30" | 113 | | | | | 62± | 52 27 | p B; S; E from p to f; b M; "has a granulated" (i.e. a resolvable) "appearance". | 110 | | 123 | III. 560 | | 1 18 0'4 | 53 41 53 | v F; E; v g l b M; near a * 13 m | 188 | | 124 | Nova. | | 1 18 12'2 | 28 35 19 | A fine rich cluster 5' diam; irreg fig; (windy) | 216 | | 125 | Nova. | | 1 19 29'1 | 58 33 21 | v F; S; R | 106 | | 126 | Σ. 131 | | 1 21 58'9 | 30 11 18 | A fine cl; R; rich; rather coarse; 6 or 8' diam; stars 10...11 m. One of Struve's "accvii". | 213 | | | | | 65'7 | 11 42 | The chief * in a cl VI or VII class 8' diam, which has one v red * near the middle; stars 9...12 m. | 219 | | 127 | Nova. | | 1 22 6'1 | 57 15 53 | v F; p L; g b M | 106 | | 128 | I. 100 | | 1 22 48'4 | 97 44 18 | B; R; p g m b M; 15...20" | 318 | | | | | 48'5 | 45 13 | B; R; g m b M; 60...90"; between clouds and in thick haze. Must be v B in clear weather. | 39 | | | | | 48'6 | 44 48 | v B; R; p s b M; 25". (Seen also sw 40, but no determination of the place obtained). | 186 | | 129 | Nova. | | 1 23 1'6 | 91 48 7 | v F; R; b M; 25" | 113 | | 130 | III. 431 | | 1 23 5'5 | 97 46 8 | v F; R; 15" | 318 | | 131 | V. 17 | | 1 24 15'6 | 60 13 9 | Enormously L; v g b M. The nucl taken; has * 12 m, n f the nucl. The diffused neb extends 15' s and as much nearly to n. It has irregularities of light, and even feeble subordinate nuclei and many small stars. Probably V. 17 is part of the diff neb of M 33. | 177 | | 132 | II. 4 | | 1 24 23'9 | 97 53 32 | p B; R; a * 6 m follows 47°5 and is 40" n. | 40 | | 133 | III. 150 | | 1 24 36'2 | 60 7 6 | v S; almost uniformly B. Place by rough comparison with the nucl of M 33, with which its pos = 51°1 Δ P D = 6' 3" ±. | 177 | | 134 | Nova. | | 1 25 41'6 | 57 13 29 | v F; p s b M. Stellar. | 106 | | 135 | III. 174 | | 1 26 11'1 | 57 11 34 | p F; p s b M. Stellar, or like a star blurred. | 106 | | 136 | Nova. | | 1 26 37'5 | 57 28 43 | p B; p L; b M; precedes a * 2m 51°0. | 102 | | 137 | II. 282 | | 1 26 48± | 98 12 0: | p B; R; is s f a * 8 m distant 10'. | 186 | | 138 | III. 454 | | 1 27 16'7 | 90 12 22 | v F; not v S; not b M | 110 | | | | | ... | 11 ± | The faintest thing imaginable | 113 | | No. | Synonym | AR 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 139 | I. 281 | h m s | 1 27 22·9 | v F; R; 1 b M; 20″. This is probably Mr. Dunlop's No. 479, but one or the other AR requires correction. | 292 | | 140 | III. 471| 1 27 26·1 | 100 52 50 | e F; S; among 2 or 3 v F st very difficult .................. | 315 | | 141 | Nova. | 1 27 27± | 57 17 ± | v F; R; another precedes, which must be III. 174. The AR conjectural, and P D liable to some error. | 100 | | 142 | M. 74 | 1 27 34·8 | 75 4 46 | e F; 5′ with a brighter mass = 1′ in centre, and this again p s b M to a suspected *. Several v s st near. | 319 | | | | 34·8 | 5 17 | B; L; R; p g m b M; 90″ diam; resolvable .................. | 173 | | 143 | Nova. | 1 28 26·0 | 84 59 29 | p B; S; R; p s b M; 15″ .................................. | 300 | | 144 | II. 283 | 1 30 36·9 | 98 22 33 | F; v S; R; v g b M; 10″ .................................. | 318 | | | | 38·6 | 22 18 | p F; S; R; p s b M; 20″ .................................. | 186 | | 145 | VII. 46 | 1 32 25·9 | 28 58 17 | A cluster of the 6th class, (i.e. very rich) ................. | 219 | | | | 26·3 | 58 44 | A fine rich cl; st 11...14 m; 3′ diam; irreg fig; place that of the most comp part; one star 6·7 m, s f the centre, is ruddy. | 216 | | 146 | Nova. | 1 32 45·9 | 34 59 2 | A D *(2070), the chief of a p rich loose cl; st 12 m....... | 386 | | 147 | II. 610 | 1 34 42·8 | 62 9 6 | p F; S; R; p s b M ........................................ | 177 | | | | ... | 10 ± | F; v S; R .................................................. | 181 | | 148 | Nova. | 1 34 57·6 | 86 37 45 | v F; R; 20″ ................................................ | 300 | | 149 | II. 611 | 1 37 51·3 | 62 58 15 | v F; R; 15″ ................................................ | 392 | | | | 53·0 | 57 51 | not v F; S; E nearly in Mer; 15″ C; 10″ br ................ | 177 | | 150 | I. 157 | 1 38 19·4 | 63 25 20 | Between two stars ............................................ | 181 | | | | 20·6 | 25 40 | e F; 1 E; sky not perfectly clear. Taken while looking for Encke's comet. | 392 | | | | ... | 25 30 | p F; E; v g l b M; pos n f to s p; between two stars; 6′1; 3 or 4′br | 178 | | 151 | IV. 42 | 1 40 4·0 | 84 56 15 | A * 9 m with a v F neb ray. A * 17 m p .................... | 95 | | | | 4·2 | 56 16 | A * 9 m with a v F narrow ray of neb; a most curious object. See fig 58. | 300 | | 152 | II. 612 | 1 40 22± | 63 12 35 | v F; R; near a * 15 m. AR per working list .................. | 392 | | 153 | Nova. | 1 40 42± | 79 9 19 | e F; AR may be a whole minute wrong ....................... | 15 | | 154 | II. 501 | 1 40 51·0 | 105 48 56 | v F; R; v g b M; 15″ ...................................... | 307 | | 155 | III. 459| 1 40 57·7 | 114 38 19 : | v F; R; g b M; 15″ a * 8 m, s p. (N.B. Both this P D and that of sw 292 are open to much error.) | 306 | | | | 59·4 | 40 37 : | v F; R; makes obtuse triangle with 2 st 8 and 9 m nearly in merid and 6′ asunder. | 292 | | 156 | II. 859 | 1 41 37·0 | 84 42 7 | p B; E; v g b M; a * 10 m, n f ............................ | 300 | | 157 | III. 562| 1 42 42·4 | 54 40 58 | v F; the n p of two, dist 90″ ± ........................... | 105 | | 158 | III. 192| 1 42 45·0 | 94 53 48 | e F; 90″ n of a * 11.12 m ................................ | 96 | | | | 47·6 | 53 38 | e F; 1 E in Mer; has * 14 m 90″ s ........................ | 97 | | | | ... | 54 24 | e F; R; the transit missed ................................ | 39 | | 159 | III. 563| 1 42 49·4 | 54 42 1 | p B; p L; 1 b M; 40″ ...................................... | 105 | | 160 | I. 62 | 1 42 54± | 100 32 56 | v F; R; v g v l b M. Aurora in sky even so far south, strong enough to illuminate the field of view and render the wires visible without a lamp. | 310 | | 161 | II. 596 | 1 42 56·8 | 84 33 17 | p B; 30″; a * 13 m 1 radius of neb dist from edge .......... | 300 | | No. | Synonym. | AR 1830°-0 | N.P.D. 1830°-0 | Description and Remarks | Sweep | |-----|----------|------------|----------------|------------------------|-------| | 162 | 55Androm.| h m s 1 43 8'6 | 50 6" 40 | 55 Androm. A fine nebulous * with a strong atmosphere losing itself imperceptibly; diam 90". It is also a double *h 1094; called "nebulosa" by Piazzi. | 183 | | 163 | Nova. | 1 43 10'9 | 54 1 18 | vF; R; among several p B stars | 188 | | 164 | II. 270 | 1 44 22'9 | 86 38 10 | pB; R; psmbM; 30" | 95 | | | | 24'4 | 38 32 | B; R; psbM; 25" | 300 | | 165 | I. 105 | 1 44 44'7 | 104 34 27 | vB; E; psmbM; 40" l; 30" br. | 308 | | 166 | III. 460 | 1 45 49'8 | 114 35 22 | not vF; R; vg bM; 30"; has a * 13 m. 90", s | 306 | | 167 | Nova. | 1 45 50'7 | 114 42 17 | vF; pL; R; gbM; has a small * 75° sp. It is barely possible that this may be III. 460 with a mistake in reading the P D. | 292 | | 168 | Nova. | 1 46 14'6 | 86 38 10 | A suspected nebula. | 95 | | 169 | II. 221 | 1 46 49'9 | 57 48 1 | pB; has a S * or stellar neb to the n. | 106 | | | | 50'1 | 47 38 | pB; R; bM; has * 13 m np | 100 | | | | 50'1 | 47 45 | F; R; has a * near it | 102 | | 170 | Nova. | 1 47 2'5 | 30 39 43 | AD * in the f part of a L, poor, triangular cl of 15 or 20 st 10...13 m. | 213 | | 171 | Nova. | 1 47 9'0 | 35 22 7 | p rich, irreg figl cluster of *s 11...13 m 8' diam | 386 | | 172 | II. 271 | 1 47 29'0 | 85 12 23 | The prec and brightest of a fine double nebula; p F; R; psb M; 20"; pos of the other = 102°4. | 300 | | 173 | II. 272 | 1 47 29'4 | 85 12 35 | The f and fainter of a double neb; vF; R; sbM; 12".... | 95 | | 174 | VII. 32 | 1 47 39'6 | 53 10 8 | An enormously L, p rich, sc cluster. Place that of a conspicuous *. The densest part is 10' n. | 188 | | 175 | II. 222 | 1 47 43'6 | 57 38 35 | pL; E; precedes a p B * by 18°0 | 102 | | | | ... | 40 ± | pB; R; AR not taken; PD rough | 100 | | 176 | III. 193 | 1 47 48'9 | 95 18 9 | eF; is 45° sf a * 9 m; Δ AR = 6°0 | 96 | | | | 51'0 | 18 5 | eF; 45° sf a *; Δ AR = 6°25 | 97 | | 177 | III. 265 | 1 48 10± | 99 51 56 | F; S; R. Transit missed; PD imperfect. | 310 | | 178 | III. 464 | 1 48 25'6 | 96 14 0 | eF | 39 | | | | 26'1 | 14 18 | F; 1E; vg bM | 318 | | 179 | 50Cassiopeia | 1 49 6'2 | 18 24 27 | I suspect this star to be nebulous | 378 | | 180 | Nova. | 1 49 43'1 | 82 29 4 | vF; S; R; 15...20"; a * 10 m 15° n p; 2' dist | 118 | | 181 | I. 112 | 1 49 59'5 | 71 49 6 | pB; R; gbM; 40" | 319 | | | | 61'6 | 49 0 | L; R; through thick cloud. Obs so doubtful that but for the agreement of the transits over both wires I should not have believed I saw it. | 312 | | 182 | II. 233 | 1 50 26'5 | 59 23 53 | B; R; gbM; 40"; a considerable neb. | 106 | | 183 | I. 101 | 1 51 8'6 | 96 47 47 | B; E; bM | 39 | | | | 11'2 | 46 28 | pB; pL; E; pos about 160° by diag | 40 | | | | 11'9 | 47 28 | pB; mE; pos = 163°0; bM to nucleus | 318 | | 184 | III. 583 | 1 51 10'1 | 62 35 18 | eF; 3 st in Mer precede it; the largest 10 m is 20° sp the neb | 177 | | 185 | II. 435 | 1 52 43± | 97 39 10 | B; pL; R; bM. Transit missed; AR by working list. Also observed sw 40, but no descrip, and place only roughly set down. | 39 | | 186 | III. 433 | 1 52 50'4 | 96 11 53 | F; pL; R; bM; 25" | 318 | | | | ... | 13 + | No descrip; taken much past merid. | 39 | | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 187 | Nova. | 1 53 2·0 | 75 6 22 | e F; S; R; has a * 11 m 15° n f. | 173 | | 188 | III. 207| 1 53 10·8| 72 26 41 | F; S; R; g l b M; 12" | 319 | | 189 | III. 566| 1 53 21·4| 52 42 38 | v F; R; s b M; near a * | 188 | | 190 | III. 208| 1 54 31·1| 74 46 46 | v F; not v S; g l b M; follows * 10 m 3·5 | 319 | | 191 | III. 151| 1 55 12·1| 61 49 31 | v F; v S; 6"; has * 12 m, 1' n, and another about 20° s p | 177 | | 192 | Nova. | 1 56 3·7 | 114 6 42 | v F; R; v g b M; 40" | 306 | | 193 | I. 152 | 1 58 15·3| 79 49 27 | Not v B; R; s b M to nucl; has * 10 m s p, dist 55". P D by obs 78, but no doubt should be 79. | 121 | | 194 | II. 604 | 1 58 30·9| 52 3 1 | p B; E | 188 | | 195 | Nova. | 1 59 12·5| 76 27 37 | F; R; b M; 15" | 173 | | 196 | Nova. | 1 59 34·5| 116 15 37 | A v F double * inclosed in a v F neb | 306 | | 197 | II. 605 | 1 59 51·8| 51 37 31 | p B; R; g b M; 25"; has a D * 15° foll | 188 | | 198 | III. 227| 1 59 59·2| 82 50 22 | v F; R; b M; 20" | 118 | | 199 | II. 482 | 2 1 1·6 | 100 56 10 | v S; R; the first of a group of 4 | 315 | | | | | 1 1·7 | F; S; R; the first of 4 in a crooked line | 310 | | 200 | II. 483 | 2 1 4·6 | 100 56 25 | The 2nd of 4. It makes a double neb with the first | 315 | | | | | 5·2 | F; S; R; the second of 4 in a crooked line | 310 | | 201 | II. 484 | 2 1 19·5 | 100 57 6 | F; S; R; the third of 4 | 310 | | | | | 19·6 | The third in order and in size | 315 | | 202 | II. 485 | 2 1 23·5 | 100 59 56 | F; S; R; the last and largest of 4 | 310 | | | | | ... | Seen. Place estimated by the others | 315 | | 203 | Nova. | 2 1 25·9 | 98 33 43 | v F; R; p s b M; 12" | 318 | | 204 | III. 604| 2 2 8·9 | 53 19 30 | v F; irreg fig | 188 | | 205 | III. 260| 2 5 52·7 | 91 33 11 | v F; R; b M | 108 | | 206 | III. 457| 2 6 32·2 | 84 48 1 | e F; R; attached to and n p a * 11,12 m. Clouded before it could be fully verified. | 300 | | 207 | VI. 33 | 2 7 8·2 | 33 37 3 | The splendid cl in Perseus. A most noble group. Much more than fills field. 2 st 7 m, the rest 8...14; one of 7 m taken, at the circumf of an ellipse of stars. | 213 | | | | | 12·4 | v superb cl. Has 2 st 8m, the rest 11...13. Fills the field and has many stragglers. In centre is the D * h 1114 and an ellipse of stars. | 387 | | 208 | III. 201| 2 7 55·5 | 76 14 19 | v F; E; has a * 10 m 4' s f | 173 | | 209 | II. 474 | 2 8 14·2 | 102 8 57 | F; R; fog thick. (N.B. The obs makes P D 104°, which must be a mistake.) | 308 | | | | | 16·7 | p F; p L; R; v g b M; 60"; by a strange conflict of errors this obs makes the P D 101°. Both are obviously wrong. | 310 | | 210 | II. 246 | 2 8 45·0 | 76 14 37 | p B; R; p g b M; a small * s f; dist 1' and a * 9 m 5' dist nearly s, a little foll. | 173 | | 211 | II. 436 | 2 9 45·1 | 97 25 49 | e F; b M; hardly visible (cloudy) | 39 | | 212 | VI. 34 | 2 10 0·7 | 33 37 13 | A noble cluster which just fills the field. It is the following of the two great clusters in Perseus; loose, but more condensed in middle. The borders graduate away. | 213 | | | | | 28·6 | A fine cl; v L; the foll of two clusters which are quite separate. A fine ruby * in the centre. | 387 | MDCCCXXXIII. | No. | Synonym | RA 1880°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|---------|-------------|----------------|------------------------|-------| | 213 | Nova. | 2 10 21·1 | 74 57′ 21″ | e F; R; g b M; 12″; near a * 16 m | 319 | | 214 | Nova. | 2 10 30·5 | 27 0 42 | A coarse straggling cl; not v rich; 10 or 12′ diam. Stars 9...13 | 221 | | 215 | II. 437 | 2 10 37·9 | 97 34 28 | p B; R; g b M; 15″; a coarse D * in field | 318 | | | | | 40·9 | F; R; b M | 40 | | 216 | III. 486| 2 11 28·7 | 106 50 26 | p B; R; p g b M; 25″ | 307 | | 217 | II. 225 | 2 11 53·0 | 57 31 40 | p B; R; b M; 25″; bad fog | 102 | | | | | 54·7 | B; R; p s b M | 106 | | | | | 55·2 | p B (in spite of a fog); R; b M; 3 small st in a curve to s p | 104 | | | | | 56·5 | p B; R; g b M; has 3 or 4 S st p in a curve | 100 | | 218 | V. 19 | 2 11 58·3 | 48 25 8 | An extr F ray 3′ or 4′ 1; 40″ br. Pos with mer = 23°·5 bad meas, the neb being too F to illuminate the wires. | 389 | | | | | 30 ± | Place hardly more than conjectural, being too late to get it on merid; v L; vm E; p F; has a chink or dark division in the middle and two stars. Pos with merid 21°·2. A wonderful object. See fig 28. | 182 | | 219 | II. 438 | 2 13 5·9 | 96 18 28 | v F; v L; R; v g l b M; 90″ | 318 | | | | | 20 ± | F; v L; b M; viewed much out of meridian | 39 | | 220 | Nova. | 2 16 4·3 | 58 31 48 | v F; S; R; forms a semicircle with 4 st | 106 | | 221 | Nova. | 2 16 9·8 | 72 16 1 | p F; L; R; 60″; n p a * 10 m dist, 3′ | 319 | | 222 | III. 177| 2 17 8·2 | 57 11 46 | v F; E; two st 13 m n p near | 104 | | | | | 9·1 | p B; L; E; v g b M; among stars | 100 | | 223 | IV. 23 | 2 18 57·6 | 91 54 29 | v B; v L; R; p s m b M; 2′ diam; fades away insensibly | 108 | | 224 | III. 261| 2 19 50·0 | 91 55 46: | v F; L; R | 108 | | 225 | II. 487 | 2 20 18·9 | 101 18 25 | v F; cloudy. Doubtful obs | 315 | | 226 | I. 154 | 2 20 29·0 | 53 37 59 | B; E in merid; g b M; 30″ long | 188 | | 227 | Nova. | 2 21 20·3 | 33 13 52 | A p rich, p L, cl; st 13...15 m; not comp at the centre. Fig an irregular parallelogram. | 387 | | 228 | Nova. | 2 21 32·4 | 46 7 43 | p rich cl; 2 or 3 B and about 20 st 13...15 m; a star 9 m taken | 389 | | 229 | II. 278 | 2 21 53·1 | 91 51 16 | p B; S; E; b M | 108 | | | | | 51 ± | p B; S; E; p s b M | 113 | | 230 | II. 237 | 2 22 8·1 | 93 42 2 | p B; R; or irreg fig; b M | 96 | | 231 | Nova. | 2 23 56·8 | 57 48 47 | S; R; p s b M. The first of 3 | 106 | | 232 | II. 211 | 2 24 2± | 61 25 ± | p B; 1 E; p g b M. AR from working list; PD uncertain | 178 | | 233 | Nova. | 2 24 13·3 | 57 48 17: | v F; R; b M. The second of 3 | 106 | | 234 | Nova. | 2 24 33·8 | 57 54 25: | p B; R. Place by rough comparison with the first of the three | 106 | | 235 | III. 572| 2 24 40·5 | 49 55 25: | v F; S; the preceding of two. Dist 3′; pos from the next = 337°·0. | 182 | | 236 | III. 573| 2 24 44·8 | 49 52 39 | p F; S; 1 E | 182 | | 237 | III. 161| 2 26 33·8 | 57 25 11 | v F; R; S; b M; 2 st 14 m n p point to it | 104 | | | | | 36·6 | p F; R; S; p s b M | 100 | | 238 | III. 557| 2 27 6·8 | 79 6 32 | p B; R; p s b M; 25″; Ω | 121 | | 239 | III. 434| 2 27 17·3 | 97 54 28 | e F | 318 | | No. | Synonym | AR 1830° | N.P.D. 1830° | Description and Remarks | Sweep. | |-----|---------|----------|-------------|------------------------|-------| | 240 | II. 238 | 2 28 32'1 | 49 51 49 | p F; p L; 1 E .......... | 182 | | 241 | III. 152 | 2 29 10'4 | 60 35 40 | p B; irreg R; b M; 18'' r. AR doubtful .............. | 178 | | 242 | I. 156 | 2 29 46'4 | 51 40 39 | v B; v m E; vs m b M, to a *. Lenticular; 5' long; pos by diagram 20° n f to s p. See fig 56. | 188 | | 243 | II. 592 | 2 30 1'8 | 79 53 40 | F; R; b M; 20''; has * 11 m 40° n f; 25'' dist .......... | 121 | | 244 | I. 102 | 2 30 4'3 | 97 25 40 | p b; p L; irreg R; 2' diam; r ......................... | 38 | | | | | 7'2 | 25 33 | No description ........................................ | 39 | | | | | 9'5 | 24 23 | No description ........................................ | 40 | | 245 | III. 581 | 2 30 22'2:: | 72 42 1 :: | Doubtful obs. Clouded .................................. | 319 | | 246 | II. 5 | 2 30 37'3 | 89 37 46 | p F; R; b M; forms a trapezium with 3 st ............... | 108 | | | | | 41'2 | 38 49 | B; R; S; 1 E; forms a trapez &c. ....................... | 113 | | 247 | III. 475 | 2 31 1'± | 71 27 30 | F; R; 1 b M; 15''. AR by working list .................. | 314 | | 248 | M. 34 | 2 31 6'1 | 47 56 43 | Fine cluster; about 20 st 9 10...11 m and as many less. Fills field, coarsely scattered. Place that of a D (h 1123). | 389 | | | | | 8'7 | 57 50 | Poor; coarse; very badly seen through haze ............ | 190 | | 249 | II. 284 | 2 31 7'4 | 98 52 13 | p B; m E; has a * 17 m at the s f end .................. | 318 | | | | | ... | 52 36 | No description ........................................ | 310 | | 250 | Nova. Polarissima. | 2 32 0 | 0 5 10 | v F; R; g b M; 25''; has a * 11 m 2' s. This nebula is remarkable for its proximity to the pole. Owing to this the AR cannot be determined exactly, and the P D is open to correction. | 374 | | 251 | III. 228 | 2 32 0'5 | 81 59 57 | v F; the p of two; a * 10 m, p in same line ............ | 118 | | 252 | III. 229 | 2 32 8'0 | 82 1 12 | e F; the f of two ..................................... | 118 | | 253 | II. 488 | 2 32 14'7 | 102 1 22 | F; R; b M; 20''; fog .................................. | 308 | | 254 | I. 63 | 2 32 41'3: | 98 59 36 | B; irreg R; p g b M; r ................................ | 310 | | | | | 44'9 | 58 38 | B; S; R; 20''; g b and p s m b M to * 12 m ............ | 318 | | 255 | II. 633 | 2 32 48'9 | 53 24 9 | p F; L; R; g l b M; 50'' ................................ | 188 | | 256 | III. 584 | 2 32 49'4:: | 62 9 5 | p B; S; R; p s b M; 12''. AR precarious ............... | 178 | | 257 | III. 162 | 2 33 0'7 | 58 17 41 | p L; R; has a red * 7.8 m 43''5 p; fog. A p good obs however in AR. | 104 | | | | | 1'8 | 18 32 | p B; p L; b M ....................................... | 106 | | | | | 3'1: | 20 ± | F; S; R. (Place not to be depended on) ................ | 100 | | 258 | I. 1 | 2 33 2'4 | 90 16 36 | F; L; E; a p B * near .................................. | 108 | | | | | 3'6 | 17 29 | F; p L; E 10° n f to s p; 2' long ...................... | 113 | | 259 | Nova. | 2 33 4'4 | 72 43 15 | e F; hardly sure ..................................... | 395 | | 260 | III. 163 | 2 33 35'7 | 58 15 22 | v F; p L. The s p of two ................................ | 106 | | 261 | Nova. | 2 33 38'2 | 58 12 22: | e F; S; the n f of two. Δ P D estim at 3' .............. | 106 | | 262 | M. 77 | 2 33 58'2 | 90 43 43 | v B; not v L; R; p s b M; has * 2' dist 40° s f ....... | 108 | | 263 | II. 273 | 2 34 26'2 | 85 45 5 | p B; R; g b M; 15'' .................................. | 95 | | 264 | I. 64 | 2 37 38'4 | 98 17 33 | v B; L; E; 100'' 1; 40'' br; v g l b M ............... | 318 | | 265 | II. 466 | 2 37 43'7 | 91 13 34 | F; p L; b M ....................................... | 107 | | 266 | II. 465 | 2 37 49'3 | 90 56 46 | e F .................................................. | 108 | | 267 | III. 462 | 2 38 46'6 | 90 58 36 | e F; R; is pointed to by 2 st n a l p the neb .......... | 108 | 3 c 2 | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|--------------------------|-------| | 268 | Nova. | h m s | 2 40 43·8 | Query whether a nebula or a knot of minute stars indistinctly seen. | 182 | | 269 | III. 449| 2 41 11·9 | 107 41 16 | p B; p L; R; g b M; 40" .................................................. | 307 | | 270 | II. 601 | 2 41 48·8 | 48 29 54 | v F; R; v g b M; 23" .......................................................... | 182 | | 271 | II. 602 | 2 43 30·3 | 49 7 32 | v F; R; v g l b M; 30" ...................................................... | 182 | | 272 | III. 450| 2 43 44·9 | 107 20 21 | v F; S; R; g b M; 15" ....................................................... | 307 | | 273 | Nova. | 2 44 13·1 | 91 58 54 | e F; p L; g b M; has * 8 m f ............................................. | 107 | | 274 | III. 580| 2 45 32·7 | 47 38 48 | v F; v S; R; g b M; 10"; makes isosc triangle with 2 st 15 m | 389 | | 275 | II. 470 | 2 46 19·7 | 100 43 26 | p B; S; R; nearly stellar .................................................. | 310 | | 276 | II. 274 | 2 49 19·3 | 87 18 28 | F; S; R; s b M; 12" ........................................................... | 95 | | 277 | II. 239?| 2 49 56·2 | 45 47 43 | F; R; g b M; 20"; follows the D * h 2167, 6°·5 ......................... | 389 | | 278 | Nova. | 2 50 54·1 | 48 5 59 | e F; S; 5" ............................................................................ | 182 | | 279 | II. 620 | 2 52 7± | 44 18 ± | v F; irreg fig. Suspected to be only a few stars. AR from working list; P D approx. | 390 | | 280 | II. 502 | 2 53 35·7 | 105 30 21 | p B; p L; R; p s b M; 40" .................................................... | 307 | | 281 | IV. 43 | 2 54 22·3 | 47 50 43 | A star 14 m with some kind of faint nebulous appendage ................. | 389 | | 282 | II. 503 | 2 55 41·7 | 106 16 8 | B; R; s b M; 40" ..................................................................... | 307 | | 283 | I. 109 | 2 56 45·6 | 116 42 53 | B; R; p s b M; 30". My obs makes the P D 115°, but this must be a mistake, as my father has three observations agreeing in 116. | 306 | | 284 | III. 578| 2 57 25·4 | 52 16 29 | F; v S; R; p s b M; 12" ....................................................... | 188 | | 285 | II. 285 | 2 57 57·3 | 100 12 5 | p B; irreg R; p s b M; 20" ................................................... | 315 | | 286 | II. 504 | 2 58 6·2 | 106 15 44 | Not v F; S; R; v g v l b M .................................................. | 310 | | 287 | Nova. | 2 59 19·1 | 37 18 57 | v B; E; p s b M; 30" l; 20" br ............................................. | 307 | | 288 | III. 262| 3 2 59± | 93 12 ± | A v S, close-packed group of 8 or 10 st 14...15 m in a space of 30" diam, so as easily to be taken for a p B nebula. | 386 | | 289 | II. 286 | 3 2 58·7 | 99 34 35 | Scarcely seen through thick haze. AR per working list; P D approx | 96 | | 290 | VI. 25 | 3 3 3·1 | 43 24 16 | e F; R; a B * 9 m n p .......................................................... | 315 | | 291 | III. 591| 3 3 8·7 | 99 36 50 | p B; R; night hazy and bad .................................................. | 310 | | 292 | Nova. | 3 4 18·8 | 95 52 21 | A rich, L, cl not v comp; irreg R with stragglers; stars 12...15 m; brightest part 5' diam. The middle taken. | 390 | | 293 | II. 603 | 3 8 34·6 | 49 6 49 | e F; v S ............................................................................... | 315 | | 294 | III. 574| 3 10 25·8 | 49 18 22 | F; S; 1E; has a * 9 m 5' dist nearly n .................................. | 39 | | 295 | III. 575| 3 10 26·9 | 49 16 44 | v F; S; E; b M; 15" long .................................................... | 38 | | 296 | II. 287 | 3 11 43·3 | 96 52 0 | F; R; b M .............................................................................. | 40 | | | | | | p B; b M; r; 60" ................................................................... | 38 | | | | | | v F; R; g b M; 12" .................................................................. | 318 | | | | | | v F; R; S .............................................................................. | 39 | | | | | | F; R .................................................................................... | 40 | | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 297 | III. 196 | 3 16 16± | 93 37 ± | The northern of two in same merid | 96 | | 298 | III. 197 | 3 16 16± | 93 39 ± | The southern of two. Δ P D = 2¼ | 96 | | 299 | III. 445 | 3 16 33:8 | 96 20 0: | e F; irreg fig; scarcely discernible | 38 | | | | 37:4 | 21 18 | v F; p m E; 20'' l, 12 br | 318 | | 300 | III. 694 | 3 19 42:9:: | 18 0 23 | No description | 380 | | | | 47:4 | 0 52 | F; R; g b M; 15''. Close to the D * h 2190 | 378 | | 301 | VIII. 88 | 3 20 45:4 | 53 15 56 | The chief * (10 m) of a cl of about 60 st which fills the field of view. | 188 | | 302 | III. 446? | 3 25 14:8 | 95 39 48 | v F; between a * p and a D * f | 96 | | | | 15:6 | 39 31 | No description. Clouded before obs could be completed | 40 | | 303 | II. 288 | 3 28 36:1 | 95 35 40: | v F; L; R; 3' | 38 | | | | 39:7 | 36 28 | L; the faintest thing imaginable | 96 | | 304 | III. 263 | 3 32 42± | 91 50 ± | No desc. R from working list; P D approximate | 107 | | 305 | III. 569 | 3 33 3:0 | 95 13 ± | No desc. The first of 3 | 96 | | 306 | II. 455 | 3 33 12:2 | 95 14 46: | R; n p a *. The second of 3 | 96 | | 307 | II. 456 | 3 33 31:7 | 95 17 ± | P D very doubtful | 96 | | | | 33:0 | 15 33 | p B; S; seen between clouds; has a B * 1' dist, 45° s f | 39 | | | | 34:4 | 15 46: | F; S | 38 | | 308 | VIII. 80 | 3 36 36:1 | 37 52 0 | A cl of about 20 st; place that of a superb D * (Σ 446); the rest 12 m. | 384 | | | | 38:5 | 52 7 | A D * Σ 446; the chief of a cl of 30 st more or less; 14...16m... | 386 | | 309 | I. 155 | 3 38 2:7 | 94 30 22 | e F; R; has a * 17 m in middle | 233 | | 310 | Nova. | 3 51 30:9 | 37 50 57 | A curious knot of stars forming a cluster in form the segment of an elliptic ring. | 384 | | 311 | IV. 69 | 3 58 35:8 | 59 40 46 | A * 9 m with a dilute, F, equable nebuluous atmosphere 60'' or 90'' diam. Other st 9 m have no such atm. A * susp n p. See Fig 31. | 56 | | | | 36:0 | 40 10 | A * 8 m with a fine atmosphere; diam 12° of time; perfectly nebuluous and fading away to nothing; a F * following; strongly suspected to have a slight chevelure, but several 8 m near, not the least. | 106 | | 312 | Nova. | 4 9 47:0 | 53 30 21 | The chief * of a v loose poor cluster 30' diam; 1 comp; stars 10...12 m. | 399 | | 313 | III. 490 | 4 11 37:9 | 91 6 54 | F; v S; a * 11 m s p | 110 | | | | 39:7 | 6 36 | F; p L; v g b M | 107 | | 314 | III. 587 | 4 17 54:6 | 94 1 12 | e F; among small stars | 233 | | 315 | I. 217 | 4 19 4:4 | 55 6 32 | B; visible in full ζ light; a * 9 m dist 3', 80° s p (afterwards corrected to n p. See Sw. 51). | 42 | | | | 5:2 | 6 48 | Place only taken. No descr. This obs makes the R 18 m, but this is an obvious mistake. | 50 | | | | 5:4 | 6 21 | p B; v L; irr R; it is inclosed among 6 stars, two of which point across its centre to a third. A * 7 m precedes about 1 m. | 105 | | | | ... | ... | A * 9 m is about 75° n p, not s p as in Sw. 42, and 2' dist .. | 51 | | 316 | II. 8 | 4 21 56:7 | 89 43 18 | The s p of a double nebula; R; p L; distance of centres 60''.. | 107 | | No. | Synonym | AR 1830°-0 | N.P.D. 1830°-0 | Description and Remarks | Sweep | |-----|---------|-------------|----------------|------------------------|-------| | 317 | II. 9 | h m s | 4 22 0'2 | The n f of the double nebula; F; S; R. Pos by a drawing made at the time 30°..40° n f. | 107 | | 318 | II. 7 | | 4 22 0'9 | p B; b M; E from s f to n p; has *50° n f, 1' dist; its situation is nearly at right angles to the longer axis of the nebula. | 110 | | | | | | p F; R; p L; has a *45° n f, dist 90''................................. | 107 | | 319 | I. 158 | | 4 23 14'8: | F; R; b M; 40''....................................................... | 38 | | | | | | F; R; b M; cloudy .................................................... | 39 | | | | | | p B; R; b M; 18...20''.................................................. | 233 | | | | | | p B; R; g b M; 15''; sky perfectly clear.............................. | 232 | | 320 | II. 524 | | 4 27 36'8 | No description; observation marked as doubtful ..................... | 109 | | 321 | II. 514 | | 4 27 52'2 | v F; p L; irreg fig; 90''; has a coarse B double star n f........... | 107 | | | | | | v F; L; m E; 3' L; 90'' br; v l b M. PD merely estimated by means of a star near it. | 110 | | 322 | Nova. | | 4 28 38'0 | v F; E; 45° n t s f; s b M; follows v Eridani 41°0 .................. | 109 | | 323 | III. 952| | 4 30 58'0 | The n p of a double neb; F; has a *8 m s p. Pos of the nebula about 65° s f by diagram. | 119 | | | | | | e F; p L; E towards the s f side, and has either a * or a second nucl s f. | 118 | | 324 | III. 953| | 4 30 59'7 | The s f nebula of the double neb .................................... | 119 | | 325 | II. 515 | | 4 31 29'7 | v F; R; has a *9 m about 12°5 f to the n ................................ | 107 | | 326 | II. 522 | | 4 32 31'8 | e F; R; v g b M; 30'' .................................................. | 315 | | | | | | No AR observed; no description....................................... | 318 | | 327 | I. 122 | | 4 32 55'7 | B; v L; R; b M; 2' diam ............................................... | 109 | | | | | | p F; L; nearly R; v g b M; 2' diam .................................. | 233 | | 328 | III. 588| | 4 35 23'1 | e F; irr R; b M; 10''.................................................. | 232 | | 329 | II. 523 | | 4 36 15'0 | p F; R; has a *7 m, 3 or 4' dist n p .................................. | 318 | | 330 | Nova. | | 4 37 32'3 | e F; irreg fig, if not a double or triple star, seen indistinctly .. | 232 | | 331 | III. 589| | 4 38 7'8 | p F; v S; v l b M; 15''................................................ | 233 | | 332 | VII. 1 | | 4 39 5'6 | A cluster of stars 11 and 12 m, three L and 5 small stars. Query if the right object. | 121 | | 333 | II. 457 | | 4 39 55'3 | v F; p L; R ............................................................... | 233 | | 334 | II. 527 | | 4 44 1'8 | p B; R; b M; has a *7 m 45° s p; very well observed.................. | 109 | | | | | | p F; S; R; 12''; has a *9 m dist 5' s p ................................ | 233 | | 335 | III. 453| | 4 45 33'6 | e F; among v S stars; has one v L * s p ................................ | 322 | | 336 | IV. 32 | | 4 48 33'1 | p B; R; like two or three stars 19 m with an atmosphere 60'' diameter. | 233 | | 337 | Nova. | | 4 49 9'8 | v Loose; p Rich; fills field; the largest *10 m; mixed magnitudes | 327 | | 338 | Nova. | | 4 49 38'0 | A resolved nebula or a small round group of very small stars, 30'' diam. | 118 | | 339 | Nova. | | 4 50 15'3 | F; S; R; b M ............................................................... | 110 | | | | | | F; R; b M; the preceding of two....................................... | 107 | | 340 | Nova. | | 4 50 47'± | p B; R; p s b M; has a B * n f; the fol of 2.......................... | 107 | | 341 | Nova. | | 4 51 30'4 | F; R; about 30'' n of a *13 m......................................... | 318 | | 342 | III. 503?| | 4 53 28'4 | e F; S; 4''; has a *12 m n f .......................................... | 233 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|--------------------------|-------| | 343 | Nova? | h m s | 94 58 20 | A very large space affected with nebulous streams in zigzags up and down. (N.B. Such observations require several verifications. The opportunity has not occurred in this case.) | 235 | | 344 | VIII. 61| 4 56 34·5 | 52 50 56 | A double * in a pretty close cluster of 20 or 30 stars. | 399 | | 345 | III. 500| 4 57 11·7 | 99 23 20 | not vF; R; g p m b M; 25" | 315 | | | | 13·4 | 22 53 | p F; S; R | 318 | | 346 | Nova. | 4 57 50·9 | 38 9 40 | A group of 8 or 9 stars 10 m, nearly in a parallelogram. A pretty object. | 327 | | 347 | V. 32 | 4 58 24·0 | 93 34 22 | A * 10 m with a neb s f; pos 138·0 from *; the centre of the neb is like a misty * 12 or 13 m, or perhaps 2 or 3 st 15 m; a small * to the s of neb makes an isosceles triangle. Place that of the * 10 m. | 233 | | | | 28·2 | 36 45 | B; L; R; p s b M; diam 3'; has a * n p (about 45°) at the edge, if not involved. | 235 | | 348 | Nova. | 5 0 53·9 | 73 42 5 | A cluster of 10 or 12 large and a good many small stars. The place that of a D *. It is perhaps an outlier of VII. 4. | 395 | | 349 | VII. 4 | 5 2 11·6 | 73 28 5 | L, rich cl; st 12...15 m; fills field. Place that of a D *. The most compressed part is 42°·5 foll the D * and 3' south of it. | 395 | | | | 19·3 | 34 6 | v L; p Rich; the prec border the brightest, consisting of st 10...12 m, but the foll the richest, consisting of st 12...18 m. Place of a * 10 m in prec border. | 396 | | 350 | VII. 33 | 5 8 21·9 | 50 50 36 | A * 7 m, very ruddy, almost orange-coloured, in a p rich cl of v s st. | 399 | | 351 | Nova. | 5 14 34·2 | 56 46 24 | Rich coarse cl of sc st 9...15 m; more than fills field | 51 | | 352 | II. 289 | 5 14 40·3 | 101 39 40 | p B; R; r; 30" | 315 | | 353 | VIII. 4 | 5 15 14± | 61 0 ± | The most condensed part of a poor cl divided into two. It consists of 20 or 30 st 9...12 m. | 115 | | 354 | VII. 39 | 5 16 41·0 | 54 50 36 | Rich p comp cl s stars; roundish with straggling borders of larger stars. | 51 | | | | 41·9 | 49 52 | p Rich; irreg R; stars 9...12 m, 50 or 60 counted; b M; the place that of the most comp part. | 42 | | | | 44·9 | 50 11 | p Rich; scattered cl of * s 12 m, and some larger, the most comp part = 3' diam. | 105 | | 355 | I. 261 | 5 20 7·9 | 55 53 54 | A nebula including a triple star, forming an equilateral triangle; sides = 4"; stars = 11, 12, 14 m. See fig 49. | 51 | | | | 11·3 | 53 22 | A triple * in a neb. A most curious object (see description of the d * h 367 in my 2nd Catal.) The neb surrounds the stars like an atmosphere. | 42 | | | | 13·9 | 53 41 | A triple * in a neb &c. &c. | 105 | | 356 | V. 38 | 5 20 34·4 | 98 31 18 | All about this place there exists diffused nebulosity. | 318 | | 357 | M. 1 | 5 24 15·7 | 68 6 36 | v L; E; v g l b M; r; 4' 1, 3' br; pos of longer axis n p to s f. | 59 | | | | | | A fine object. See fig. 81. | | | 358 | M. 36 | 5 24 56·5 | 55 57 52 | A coarse straggling cl which fills the field; a v pretty object; place B * in M. | 42 | | | | 65·5 | 59 24 | Rich; B; straggling stars; place of a D * h 368 whose place in my 2nd Catal is set down very erroneously by a mistake of copying. | 51 | | | | 70·4 | 59 16 | A considerable rich cl of L st 9...11 m; fills the field. The chief * is double. | 105 | | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|---------------|------------------------|-------| | 359 | III. 865 | 5 26 44·2 | 58° 7′ 57″ | F; R; S; p s b M. | 106 | | 360 | θ Orionis | 5 26 55± | 95 30 30± | Observed in sweeps 16, 38, 40, 110, 172, 173, 232...235, 309, 318, &c. See description and figure in Mem. Astr. Soc. 1826. | | | 361 | V. 31 | 5 27 6·9 | 96 2 18 | θ Orionis involved in a feeble neb 3′ diam | 318 | | 362 | Nova. | 5 27 7·4 | 94 28 10 | A coarse and poor but v splendid cl of L st; a beautiful object | 41 | | 363 | V. 34 | 5 27 35·3 | 91 19 3 | ε Orionis. Place by Catal a v brilliant * involved in an immense nebulous atmosphere, whose n and s limits are 91° 7′ 29″ and 91° 31′ 29″. Viewed also and shown to Mr. Dunlop in sweep 110. | 107 | | 364 | Nova. | 5 29 42·5 | 34 17 57 | A poor cl of 8 or 10 st 11 m | 324 | | 365 | IV. 34 | 5 32 47·6 | 80 59 57 | A circular disc 12″, a little mottled and of a pale light; a little ill-defined, but not hazy; a planetary nebula. | 118 | | | | | 48·3 | Planetary neb a little indistinct at the edges; rather oval and perhaps of a mottled light. | 121 | | 366 | VIII. 2 | 5 34 47·5 | 81 26 37 | A large tract of stars filling many fields. It extends much further in R. | 121 | | | | | ... | VIII. 2 viewed. A L ill-defined tract of loose stars, neither rich nor condensed. | 118 | | 367 | Nova. | 5 35 27·0 | 77 11 40 | A * 8.9 m with F neb | 393 | | 368 | M. 78 | 5 38 1·3 | 90 0 10 | Two stars 9 = 9 m; pos 60° n f; dist 50″ in a wispy nebula. See fig 36. | 113 | | | | | 2·6 | A v L wisp-shaped neb involving 3 st. It extends 5′; terminating abruptly to n, but extending s f beyond the 3rd *. | 107 | | 369 | M. 37 | 5 41 8·2 | 57 30 56 | v fine L cl, all resolved into st 10...13 m. It fills 1½ field, but the straggling stars extend very far. There may be 500 stars. | 52 | | | | | 10·3 | Splendid cl st 11...15 m; no unresolved neb; p comp but not m b M; fills field. | 51 | | | | | 10·8 | Irregular; not very rich; fills field | 56 | | 370 | III. 510 | 5 44 32± | 97 30 38 | v F; R; p s b M. R from working list; P D approximate. | 318 | | 371 | VII. 24 | 5 45 4·7 | 89 39 29 | The 2nd and brightest * of a poor straggling cl 10 or 12′ long | 107 | | 372 | VIII. 26 | 5 50 45·2 | 66 42 40 | About 40 or 50 st. The largest 8 m taken. The rest are 10...15 m | 59 | | 373 | Nova? | 5 53 50·8 | 100 36 25 | 3 Monocerotis. I am sure this star has a F neb atm 2′ or 3′ diam. Eye-glass examined, not dewed. | 315 | | 374 | Nova. | 5 54 2·8 | 84 16 53 | L; p rich; very scattered; place of * 10 m in M. | 320 | | 375 | VI. 17 | 5 56 59·2 | 65 53 46 | Rich; m compressed almost to nebulosity; stars very small; irreg triangular figure. | 59 | | 376 | Nova. | 5 57 36·5 | 38 17 51 | A poor cl 7′1, 3′ br; about a dozen st 11 m | 325 | | 377 | M. 35 | 5 58 22·2 | 65 39 13 | a L, coarse, p rich cl of st 9...16 m, which fills 2 or 3 fields, but chiefly one in which are about 100 stars. | 58 | | 378 | IV. 44 | 5 58 40·9 | 96 11 43 | A star 7 m with a p strong neb atmos. | 318 | | 379 | VIII. 24 | 5 58 51·2 | 76 1 34 | A pretty cluster of 20 or 30 st 10...11 m with one 9 or 9.10 which is double (Σ 848). | 393 | | 380 | VIII. 6 | 6 0 36·5 | 85 15 48 | A fine cluster; coarse; p rich; place of a * 9 m. | 320 | | 381 | IV. 38 | 6 1 13·9 | 96 18 48 | The large star of a double star has a very strong nebuluous burr | 318 | | 382 | Nova. | 6 2 30·2 | 93 29 52 | A large loose straggling cl of 8th class. The place is that of a double star. | 234 | | No. | Synonym. | AR 1830°. | N.P.D. 1830°. | Description and Remarks. | Sweep. | |-----|----------|-----------|---------------|-------------------------|--------| | 383 | IV. 20 | h m s | 6 2 48:9 | A * 10.11 m has a very sensible nebulous burr, and 3 more are rather nebulous; others in the field are not so. | 318 | | | | | | A * 10 m with a v F atmos. Two others s p are free from such atmos. A very F neb suspected s p this object. (N.B. The obs gives AR 24°8', but this is a manifest mistake of the wire which corrected = 51°3.) | 235 | | 384 | VII. 25 | 6 3 3:8 | 84 31 38 | A p rich, comp cl; one st = 9 m, 3 or 4 = 11 m, and many 12...15 m. Place that of the D * h 2288. | 320 | | 385 | Σ. 885 | 6 7 46:6 | 83 57 43 | The chief of a tolerably neat cl of L stars .................. | 320 | | 386 | VII. 20 | 6 12 35:9 | 97 13 49 | Coarse scattered cl; irreg R; st 11...15 m .................. | 16 | | | | 40:0 | 13 38 | Very pretty scatt cl 8...10' diam; p rich; stars = 11...14 m | 318 | | 387 | Nova. | 6 15 0:0 | 94 36 34 | The first * 6 m of a coarse poor cl; st 11...12 m ............ | 234 | | 388 | VII. 26 | 6 18 32:2 | 99 33 26 | A poor cl of v S stars; rather comp in M stars 12...15 m .. | 309 | | 389 | VIII. 9 | 6 20 0± | 73 12 35 | A p rich v loose cl; fills 2 or 3 fields; not b M; st 10...13 m | 395 | | 390 | VII. 5 | 6 20 34:0 | 83 3 22 | Irreg fig d cl like a hollow triangle in the crowded part of Milky Way; st v S; 12...15 m; one star 10 m. The surrounding loose stars are all large. | 118 | | 391 | VIII. 49 | 6 21 24:5 | 54 40 24 | Hardly to be called a cluster ................................ | 51 | | | | 38:2 | 42 0 :: | A v coarse straggling cl 10' diam; 30 or 40 stars 10...15 m. A * 10 m taken, but one of 7 m precedes to the n. | 124 | | 392 | VII. 2 | 6 21 53:1 | 84 56 28 | The place of * 8 m in most comp part of a L, poor, but brilliant cl. | 237 | | 393 | IV. 3 | 6 23 17:1 | 79 43 40 | A * 11 m with a milky neb surrounding it, but chiefly on the sp side. The star is not sharp—not stellar, and the neb fades gradually away from the *; 70 or 80" diam; has a * 7m 30° n f. | 120 | | | | 20:1 | 43 30 | A neb with nucl near the n f edge, which has not the sharpness of a *, but is dull and dead; = * 13 m; has a * 8 m 6°:55 foll s to n. | 121 | | 394 | Nova. | 6 25 36:3 | 94 56 40 | Place of a * 8:9 m in full part of a L p rich loose cl; irreg oblong fig; st 12...14 m. | 235 | | 395 | VIII. 3 | 6 25 40± | 81 30 ± | A large tract full of stars; v rich; place from working list. Viewed | 118 | | 396 | VIII. 50 | 6 25 52± | 84 31 ± | L, p rich; st small; place by working list .................. | 237 | | 397 | VII. 22 | 6 26 47:5 | 82 12 27 | A p rich, S cl; irreg fig; st 11...15 m ..................... | 118 | | 398 | VIII. 48 | 6 29 31:1 | 91 19 19 | Very coarse; v poor; v straggling; the chief * 8 m taken .. | 107 | | 399 | IV. 2 | 6 29 51:1 | 81 7 18 | A * 11.12 m with a p B cometary tail. See fig 64 ............ | 120 | | | | 54:0 | 6 32 | * 12 m with B cometic branch 60" l whose axis is 60° n p. The * is a little ill defined. The apex of the neb comes exactly up to *, but does not pass it. | 118 | | | | 54:3 | 6 54 | Cometic. Has a * 9.10 m 50° n f dist 2' .................... | 121 | | 400 | VII. 37 | 6 30 51:0 | 88 42 20 | A great many sc st; and a strong suspicion of a more comp part—(thick haze). | 322 | | 401 | 15 Monoc | VI. 31 | 36:8 | A * 5.6 m enveloped in a neb haze. Has about 15 or 16 small stars about it, one of which is a neat D * to s f. (N.B. This is a most remarkable object, being at once a close D *, a cluster and a nebulous star.) | 120 | | | | 79 57 55 | | A poor cl 30 or 40 S st 12.13 m ............................ | 393 | | 402 | Nova. | 6 31 59:9 | 77 55 32 | The most condensed part of a p rich, p comp cl st 11...15 m; irreg fig; diam of most comp part = 3...4'; triangular. | 115 | | 403 | VI. 21 | 6 32 40:2 | 62 52 2 | | | | No. | Synonym. | RA 1830-0. | N.P.D. 1830-0. | Description and Remarks. | Sweep. | |-----|----------|------------|----------------|-------------------------|--------| | 404 | VI. 3 | h m s | 6 34 56± | Close cl of v small st; poor; twilight; preceded by a coarse cl of large ones. | 237 | | 405 | VIII. 36? | 6 35 0'9 | 86 23 13 | Coarse sc cl; not v rich; place of * 9 m .................. | 320 | | 406 | II. 614 | 6 36 3'2: | 56 15 50: | F; S; b M; the southern of two ................................ | 124 | | | | | 5'5 | F; forms a D neb with another exactly n ........................ | 51 | | 407 | II. 615 | 6 36 3'2: | 56 13 50: | e F; v S; the northern of two .................................. | 124 | | | | | 5'5 | e F; the northern of a d neb .................................. | 51 | | 408 | VIII. 31 | 6 39 9'3 | 92 58 10 | Loose L irreg sc cl of about 100 st 9...15 m .................. | 41 | | | | | ... | Viewed; p rich; v coarse; a few st = 9 ..10 m ............... | 235 | | 409 | III. 897 | 6 39 41± | 56 19 24: | e F; the northern of two, 3 or 4' apart ...................... | 51 | | 410 | III. 898 | 6 39 41± | 56 23 24: | e F; the southern of two ...................................... | 51 | | 411 | M. 41 | 6 39 43 | 110 34 13 | Coarse; fills field. The chief, 8 m, is red; a poor cl. (The place is estimated from a D * in the cl.) | 236 | | 412 | Nova? | 6 42 49'8: | 96 46 37: | A coarse cl; not v rich; 30 or 40 st; probably only an outlying portion of VIII. 39. | 122 | | 413 | VI. 27 | 6 43 1'1 | 89 20 39 | A D * in the chief group of a p rich coarse cl not v comp. Broken into 3 groups. The s p group is the richest. The P D mistaken 5' in reading off; corrected. | 397 | | | | | 3'9 | The principal D * in a cl; p rich; irreg fig; not m comp .... | 113 | | | | | ... | The brightest * (D h 740) of a fine cl; rich; not v comp; irreg fig. | 107 | | | | | 20 ± | A fine rich cl 10' diam; irreg fig; place of a D star ........ | 322 | | 414 | VIII. 39 | 6 43 33'5 | 96 53 30 | A v poor S cl; about a dozen st 11 m in a rich region ........ | 135 | | | | | 36'0 | Coarse; p rich; 15 or 20 st in middle, p comp; with stragglers which fill the field. | 318 | | | | | 37'7 | Poor cl; 12 or 15 S stars, and 2 or 3 larger; place of the 2nd star 10 m in cl. | 136 | | 415 | VI. 2 | 6 45 2'6: | 71 45 28: | A p L comp cl 5 or 6' diam; irreg fig; p g l b M; place doubtful from temporary instability of the zeros. | 333 | | | | | 18'2 | P rich cl; acutangular, the acute angle precedes; the p side is bounded by a remarkably definite line; pos 223°4; st 14...16 m. See fig 91. | 313 | | 416 | VIII. 51 | 6 46 19'8 | 96 59 19 | Very poor cl; is only an outlier of VIII. 39, the st being more sc, less rich, and larger. | 136 | | | | | ... | Viewed. Has no title to be called a cluster .................. | 135 | | | | | ... | Viewed. An outlying portion of VIII. 39 ..................... | 318 | | 417 | VI. 18 | 6 47 46'3 | 96 59 18 | No descrip .................................................... | 318 | | | | | 48'7 | A cluster, not v rich; 4' diam; irreg fig; st 12...13 m ..... | 135 | | | | | 49'2 | p rich; irreg R fig; st 13...16 m; strong twilight .......... | 136 | | 418 | VIII. 60 | 6 49 22'8 | 94 22 0 | A sc cl of S stars, not rich .................................. | 41 | | 419 | Nova. | 6 49 27'1 | 79 31 10 | A poor cluster. The largest star 10 m taken .................. | 120 | | 420 | Nova. | 6 49 27'4 | 39 10 16 | v F; doubtful .................................................. | 329 | | | | | 32'4 | e F; doubtful. (The agreement of the places dispels the doubt, and shows that a nebula really exists here.) | 327 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep. | |-----|---------|-----------|--------------|------------------------|--------| | 421 | II. 304 | 6 51 27·0 | 97 33 40 | pB; R; S; r; among a multitude of stars .................. | 135 | | | | | 28·7 | pB; R .................. | 318 | | | | | 30·5 | F; S; R; has a * 13 m s, dist 60" ...................... | 136 | | 422 | VII. 14 | 6 51 42·6 | 103 28 16 | A v coarse loose cl of stars 8 or 9 m .................. | 111 | | 423 | VIII. 1 | 6 52 13·1 | 86 42 39 | Place of * 9 m in a v coarse straggling cl of 3 or 4 fields in extent. Only a rich part of the heavens. | 239 | | | | | 14·5 | Linear cl of stars 11...13 m, forming a bent line nearly 15' long, terminated on the f side by a * 8 m whose place is that here taken. | 237 | | 424 | II. 861 | 6 52 37·6 | 39 10 46 | p B; R; p g b M; 15"; n p a * 8 m; pos about 30° s f; dist = 1 diam of neb from edge. | 329 | | 425 | M. 50 | 6 54 42·2 | 98 5 19 | Rich; comp; fills field; stars 10...15 m; place of a * 10 m in middle—a fine cluster. | 16 | | | | | 45·5 | A L rather straggling cl 10...12' diam; st 11...15 m. The largest in M, taken. | 135 | | | | | 46·6 | Superb cl; fills whole field; irreg R; stars 11...15 m; not comp in M; straggling stars extend over a circle 30' in diameter. | 318 | | | | | 49·4 | A fine v L sc cl; has a red star 8.9 m to s of the more compressed part. | 136 | | 426 | II. 734 | 6 55 8·7 | 39 3 20 | e F; R; p s l b M; has a small group of st immediately p like the letter Y. | 327 | | 427 | VII. 38 | 6 55 16·0 | 88 41 39 | Fine rich p L cl; st 12...18 m; 10' diam. One * 11 m (place taken); straggling. | 397 | | | | | 32·1 | The most comp part of a v L coarse sc cl. The stars 11...15 m. Towards the north they are 9, 10, and more coarsely sc. | 322 | | | | | ... | Rich L cl; fills field; st 14...16 m; not comp towards a centre. | 113 | | 428 | IV. 25? | 6 56 8·7 | 101 4 16 | A D * whose L * is in centre of a v F neb which involves the s * also. | 130 | | 429 | II. 735 | 6 56 17·3 | 41 8 6 | v F. Among stars ......................... | 329 | | 430 | II. 862 | 6 56 30·3 | 39 33 26 | F; S; R; p s b M; 12"......................... | 330 | | 431 | III. 899| 6 56 35± | 54 37 ± | v F; R; b M; 30". AR by working list ............... | 124 | | 432 | VIII. 40| 6 56 54·3 | 62 33 18 | A small cl of 10 or a dozen st 11...13 m in an ellipse .... | 57 | | | | | 56·3 | A L coarse straggling cl of L stars. The part taken is a small oval group 90" diam in the following part. | 115 | | 433 | II. 736 | 6 58 8·3 | 39 33 26 | p F; R; g b M; 20"............................. | 330 | | | | | 9·9 | p B; p L; R; g b M; 25"; two s st p ............... | 329 | | 434 | II. 769 | 6 58 24·2 | 70 57 38 | p B; p L; R; g l b M; 40". In a rich part of the heavens .... | 333 | | 435 | Nova. | 6 58 38·1 | 95 21 59 | Very loose and straggling cluster .................... | 122 | | 436 | VII. 27 | 7 1 49·9 | 98 21 13 | A poor straggling cl. Place of a D * ................ | 318 | | 437 | Nova. | 7 5 31·4 | 101 12 14 | A loose straggling cl. Place of a D * ................ | 129 | | 438 | VII. 16 | 7 7 14·3 | 115 26 30 | Loose straggling cl; the p part is rather separated from the f, and more comp. Place that of 3 st in the f part. | 317 | | 439 | VI. 6? | 7 7 22·1 | 75 55 52 | A p rich cl of v s stars; irreg; R; 5' diam; not b M; st 11...16 m. | 393 | | 440 | VII. 12 | 7 10 2·2 | 105 20 15 | A rich cluster of stars 10 m ....................... | 111 | | No. | Synonym | RA 1880°.0 | N.P.D. 1880°.0 | Description and Remarks | Sweep | |-----|---------|------------|---------------|------------------------|-------| | 441 | VII. 17 | 7 11 40·1 | 114 39 20 | A L * 7 m in the centre of a beautiful cl 8' diam; not v comp; nearly R; not more comp in M; stars 11...14 m. | 317 | | 442 | Nova. | 12 32·5 | 97 15 8 | Two S p close groups of p L st in the Milky Way, rather a remarkable cl. | 318 | | 443 | Nova. | 7 12 55·1 | 100 4 24 | The p star (which is red) of a p rich S cl; fig irreg triangular; #s 15 m—in Milky Way. | 129 | | 444 | II. 316 | 7 14 49·1 | 60 11 20 | The sp of a curious B double neb or an elongated bicentral neb; nuclei approaching to stars 45° n f to sp 30'' dist. | 57 | | | | | | A double neb close B S R s B M; pos 45° n f or s p—dist of centre 60''. See fig 72. | 115 | | 445 | II. 317 | 7 14 50·9 | 60 11 0 | The n f of the double neb ................................................. | 57 | | 446 | Nova. | 7 17 20± | 55 51 ± | The first of four ....................................................................... | 128 | | 447 | III. 703| 7 17 25·5 | 55 50 ± | A v F neb; another neb s p; the 2nd of 4 .................................. | 128 | | 448 | III. 900| 7 17 47·5 | 55 51 40 | e F; R; b M; 20''; the 3rd of 4 .............................................. | 128 | | 449 | III. 901| 7 18 0·0 | 55 48 18 | v F; R; p s b M; 30'' .................................................................... | 128 | | 450 | IV. 45 | 7 19 7·7 | 68 45 2 | A * 8 m exactly in centre of an exactly R B atmosph 25'' diam; the star is quite stellar, not a mere nucl. Another * 8 m distant 100'', and about 85° n p has no such atmos.—A most remarkable object.—Fig 31 (IV. 69) will also represent this neb. | 59 | | 451 | VIII.36?| 7 20 14± | 101 24 ± | A straggling portion of Milky Way ............................................. | 129 | | 452 | Nova. | 7 21 8·8 | 17 57 55 | A very loose sc cl of large stars, or a starry place ...................... | 230 | | 453 | III. 19 | 7 21 28·0 | 79 59 58 | e F; R; l b M; = 15 m; has the f of 4 stars near it ....................... | 123 | | | | | 28·5 | e F; among several st 13...14 m; one = 14 m is in the neb ............... | 120 | | | | | ... | Most excessively F ....................................................................... | 132 | | 454 | VII. 65 | 7 21 34·2 | 103 37 48 | A S cl of v S stars among rich parts of the Milky Way .................... | 111 | | 455 | VIII. 37| 7 25 27·4 | 105 5 2 | A cl with 1 st 9 m; not rich .................................................... | 111 | | 456 | II. 821 | 7 25 44·8 | 54 24 10 | Not v F; S; R; 10''; nearly planetary; but a l hazy; v g v l b M ....... | 128 | | | | | ... | A curious, almost planetary neb 10'' diam R; light nearly equable; between 2 S st. | 51 | | 457 | I. 218 | 7 26 35·5 | 50 44 57 | p F; L; R; v g b M; 70''; C; a L * 8 m precedes 19°·0, and before that is a D *. | 401 | | | | | ... | Viewed; not v B; L; p m E in parallel 2' 1, 75'' br; a * 7.8 m precedes 19°·0 and 15'' to s, and preceding this is a coarse double *. | 335 | | 458 | VI. 1 | 7 28 18·7 | 68 3 17 | A p rich cl; irreg fig; 50...100 st; 11...18 m; 5...7' diam. | 59 | | 459 | VII. 38 | 7 28 46·4 | 104 6 28 | The chief * of a L, p rich, straggl cl. It is double .................... | 111 | | 460 | II. 822 | 7 30 6·5 | 37 16 50 | v F; among s stars; one 8 m precedes at some distance .................... | 327 | | 461 | Nova. | 7 32 59·7 | 37 31 50 | v F; S; R; b M; diam 8'' ................................................................ | 327 | | 462 | Nova. | 7 33 26·4 | 80 20 45 | e F; has * 15 m 90'' dist 30° n p ............................................. | 123 | | 463 | M. 46 | 7 34 1·6 | 104 25 45 | The brightest part of a v fine rich cl; stars = 10 m; which fills the field. Within the cl at its n edge is a fine planetary neb. | 111 | | 464 | IV. 39 | 7 34 1·6 | 104 20 25 | A planetary neb 3°·75 (time) in diam. Exactly R of a F equable light. Has a v minute * a l n of centre. It is not b M nor fading away, but a little velvety at the edges. At the n edge of the fine cl M 46. | 111 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 465 | Nova. | h m s | 7 35 12·3 | 34° 59′ 2″ | Four small stars in a semicircle, within whose concavity there is a F nebulosity, which I am pretty certain is real. | 324 | | 466 | Nova. | | 7 37 25·7 | 114 16 59 | A * 8 m followed by a poor cl of 18...20 st, 11...13 m.... | 317 | | 467 | Nova. | | 7 40 31·6 | 34 5 2 | v F; R; v g b M; and losing itself imperceptibly............. | 324 | | 468 | III. 479| | 7 42 46·0 | 80 1 15 | A 1 group of S st which has a neb look, and perhaps there may be neb among them. No other near. | 120 | | | | | | 46° 0 | A S group of st; with attention counted 5 with power 320°; form a neb group 20″ diam. | 123 | | 469 | Nova. | | 7 43 20·4 | 32 53 12 | e F; R; the preceding of two .................................. | 324 | | 470 | III. 836| | 7 44 14·6 | 32 52 42 | F; R; 15″; the foll of two .................................... | 324 | | | | | | 15° 0 | p F; R; 15″; n p a * 9 m which is 2 diameters of neb dist from its centre. | 323 | | 471 | III. 830| | 7 44 51·4 | 36 41 35 | p F; E, or has a v S * s p and a L * n f. Also query if not a v S * in centre. | 327 | | 472 | IV. 22 | | 7 45 25·5:: | 115 57 29 | A * 9 m with a W of st and nebulosity, or ? if not a v F neb about the stars—(no red colour seen). | 317 | | 473 | II. 302 | | 7 47 2·2 | 65 47 28 | F; S; R ......................................................................... | 58 | | 474 | VII. 10 | | 7 47 27·4:: | 113 51 51 | A cl p rich; v coarsely sc, 10...15′ diam; perhaps 50 st.... | 317 | | 475 | III. 837| | 7 47 59·9 | 32 59 12 | v F; R; g l b M; 15″ ................................................ | 323 | | 476 | III. 750| | 7 48 30± | 49 43 ± | Viewed by working list; p B even though there is C enough to see the wires well. R; g b and then s b M; 20″. | 335 | | 477 | Nova. | | 7 49 3·4 | 62 31 17 | v F; S; R; b M.................................................................. | 115 | | 478 | III. 709| | 7 49 9·5 | 38 47 20 | F; L; R; v g b M; 60″. Among stars ................................ | 327 | | 479 | VII. 23 | | 7 49 28·1 | 119 36 24 | A fine rich cl; L; stars 12 m and nearly equal; not m comp M about 3′; at the centre equally comp and thence looser. | 316 | | 480 | VI. 37 | | 7 51 50·1 | 100 19 34 | The 1st * 11 m in the p part of a rich R p comp cl irreg fig; * s 11...20 m, so as to be nebulous. The most comp part = 4′ or 5′ diam. | 129 | | 481 | II. 554 | | 7 51 57·2 | 73 49 35 | F; R; 15″. Pos of a * 12 m = 225°·5, dist = 60″ .............. | 395 | | 482 | III. 605| | 7 52 57·7 | 66 8 31 | v F; S; R ......................................................................... | 59 | | 483 | III. 512| | 7 53 8·6 | 80 7 15 | p B; R; p s b M.................................................................. | 120 | | | | | | 9·5 | No descrip ....................................................................... | 132 | | 484 | III. 7 | | 7 53 11·0:: | 80 59 25:: | Follows 2 v S st; obs doubtful. Nearly missed obs, owing to the working list being much out in P D. | 123 | | | | | | | Viewed; F; v S; rather E. 2 st s p. Seen also, but no descrip given, in Sw 132. | 120 | | 485 | Nova. | | 7 54 54·0 | 31 44 52 | p F; R; p s b M; s f a * 9 m dist 3′ ................................ | 323 | | 486 | III. 877| | 7 57 35·1 | 100 57 6 | F; L; R; v g b M; 90″; among stars of the Milky Way........... | 129 | | 487 | III. 752| | 7 58 10·7 | 71 41 26 | e F; R; ........................................................................... | 334 | | 488 | VIII. 30| | 7 58 40± | 117 41 22 | Cl p rich; v coarsely sc; fills field; st 10...15 m. AR by working list. | 317 | | 489 | II. 726 | | 7 59 18·0 | 55 33 44 | p B; R; b M; 40″.................................................................. | 51 | | | | | | 21·0 | F; L; R; v g l b M; 80″................................................ | 128 | | 490 | III. 840| | 7 59 27·4 | 33 50 22 | p B; L; R; p s b M; diam 60″ and very gradually fading away; has a * 8 m pos = 164°·3. | 324 | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|----------|-----------|--------------|-------------------------|-------| | 491 | IV. 55 | h m s | 8 1 10°0 | p F; R; 60''; very nearly uniformly B, but hazy at edges. It is a resolved globular cluster. Being a remarkably fine night, I see the stars; they are 20 m; a * 9.10 m is 40° s f dist 2'. | 139 | | 492 | III. 710 | | 8 2 14°1 | Not v F; L; l E; v g b M; 90'' .................................. | 329 | | 493 | II. 719? | | 8 3 55°4:: | v F; R; a coarse d * p points to it. Δ AR = 1° 2° ................ | 401 | | 494 | II. 627 | | 8 4 17°2 | F; S; R; has a * 8 m, 4' dist p ................................. | 59 | | 495 | Nova. | | 8 5 10°7 | p B; S; m E; pos in merid; p s m b M; 15'' 1, 6'' br. A * 7 m follows. | 323 | | 496 | VI. 22 | | 8 5 18°7 | Fine L, p rich, very straggling cluster of st 9.10 and 10.11 m. The straggling edges extend a full field either way. Place that of a D * in the most comp part. | 235 | | | | | | 18°8 | 18°54 | | | | | | | | | 497 | II. 303 | | 8 8 46°7 | A superb cl which fills the whole field; st 9.10...13 m and none below, but the whole ground of the sky on which it stands is singularly dotted over with infinitely minute points. Place that of a B st, the s of two which point into the concavity of an arc. | 234 | | 498 | III. 256 | | 8 9 11°1 | A cl of about 100 large st 10 and 11 m .......................... | 21 | | 499 | III. 606 | | 8 9 21°8 | p B; R; b M .......................................................... | 59 | | 500 | III. 607 | | 8 10 28°2 | v F; between a * 12 m, s f and one 16 m, n p, the former dist about 1 diam, the latter about ½ diam from the edge. | 397 | | 501 | II. 634 | | 8 10 41°2 | v F; S; R ............................................................ | 59 | | 502 | VI. 39 | | 8 12 1°8 | v F; S; R ............................................................ | 59 | | 503 | VII. 64 | | 8 12 11± | A v loose straggling but p rich cl which fills the field, st 9 m and under; v l comp M. Some large st precede it. | 316 | | 504 | III. 753 | | 8 15 16°9 | A fine, p rich cl; stars 11 m pretty uniform 5...6' diam. The chief stars make a zigzag line, the outliers extending 20'. | 316 | | | | | | v F; R; 1 b M; has a * 1' p ..................................... | 63 | | | | | | v F; R; g b M; is 90'' f a * 11 m, and many small st near; windy. | 333 | | | | | | v F; p L; v g b M; 40''........................................... | 334 | | 505 | II. 315 | | 8 16 52°7 | p B; R; v s b M to a *; 20'' .................................... | 58 | | 506 | III. 599 | | 8 17 48°7 | v F; irreg fig; has a coarse D * 30° s p, 2' dist ............... | 59 | | 507 | III. 234 | | 8 22 12°9 | v F; S .............................................................. | 59 | | 508 | Nova. | | 8 22 13°0 | e F; S; R; n p a star (about 5° n p). The preceding neb of 2... | 328 | | | | | | e F; S; R; 8''; one or other of these ARs is probably affected by an error of 10° in reading off the time. | 327 | | 509 | III. 292 | | 8 22 50°9:: | e F; doubtful obs, as at first the neb was hardly seen. Verified, but too late for a good AR. In field with a D * which points rather s of it. | 56 | | | | | | e F; R; b M; 30''. This AR preferable .......................... | 64 | | 510 | Nova. | | 8 22 51°4 | F; S; R; about 40° s f a * ..................................... | 328 | | | | | | v F; S; R; 12''. The following and brighter of 2............... | 327 | | 511 | Nova. | | 8 23 38°4 | e F; a doubt remained; windy .................................... | 115 | | 512 | II. 318 | | 8 24 53°3 | F; R; b M .......................................................... | 64 | | | | | | F; irr R; b M .................................................... | 57 | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep. | |-----|----------|-----------|--------------|-------------------------|-------| | 513 | IV. 35 | h m s | 8 25 34'4" | A * 14 m with a fan-shaped brush 15'' 1 to the s p side; the brush however judged by both Mr. Dunlop (who saw it) and myself not to be in contact. A B * 6.7 m, n f. | 111 | | 514 | II. 319 | | 8 27 8'8" | v F. Clouded before P D could be well obtained .................. | 64 | | | | | 11'0 | p B; S; R; b M .................................................. | 57 | | | | | 12'0 | F; L; b M; 60...80'' ............................................ | 115 | | 515 | III. 257 | | 8 27 15'9:: | Extremely doubtful, as I could not recover the object ........... | 397 | | 516 | VII. 63 | | 8 30 15'6 | A fine cl shaped like a flattened X. Stars 11...13 m; fills field, but the most comp part = 6' diam; p rich; not m comp M. | 316 | | 517 | Præsepe. | | 8 30 25'1 | Præsepe Cancri (M 44) is so very loose and straggling that it would only be noticed as a region rich in L stars;—so also described in Sweeps 59 and 63. | 333 | | 518 | I. 204 | | 8 31 24'7 | p B; p m E; p s m b M; 30'' l; 20'' br ........................ | 330 | | | | | 27'1 | B; S; E; p s b M; pos n p to s f............................... | 329 | | | | | 28'0 | p B; p m E; p s m b M, almost to a *; 30'' l .................. | 328 | | | | | 30'7 | p B; E; S. A fog coming on ..................................... | 327 | | 519 | Nova. | | 8 32 50'3 | A v F cl or r neb; g b M; 80'', one * 17 m distinct; stars and nebulosity; has 2 p B st s and one following. | 234 | | 520 | I. 288 | | 8 32 59± | v B; 1 E, in parallel; p s m b M, to a nucl = a * 12 m; 30''. Has a L * p and another f, at a considerable dist. | 170 | | 521 | III. 49 | | 8 33 9'8 | F; R; b M; 12'' .................................................. | 395 | | | | | 12'1 | Not v F; S; R; p s b M; 12'' .................................. | 243 | | 522 | II. 727 | | 8 33 17'0 | F; L; R; place badly taken ..................................... | 51 | | | | | 23'0 | F; L; R; r; 50...60'' .......................................... | 128 | | | | | 24'4 | F; L; R; r.......................................................... | 127 | | 523 | Nova. | | 8 35 13'0 | e F; p s b M ...................................................... | 324 | | 524 | Nova. | | 8 37 50'4 | A neat cl of stars 9 and 10 m regularly arranged about a central one. (N.B. This is nearly the place of III. 50, but no neb was noticed.) | 241 | | 525 | Nova. | | 8 38 14'8 | The chief * of a coarse cluster ................................ | 139 | | 526 | II. 80 | | 8 39 39'4 | p B; R; b M. Query if not bicentral ............................ | 63 | | | | | 40'8 | v B; R; v s m b M to a *; a v F * follows ..................... | 333 | | | | | 41'4 | v B; p L; p g m b M; a v S * s f almost involved ............. | 334 | | 527 | II. 48 | | 8 40 18'4 | The faintest object imaginable, and discerned with the utmost difficulty. Sky perfectly clear. | 334 | | 528 | VIII. 10 | | 8 40 37'9 | A poor cluster of 4 or 5 large and a few sc s st ............... | 242 | | | | | 62'1 | The chief star 9 . 10 m of a place rich in stars ............... | 120 | | | | | 63'2 | A v coarse and poor cl. Place of a D *.......................... | 241 | | | | | ... | An insignificant cluster. No other near ........................ | 123 | | 529 | III. 294 | | 8 41 8'8 | p B; R; v g m b M; 15'' ......................................... | 56 | | 530 | I. 242 | | 8 41 15'1 | B; L; v s m b M to a * 10.11 m, but sharply defined. It is a neb * with a v F extensive nebulosity. | 328 | | | | | 16'3 | v B; v s m b M to nucl. Seen through thick fog; a L * s f dist 10' and 2 S st p near. | 327 | | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|----------|------------|----------------|-------------------------|-------| | 531 | M. 67 | h m s | 8 41 29'4 | Pretty rich cl of sc st 10...15 m .................................. | 17 | | | | | | 200 st, more or less; it fills field; st 11...15 m. It is preceded by a rich region of st 9...10 m. | 19 | | | | | | Superb cl very rich and brilliant; fills field; stars 9...15 m; straggling at edges and not very comp in M. | 241 | | | | | | 100 or 200 st coarsely sc 11...15 m .................................. | 22 | | | | | | A cluster. No further descrip ........................................ | 242 | | 532 | I. 200 | 8 42 5'0 | 55 57 42 | v B; v L; m E; 45° n f to s p; g m b M; 5'1; 40" br; windy | 127 | | | | | | v B; v L; g m b M; 5'1; 50" br; E 45° (s p by diag) ............... | 128 | | | | | | v B; v m E; pos 40°-9 by microm 4'1; 1" br; p g b M; 4 stars near | 337 | | 533 | III. 712 | 8 42 53'4 | 40 12 1 | v F; p L; R; 30"; a * 12 m s f (one semidiam from edge) and one 13 m, n p. | 330 | | | | | | p F; R; g b M; 20" ..................................................... | 329 | | 534 | III. 831 | 8 44 37'6 | 37 17 13 : | v F; S; R; p s b M ..................................................... | 328 | | 535 | II. 823 | 8 44 43'6 | 38 0 18 | p B; m E nearly in merid; p s b M .................................... | 328 | | 536 | II. 880 | 8 45 49'6 | 92 25 19 | p B; S; E nearly in parallel between 2 st of 12 and 15 m, each half the length of the neb from the adjacent extremity. See fig 61. | 21 | | 537 | IV. 66 | 8 46 33'4 | 35 35 7 | A * 11 . 12 m with a p B fan-shaped neb appendage in which there seems to be one v F *. A curious object. See fig 65. | 324 | | 538 | Nova. | 8 47 2'6 | 92 32 49 | v F; R; r; 30"; stars suspected in it. A * 9 m precedes. This may possibly be II. 281 with an error of 10' in P D, but I have no reason for believing my obs erroneous. | 20 | | 539 | Nova. | 8 47 17± | 10 8 ± | p B; S; E from n f to s p. Has a * nf................................. | 171 | | 540 | Nova. | 8 48 1'8 | 44 26 37 | p B; L; E; v g b M; 2'1; 1½' br; with attention a central point is seen = a * 18 m. | 139 | | 541 | III. 540 | 8 49 32'1 | 53 37 12 | A strong suspicion of a neb, but clouds prevented verification. | 331 | | 542 | II. 557 | 8 49 48± | 83 0 ± | F; p L; R; AR from working list, and P D hardly more than conjectural. | 116 | | 543 | II. 529 | 8 50 28'9 | 94 14 10 | v F; R; v g b M; p L; 60" ............................................. | 235 | | | | | | p F; R; v g b M; 25" .................................................. | 234 | | 544 | Nova. | 8 51 13'3 :| 53 35 47 | e F; S; R ................................................................. | 401 | | 545 | II. 834 | 8 51 28'3 | 29 23 47 | e F; R; quite certain.................................................. | 404 | | 546 | Nova. | 8 52 31'3 | 92 43 19 | v F; L; R; b M............................................................ | 21 | | 547 | Nova. | 8 53 0± | 93 3 54 | e F; R; AR between 52m 31s and 54m 41s................................ | 21 | | 548 | Nova. | 8 53 34± | 12 49 ± | p B; p L; E; v g l b M; 90'1; 40" br.................................. | 171 | | 549 | Nova? | 8 53 56'4 | 37 34 23 | Four small st with a strong suspicion of nebula among them .. | 328 | | 550 | I. 249 | 8 54 2'7 | 28 51 20 | v F; p L; R; v g b M; 60"; C C. A * 8 m n p....................... | 404 | | 551 | III. 60 | 8 55 1'4 | 70 53 2 | v F; R; has a double * to n.......................................... | 63 | | | | | | v F; is s of a coarse double * ...................................... | 334 | | 552 | III. 825 | 8 55 21'2 | 53 56 35 | Near a *, but doubtful ............................................... | 337 | | | | | | e F; has * 12 m 45...50° n p; dist 60"............................. | 401 | | | | | | e F; R; v g l b M. A * 11 m 75° n p; 40"............................ | 128 | | | | | | e F; S; s of a st 12.13 m .......................................... | 127 | | No. | Synonym | AR 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 553 | II. 828 | 8 56 40·4 | 35 28 17 | pB; pL; lE; vglbM | 324 | | 554 | III. 647 | 8 57 38·4 | 51 41 37 | pF; R; S; but not nearly so F as II. 825, which precedes it in the sweep. | 401 | | 555 | I. 250 | 8 58 19·3 | 29 16 31 | pB; lE; psbM; 50" l, 45" br | 404 | | 556 | Nova. | 8 58 22·8 | 38 55 31 | eF; sbM to a * 15 m; the first of 3 | 330 | | 557 | III. 236 | 8 58 32·7 | 67 52 22 | No description | 59 | | 558 | II. 520 | 8 58 42·8 | 85 55 30 | vF; pL; g b M, but not to a nucleus | 238 | | 559 | Nova. | 8 58 43·7 | 38 54 1 | Not eF; lE; bM. The second of 3 | 330 | | | | 45·5 | 53 16 | Not vF; lE; S; psbM; 15" | 329 | | 560 | II. 275 | 8 58 49·0 | 104 49 14 | eF; pL; has a small * just n, and four more preceding | 111 | | 561 | Nova. | 8 58 52·2 | 38 57 21 | vF; R or vlE. The last of 3 S neb | 330 | | | | 54·1 | 57 6 | vF; S; lE; 10" | 329 | | 562 | II. 490 | 8 59 3·5 | 56 11 20 | F; mE in direction 45° np; 3' l, 1' br | 128 | | | | 6·5 | 11 24 | F; E 75° np...sf; 90" l, 30" br | 51 | | | | 7·6 | 11 7 | F; L; mE; pos np...sf | 127 | | 563 | Nova. | 9 0 55·5 | 44 21 2 | pB; vL; R; vgbM; r; 3' diam. C | 139 | | 564 | I. 2 | 9 1 14·8 | 82 16 27 | pB; R; gmbM | 18 | | | | 17·9 | 16 26 | vB; R; psbM; 2' diam; the hazy border perhaps extends further; r:: | 116 | | 565 | III. 61 | 9 1 20·1 | 71 37 42 | vF; S; r. My MS obs makes the PD 70°, but my father's obs makes it 71°. Each relies on a single obs. Of course I prefer 71. | 63 | | 566 | II. 546 | 9 1 50·5 | 54 17 34 | pB; S; R; mbM; 20" | 51 | | | | 51·1 | 16 40 | B; R; vsmbM; 20" | 337 | | | | 52·7 | 16 27 | pF; R; bM; 30" | 127 | | | | 54·0 | 16 35 | Not vF; R; psbM; 25" | 401 | | 567 | III. 825 | 9 2 11·9 | 54 22 31 | vF; S; 7·5 following a S double * | 337 | | 568 | I. 167 | 9 3 4± | 49 16 ± | Viewed. Found in place as determined by my father. No description. | 335 | | 569 | I. 66 | 9 3 25·1 | 104 7 31 | pB; E in parallel; psbM; 60" l | 111 | | 570 | I. 216 | 9 3 39·8 | 20 4 51 | F; E in parallel; psbM; 30" | 377 | | 571 | I. 59 | 9 4 44·4 | 113 30 4 | pB; R; g b M; 25" | 317 | | 572 | Nova. | 9 6 19·4 | 54 52 10 | vF; R; has a D * 5' n; 1°p | 128 | | | | 21·5 | 51 15 | vF; S; R | 337 | | 573 | III. 296 | 9 6 28·3 | 58 24 28 | The faintest conceivable | 56 | | 574 | III. 832 | 9 6 31·7 | 36 46 48 | A * with vF neb attached, in which is involved another * 10" dist. | 328 | | 575 | III. 62 } | 9 6 38± | 70 20 33 | A S F close double nebula. The individuals are 30" asunder. Place hardly more than conjectural in P.D. AR by working list. | 63 | | | III. 63 } | | | | | | 576 | II. 868 | 9 7 12·0 | 25 2 45 | vF; S; near a * 8 m | 410 | | 577 | Nova. | 9 7 12·4 | 69 5 56 | vF; S; R; the np of two, distant 8' | 59 | | 578 | Nova. | 9 7 30·0:: | 69 14 19: | vF; S; R; the sf of two, distant 8' | 59 | MDCCCXXXIII. | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 579 | Nova. | 9h 7m 56s | 28° 50' 33" | F; p m E.................. | 410 | | 580 | II. 505 | 9h 8m 12s | 105° 35' 52" | pB; E to n f; p s b M; 60" | 111 | | 581 | Nova. | 9h 9m 0s | 55° 33' 25" | e F; E........................ | 337 | | | | | 33° 0 | v F; it is the s p of two. The other is I. 113............. | 51 | | 582 | I. 113 | 9h 9m 22s | 55° 32' 24" | B; R; b M.................. | 51 | | | | | 23° 0 | p B........................ | 337 | | 583 | III. 627| 9h 9m 55s | 49° 59' 46" | p F; S; R.................. | 335 | | 584 | I. 205 | 9h 10m 14s| 38° 18' 3 | v B; v m E; v s m b M; pos 150° 8'; comes up to a nucleus, a star 10.11 m; has 2 st not involved 11 & 12 m, and a 3rd 10 m perp to axis of neb. | 328 | | 585 | Nova. | 9h 10m 20s| 105° 45' 43" | e F; R; b M; precedes a * 8° 5 ......................... | 111 | | 586 | III. 827| 9h 10m 22s| 53° 54' 57" | v F; not v S; R; 100"....120" s f a * 10 m .............. | 127 | | | | | | Viewed. It is 1 field (1mI ½ ±) f a v B * 6.7 m........... | 128 | | 587 | III. 488| 9h 12m 5s | 105° 47' 43" | v F; L; E n f to s p; 1b M. It is 9° 5 in AR preceding a * 11 m, and is S of the *. | 111 | | 588 | III. 629| 9h 12m 25s| 49° 8' 56" | v F; S; R; has a * 10 m 2' dist prec. The first of 2....... | 335 | | 589 | III. 714| 9h 12m 26s| 40° 4' 56" | v F; p L; R; v g b M. The preceding of 2, making an isosceles triangle with the other and a star. | 330 | | | | | 28° 8 | p F; R; p s l b M; 20". The s p of 2, making an isosc triang with a * 9 m. | 329 | | 590 | III. 630| 9h 12m 29s| 49° 7' 6" | e F; p L; v g b M; the following of 2 ..................... | 335 | | 591 | III. 713| 9h 12m 40s| 40° 2' 1 | p F; 1E; v g b M; the foll of 2 .......................... | 330 | | | | | 41° 7 | Not v F; R; p s b M; 20"; the n f of 2, making isose triang with a * 9 m. | 329 | | 592 | I. 132 | 9h 13m 14s| 101° 11' 24" | p B; R; 45"; p g m b M; almost to nucl.................... | 129 | | 593 | I. 137 | 9h 13m 53s| 54° 45' 4 | B; R; m b M; 40"; not resolved with 240.................. | 51 | | | | | 54° 9 | B; R; p s m b M; almost to a nucleus...................... | 128 | | | | | 55° 5 | v B; R; v s m b M, to a *; follows a * 7 m and is 3' S of it. | 336 | | 594 | III. 520| 9h 15m 20s| 99° 42' 26" | F; extended between 2 stars 12 & 16 m..................... | 129 | | 595 | III. 846| 9h 15m 24s| 31° 54' 7 | v F; p L; 1E; v g l b M; 35° l, 30" br .................. | 323 | | 596 | I. 260 | 9h 16m 10s| 26° 46' 41" | p B; R; p s b M; 20". Among stars ......................... | 411 | | | | | 10° 9 | p F; R; S; v g b M; 40"; a * 12 m follows. Δ AR = 16° 5; pos = 72° 6. | 404 | | 597 | II. 546 | 9h 16m 26s| 77° 49' 48" | The bisection at 16° 31° 1, 50' 33" ; dist of centres 2 ½' or 3' .. | 17 | | | | | 28° 6 | The preceding, brightest, and most condensed of two; both B; R; p s b M. | 120 | | | | | 29° 0 | The p of a double neb, both R; g b M; 40"; dist from each other 90" ±. The bisection observed at AR 16° 32° 0; P D 77° 50' 21"'. | 19 | | | | | 30° 7 | p F; S; R; p s b M; the n p of two. Pos of the other from this = 110° 6. | 242 | | | | | 32° 1 | v F; S; R; the n p of two. Pos of the foll 107° 3........ | 241 | | | | | 32° 2 | The first and brighter of two............................ | 123 | | No. | Synonym | AR 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 598 | II. 547 | h m s | o ' " | The f and fainter of 2 p B; p s b M ......................... | 120 | | | | 9 16 33'6 | 77 51 0 | The f of a D neb. R; g b M; 40" ................................ | 19 | | | | | 35'0 | F; R; g b M; the s f and larger of 2, pos from the 1st = 110°.6 | 242 | | | | | 35'7 | The fainter of two 25° s f .................................. | 123 | | | | | 36'1 | v F; S; R; the s f of 2 ..................................... | 241 | | | | | 36'2:: | The f of a double nebula. See II. 546,........................ | 17 | | 599 | Nova. | 9 17 59± | 66 15 17 | e F; v S; E in parallel; AR very uncertain .................. | 59 | | 600 | III. 555| 9 18 57'6 | 100 54 29 | p B; p L; R; v g l b M; 80". The MS makes the P D 101°, but two agreeing obs of my father prove this to be a mistake. | 129 | | 601 | Nova. | 9 19 59'4 | 31 46 37 | v F; R; v g b M; 15"; has a coarse D * 7' s .................. | 323 | | 602 | III. 297| 9 20 12'8 | 59 41 1 | F; v s m b M to a * 12 m .................................... | 56 | | | | | 13'2 | S; R; s b M; 20"; has a * 8 m 55° n f dist 3'. N.B. The working list very erroneous in P D. An extraordinary difference in these obs. | 115 | | 603 | III. 8 | 9 20 26'4 | 81 31 56 | 2 or 3 st and nebulosity .................................... | 116 | | 604 | I. 56 } | 9 22 32'2 | 67 45 5 | v B; v L; E; 3' long. An approach to a 2nd nucleus. See fig 70 | 59 | | | I. 57 } | | 32'3 | An e F, R, neb. Appended n f to a v L, R, v B, one p s b M, but not to a *. | 246 | | | | | ... | I. 56 is v B; E; g b M; r. Long attention shows a v F, L, R, neb attached n f. | 244 | | 605 | Nova. | 9 22 57'5 | 23 18 23 | e F; S; p s b M; 12" ........................................ | 412 | | 606 | II. 495 | 9 23 1'2 | 80 48 56 | p F; S; 1E .................................................. | 134 | | | | | 1'9 | F; not v S; R; g l b M ...................................... | 116 | | 607 | II. 506 | 9 23 38'0 | 105 59 36 | F; b M; 1 Esf; 30" .......................................... | 111 | | 608 | II. 40 | 9 24 38'5 | 79 6 0 | F; R; b M; 40"; the preceding of two ........................ | 123 | | 609 | III. 513| 9 24 56'3 | 79 8 30 | v F; R; b M to a nucleus; 25" ................................ | 123 | | 610 | II. 260 | 9 25 10'4 | 67 32 38 | No description .............................................. | 246 | | | | | 19'7 | F; S; R. Seen also in Sw. 244 in its place by working list, but no place taken. | 59 | | 611 | III. 298| 9 25 36'4 | 57 33 2 | F; R; v s b M almost to a * .................................. | 56 | | 612 | III. 963| 9 27 11'2 | 12 39 46 | e F; has a coarse D * 3' following .......................... | 414 | | 613 | Nova. | 9 28 53'7 | 55 14 5 | v F; v L; 1E parallel to merid; v g b M; has a * 10 m following | 128 | | | | | 53'8 | Not v F; L; R; v g l b M; 40" ................................ | 337 | | 614 | III. 4 | 9 29 1'7 | 79 42 56 | Not v F; S; 1E; p s b M .................................... | 134 | | | | | 3'9 | e F; R ....................................................... | 123 | | | | | ... | v F; R; v g b M; 30" ....................................... | 120 | | 615 | III. 519| 9 30 3± | 82 16 ± | e F; p L; v g b M. AR by working list ....................... | 116 | | 616 | IV. 68 | 9 30 4'5 | 30 23 37 | S; R; v s m b M, yet not to a nucleus ....................... | 323 | | | | | 6'3 | p B; R; s m b M; almost to a *. Has a * 11 m 20°'0 p and 15 or 20" n. AR very precarious. | 404 | | 617 | Nova. | 9 30 15'4 | 16 14 7 | e F; has a * 13 m near ..................................... | 382 | | 618 | Nova. | 9 30 38'0 | 20 37 19 | F; R; p L; v g l b M; 40"; is s of a S group of st .......... | 377 | | 619 | III. 315| 9 30 47'4 | 16 15 37 | v F; R; b M .................................................. | 382 | | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 620 | III. 541 | 9 30 56·1 | 53 20 57" | F; pL; R; vglbM; 30"; has * 18 m 30" p.................. | 331 | | 621 | Nova. | 9 31 50·8 | 85 37 57 | vF; R; g b M ......................... | 18 | | 622 | I. 114 | 9 32 45·7 | 57 25 ± | B; vL; E; vgbM; 2' l, 1½ br. PD estim.................. | 128 | | | | | 47·5 | B; vL; vglbM; E; 2½' by 1½'...................... | 127 | | | | | 47·8 | vB; vL; 1st class rather E; 2' ..................... | 337 | | | | | 47·8 | B; E; g b M; 60". The sp of two...................... | 56 | | 623 | III. 751 | 9 32 57·1 | 52 58 27 | vF; R; b M; filamentous (i.e. as if filaments hung round it: an effect probably of diverging lines of small stars, as in M 13. See fig of this last. This appearance therefore indicates its consisting of stars). | 331 | | 624 | II. 491 | 9 33 0·2 | 57 17 0 | pB; pL; E .................................. | 128 | | | | | 4·3 | pB; R; g b M; 30".......................... | 56 | | | | | 6·3 | B; pL; 60" .................................. | 337 | | | | | 6·5 | pB; R; vgbM; the nf of two ....................... | 127 | | 625 | I. 285 | 9 33 4·2 | 21 18 13 | B; vL; mE in pos = 332°·4; vglbM, 3' l, 1' br; has several S st in it, and one 12 m nearly at right angles to the axis of extension. | 411 | | 626 | II. 275 | 9 33 16·8 | 88 53 45 | pB; L; R; vglbM; 75"; r; well observed (and correctly reduced). | 113 | | | | | 22·4:: | F; L; R; vglbM; 50". AR approximate.............. | 397 | | 627 | Nova. | 9 33 20·2 | 57 12 54 | F; the foll and most northern of 3 ................. | 128 | | 628 | III. 527 | 9 33 30·3 | 97 49 20 | eF; R; vl b M.................................. | 136 | | 629 | I. 78 | 9 33 53·9 | 16 56 19 | vB; R; pgmbM; 50"; has a * 13 m following 1' dist, exactly in the parallel. | 382 | | 630 | I. 61 | 9 33 56·8 | 92 56 9 | B; R; b M. A * 9 m precedes 3°·0, and is s of neb .... | 21 | | 631 | III. 521 | 9 34 49·1 | 99 36 49 | pB; R; psbM.................................. | 129 | | 632 | III. 528 | 9 34 50·0 | 98 49 54 | eF; pL; vglbM.................................. | 136 | | | | | 54·7:: | F; R; b M; a hurried and imperfect obs ............ | 129 | | 633 | III. 34 | 9 35 49± | 78 14 ± | eF. AR from working list; PD rough approx........... | 123 | | | | | ... | vF; R; b M. PD only a rude approx ................. | 338 | | 634 | Nova. | 9 37 14·2 | 67 11 53 | F; vS; b M. The sp of two ......................... | 59 | | 635 | III. 277 | 9 37 31·6 | 103 32 56 | Not vF; R; b M; 30"............................. | 111 | | 636 | Nova. | 9 37 36·4:| 67 8 19 | F; vS; R; b M. The nf of 2; pos 40° nf ............. | 59 | | 637 | III. 278 | 9 37 38·1 | 103 35 11 | pF; R; b M; 25"............................... | 111 | | 638 | II. 717 | 9 38 7·3: | 45 7 12 | pB; irreg R; b M; r............................. | 139 | | 639 | V. 26 | 9 38 27·5 | 55 47 59 | A singular curved wisp of nebula. It curls up and tapers off at the sp side, and is clubbed at the nf extremity. | 51 | | 640 | Nova. | 9 39 6·4 | 44 53 34 | Not vF; R; b M; r. The first of 2 .................. | 138 | | 641 | Nova. | 9 39 12·4 | 44 52 0 | F; psbM; r; stars seen. The second of 2 ............ | 138 | | 642 | Nova. | 9 39 54·6 | 76 23 44 | F; pL; R; glbM; 50"............................. | 240 | | 643 | V. 23 | 9 40 25·9 | 17 0 3 | eF; vL; vglbM; 3' l; 2½' br ..................... | 382 | | 644 | Nova. | 9 40 32·9 | 94 25 21: | eF; L; 60". The preceding of two .................. | 234 | | No. | Synonym | R 1830-0. | N.P.D. 18300. | Description and Remarks | Sweep. | |-----|---------|-----------|---------------|------------------------|-------| | 645 | I. 115 | 9 40 50·5 | 55 39 34 | p B; R; b M; has a * 10 m 20° s f, dist 30" .................. | 51 | | | | | 53·9 | v F; R; b M; has a * 10 m s f................................. | 128 | | 646 | III. 51 | 9 40 52·3 | 76 23 9 | e F; p L; R ..................................................... | 338 | | | | | 53·0 | e F .............................................................. | 243 | | | | | 55·1 | v F; E nearly in parallel; v g b M; 30" l, 20" br ............ | 242 | | 647 | Nova. | 9 41 8·5 | 94 22 51 | F; R; v g l b M; r. The following of 2 ........................ | 234 | | 648 | III. 52 | 9 41 16·6 | 76 28 0 | v F; p L; E. P D estimated from III. 51, which precedes ....... | 242 | | 649 | M. 82 | 9 41 16·9 | 20 7 49 | e B; e L; E, pos = 156°·0; g b and then s v m b M, with faint rays of light nearly to extremities of field (15'). The most condensed part is 4' l and 3' br. | 377 | | 650 | Nova. | 9 42 13·4 | 59 58 41 | p B; S; p s b M; between 2 B st ................................ | 408 | | | | | 17·4 | A * 12 m with an e F neb atmos about 10 ... 12". It is between a * 8.9 m n p and one = 10 m, s f, neither of which are so affected. A curious object. | 115 | | 651 | II. 835 | 9 44 4·2 | 29 53 45 | p F; S; R ..................................................... | 406 | | | | | 14·9 | e F; p L; 35"; v g b M; has a * 10 m 7' n .................... | 323 | | 652 | III. 254| 9 44 53·6 | 87 37 44 | v F; m E, pos = 111°·5; 80" l, 15" br. Aurora in sky, even at this P D. | 397 | | 653 | II. 903 | 9 45 41·3 | 13 1 41 | Very doubtful. C and haze .................................... | 414 | | 654 | II. 333 | 9 46 1·4 | 17 0 57 | v F; S; R; 10"; near * 11 , 12 m ................................ | 382 | | 655 | II. 334 | 9 46 16·4 | 17 3 48 | F; R; 20"; v g l b M ........................................... | 382 | | 656 | VI. 4 | 9 46 23·4 | 84 55 38 | p B; g b M; r; 1 E; 60" l, 40" br; twilight. No other cluster or neb near. | 143 | | | | | 26·8 | e F; R; v g b M; a very condensed cl or r nebula. A * 8 m follows. | 238 | | | | | | e F; difficult to see for C. It is like a v F r neb 2 or 3' diam; precedes * 6 . 7 m about 1½m. | 237 | | 657 | II. 492 | 9 48 21·1 | 56 49 35 | F; 1 E; 30"; has * 9 m 6' f .................................. | 337 | | | | | 22·0 | p B; E; has a * 9 . 10 m n f .................................. | 51 | | | | | 22·5 | p B; p L; E in parallel; g b M; 60" l, 40" br; has * 10 m n f | 128 | | 658 | I. 286 | 9 48 33± | 20 26 45 | B; R; p s b M; 60". R from working list, but found in its place. | 377 | | 659 | I. 272 | 9 49 2·8 | 78 50 13 | p B; p L; R; g b M; 40" ....................................... | 123 | | 660 | III. 542| 9 49 31·1 | 53 47 17 | e F; R; v g v l b M; 60"; has a * 10 m in parallel, dist 7' .... | 331 | | 661 | III. 24 | 9 51 36·7 | 66 47 19 | v F; S ............................................................ | 59 | | 662 | III. 916| 9 52 27·8 | 29 4 51 | F; v S; R; b M; a coarse D * n f points to it; has a * 11 m 30" dist, pos 142°·2. | 406 | | 663 | Nova. | 9 52 38·7 | 64 28 23 | p B; S; m E in parallel; 30" l, 10" br; b M to nucleus .... | 58 | | | | | 42·2 | p B; m E; p s b M; 30" l; 10" br ................................ | 407 | | 664 | III. 478| 9 52 39·6 | 56 28 35 | e F; S ............................................................ | 337 | | | | | 40± | e F; doubtful .................................................. | 51 | | 665 | IV. 48 | 9 53 29·1::| 48 26 51:: | A v S * 14 m seems to have some nebulous appendage, but C troublesome. | 335 | | 666 | II. 320 | 9 54 13·3 | 57 59 42 | F; S; R; s m b M; is equal to a * 12 m ....................... | 56 | | No. | Synonym | AR 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 667 | Nova. | h m s | 9 55 19·5 | pB; R; sm bM; 20" | 138 | | | | | 19·8 | Not eF; S; R | 330 | | | | | 21·6 | B; R; ps m bM; almost to a * 12m | 329 | | 668 | I. 163 | 9 56 45·3 | 96 53 33 | vB; L; mE; vs m bM; almost to a nucl; 3' 1, 30" br. With 12 inches aperture, its nucleus is rather speckled; with 6 inches it is barely discernible as a neb. PD by MS 97°, but my father's obs makes it 96°. Each has but one obs. Of course I prefer 96. | 136 | | 669 | III. 65 | 9 59 2± | 70 45 ± | eF; S; R. Forms a triangle with 2 st. AR by working list; PD rough approx. | 332 | | 670 | Nova. | 9 59 9·3 | 79 12 0 | eF; S; ps bM; follows 31 Leonis 16·5, and is 1' 40" s of it | 123 | | 671 | Nova. | 9 59 16·0 | 70 56 6 | pB; p m E; g b M; 40" 1, 20" br. Found in looking for III. 65 by working list. | 334 | | 672 | Nova. | 10 0 17·0 | 43 12 27 | F; R; g b M; 25" | 139 | | 673 | III. 518| 10 1 49·6 | 101 35 29 | F; L; R; vg b M; 60". In field with λ Hydræ. | 129 | | 674 | I. 79 | 10 2 8·9 | 15 45 46 | vB; L; R; at first vg, then vs, vm b M | 382 | | 675 | Nova. | 10 2 52·5 | 38 40 33 | A star 7 m has a photosphere 2 or 3' diam. Sky perfectly clear; glass quite clean; windy. Another * of same magnitude viewed presently after has no photosphere. | 328 | | 676 | Nova. | 10 3 ± | 14 45 ± | vF; S; R. AR extremely precarious. | 171 | | 677 | III. 53 | 10 3 31·7 | 76 29 59 | eF; pL; R. | 242 | | 678 | II. 639 | 10 3 43·5:: | 50 24 39:: | B; R; ps b M; 35" | 335 | | 679 | Nova. | 10 3 47·6 | 32 29 57 | eF; R; vg l b M; 15" | 323 | | 680 | III. 255| 10 3 51·9 | 86 1 38 | pB; S; R; ps b M; 15" | 143 | | 681 | II. 640 | 10 4 0·5:: | 50 31 21:: | F; R; g b M; 30" | 335 | | 682 | II. 43 | 10 4 2·3 | 66 25 20 | pB; L; R; gl b M; a * 10 m precedes | 244 | | | | | 3·9 | Not vF; L; R; vg l b M; 70" | 246 | | | | | ... | pB; pL; b M; r | 59 | | 683 | Nova. | 10 4 39·5 | 28 55 45 | F; ps b M; like a star rubbed out. A * 7·8 m in field np—dist 5'. | 406 | | 684 | I. 3 | 10 4 54·9 | 85 44 18 | B; pS; R; ps b M; 25" | 143 | | | | | 56·4 | pB; R; ps b M; 20...30" | 238 | | | | | 57·1 | B; R; ps m b M; the preceding and brighter of two. Δ AR = 29·25 | 237 | | | | | 64·8:: | B; R; g b M; 60". The p of 2. (The AR very precarious, the chronometer not being then in use.) | 18 | | 685 | I. 4 | 10 5 24·2 | 85 41 30 | B; R; ps b M; 30". Has a * 10 m 20° nf, dist 90" .......... | 143 | | | | | 24·7 | B; R; pg m b M; the foll and fainter of 2. Δ AR = 29·25.. | 237 | | | | | 26·2 | pB; 1E; 30"; has * 12 m nf; pos 78°·2; 70" dist .......... | 238 | | | | | 33·8:: | B; R; gm b M; 60"; the foll of 2. AR very precarious .. | 18 | | 686 | Nova. | 10 5 39·6 | 42 33 47 | F; S; R. | 139 | | 687 | III. 25 | 10 7 11·2 | 68 1 31 | Not vF; S; R; ps b M; 16" | 246 | | | | | 12·0 | Not vF; S; R; ps b M | 244 | | | | | 12·7 | pB; pL; R | 59 | | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 688 | I. 168 | 10 8 1·2 | 47 44 7 | F; vL; R; vg bM; a * 8 m p, 10' dist. .................. | 248 | | 689 | Nova. | 10 8 4·5 | 47 32 11 | pF; vL; R; vg bM; 12·5 of time in diam; has a * 11 m 2' north. | 335 | | 690 | III. 910| 10 8 15·6| 31 44 12 | eF; pL; 30'' .............................................. | 323 | | 691 | Nova? | 10 8 34·0| 42 42 52 | F; S; R; bM; 15 ... 20''. If this be III. 704, there must exist a great error in P D on one or other side. | 139 | | 692 | II. 44 | 10 8 42·6| 67 19 5 | B; pmE; psbM .............................................. | 244 | | | | | 42·3 | pB; E; g bM; 45'' 1, 40'' br ................................ | 246 | | | | | 44·8 | B; E; sbM to nucl; 60'' 1; the sp of 2 .................. | 59 | | 693 | II. 45 | 10 9 1·5 | 67 15 35 | B; R; has a * 8 m n, dist 60''. The nf of 2 ............ | 59 | | | | | 2·0 | pB; R; psbM; pos of a * 10 m from neb = 352° 0 ......... | 244 | | | | | 2·2 | B; R; psbM; 30''; has * 10 m n p, 90'' dist. .......... | 246 | | 694 | III. 348| 10 9 11·7| 61 29 31 | So eF that I remained unsatisfied ....................... | 57 | | 695 | I. 199 | 10 9 23·3| 43 35 19 | F; vL; bM; mE; 6' 1, 2½' br; r .......................... | 140 | | 696 | II. 720 | 10 10 16±| 46 9 45 | vF; R; vg bM; 30''; the preceding of 3 neb in a triangle. Some stars near. | 248 | | 697 | I. 266 | 10 10 30·6| 32 13 7 | vF; L; E; vglbM; 2' 1; 1½' br .......................... | 323 | | 698 | Nova. | 10 10 31·0| 61 19 57 | F; L; 40 ... 60''; gbM ................................... | 115 | | 699 | II. 721 | 10 10 32·5| 46 11 52 | vF; R; vg bM; 30''; the second of 3 in a triangle ...... | 248 | | 700 | II. 722 | 10 10 44·1| 46 9 52 | vF; R; vg bM; 30''; the last of 3 in a triangle ....... | 248 | | 701 | Nova. | 10 11 6·0 | 63 38 48 | F; R; 30''; has a * ..................................... | 58 | | 702 | III. 330| 10 12 14·7| 65 12 54 | eF; R; 20'' .............................................. | 407 | | 703 | II. 882 | 10 13 42·2| 31 0 17 | pF; L; E; vg bM; 30 ... 40'' ............................ | 323 | | 704 | Nova. | 10 14 11·9| 22 20 3 | A cluster of 20 stars more or less, 10, 11 and 12 m, scattered over a space 10' diam. A star 7 m s. | 412 | | 705 | Nova. | 10 14 38·9| 76 35 4 | A very close D * of the first class involved in a nebulous wisp. "A most curious, delicate and interesting object." This is my double star No 2529. | 243 | | | | | 39·2 | A triple star in a nebula, a fourth * suspected .......... | 242 | | | | | 40·5 | A double * in vF nebula .................................. | 338 | | 706 | Nova. | 10 14 57·3| 62 7 2 | pB; R; psbM; 30'' ...................................... | 115 | | 707 | Nova. | 10 15 12·3| 27 52 13 | eF; S; psbM; 8''; 2 st 11 and 12 m follow .............. | 406 | | 708 | III. 883| 10 15 29·1| 31 55 22 | Not vF; R; psbM; 20'' .................................. | 323 | | 709 | III. 631| 10 15 41·0| 49 30 46 | pF; R; S; pg bM; 10 ... 12'' ............................ | 335 | | 710 | IV. 10 | 10 15 53·1| 71 59 2 | A * 9 m, with vF neb. atmosph, rather excentric. Has 2 st p and ? another vS * f. | 332 | | | | | 53·2 | A * 9 m, with a vF neb. The * is excentric, and has another * foll at extreme edges. | 63 | | 711 | I. 86 | 10 17 42·6| 60 37 5 | vB; R; gm bM; 40'' ...................................... | 68 | | | | | 43·1 | vB; R; psmbM; r; 40'' .................................. | 408 | | | | | 43·5 | vB; mE; vsmbM; 40'' 1, 15'' br ........................ | 343 | | | | | 43·9 | B; E; comes up to a nucleus ............................ | 57 | | | | | 38 31 | vB; E; comes to nucleus. Transit missed ................ | 66 | | No. | Synonym | R 1830.0 | N.P.D. 1890.0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 712 | Nova. | 10 17 52·5 | 85° 16′ 38″ | e F; S; R; two st, 10 and 11 s p, dist 90″ | 142 | | | | | | e F; has a * 6 m, 30° n p, dist 8′ | 143 | | | | | | Viewed. It is 31°·5 foll a * 6.7 m, and makes a triangle with 2 S st. | 238 | | 713 | II. 374 | 10 18 22·2 | 66 17 25 | p B; R; S; ps b M; 15″ | 244 | | | | 23·0 | 17 17 | No description | 246 | | | | | | F; S; b M | 59 | | 714 | I. 72 | 10 19 43·5 | 59 38 19 | p B; E; b M | 68 | | | | 47·3 | 38 37 | p B; R; s b M | 6 | | | | | | F; R; ps b M; 40″; has coarse D * 23°·0 f | 341 | | 715 | II. 870 | 10 20 34·7 | 24 5 41 | F; R; g b M; 18″ | 411 | | 716 | Nova. | 10 21 21·4 | 33 2 27 | e F; between 2 S stars | 323 | | 717 | II. 871 | 10 21 22·1 | 24 23 6 | v F; R; ps m b M; almost to a star | 411 | | 718 | III. 349| 10 21 32·3 | 60 20 18 | p F; a * very near or else extended | 408 | | | | 34·2 | 20 17 | p B; R; ps b M | 343 | | | | 35·4 | 20 32 | p F; S; b M; has a * s f | 115 | | | | 36·4 | 20 32 | v F; S; R | 57 | | 719 | III. 331| 10 22 4·2 | 64 15 18 | F; E; g b M | 58 | | 720 | II. 358 | 10 22 45·0 | 61 27 23 | F; R; 25″ | 415 | | | | 45·3 | 27 56 | v F; R; gl b M; 30″ | 408 | | | | 47·1 | 27 31 | F; has a D star f | 66 | | | | 50·3 | 28 22 | p B; p L; R; b M | 115 | | 721 | II. 359 | 10 23 22·3 | 60 36 32 | B; R; g b M; 30″ | 68 | | | | 23·3 | 37 28 | p B; v S; R | 57 | | | | 23·4 | 37 26 | B; R; pg m b M; 15″ | 408 | | 722 | III. 917| 10 25 10·9 | 30 30 57 | v F; p S; R; ps l b M; 15″ | 323 | | 723 | III. 918| 10 25 14·4 | 30 34 17 | e F; S; R; vg l b M; 12″ | 323 | | 724 | I. 164 | 10 26 28·6 | 51 48 2 | p B; m E; gl b M; 2′1, 45″, br | 331 | | 725 | III. 767?| 10 26 53·7 | 39 0 36 | v F; two distant stars nearly on parallel | 329 | | 726 | III. 54 | 10 27 22·0 | 76 25 23 | p L; so faint as to be barely perceptible, but a sure observation. | 338 | | 727 | III. 55 | 10 27 34·1 | 74 57 2 | F; R; g b M | 24 | | | | 35·0 | 57 34 | e F; S; R; ps b M; 10″ | 243 | | 728 | II. 46 | 10 27 38·7 | 67 14 19 | B; R; ps m b M; 35″ | 244 | | | | 40·6 | 14 38 | B; E; nearly lost by looking too late | 59 | | | | | | No descrip. P D only rudely taken to satisfy myself of an error in my father's place, as shown in the working list. | 246 | | 729 | III. 615| 10 27 48·4 | 51 40 2 | e F | 401 | | | | 51·3 | 40 17 | v F; S; ps b M; 12″ | 331 | | 730 | III. 66 | 10 27 49·5 | 70 59 57 | v F; v S; R; Ib M | 63 | | | | 50·0 | 59 6 | v F; S; R; g b M; 12″ | 334 | | 731 | IV. 60 | 10 28 6·6 | 35 36 32 | B; R; v s m b M, so as to form almost a disc 15″ diam. Surrounded by a v feeble atmosphere. See fig 40. | 324 | | No. | Synonym | RA 1830-0 | NP.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|-------------|------------------------|-------| | 732 | II. 745 | 10 29 22·4 | 41 43 6 | F; mE; between a * 10 m and 1 of 14 m .................. | 329 | | | | 25·6 | 41 17 | vF; E in a direction between 2 small stars 13 m and 11 m, from s p to n f. (Fog.) | 330 | | 733 | Nova. | 10 29 52·2 | 12 17 24 | pB; S; psmbM ......................... | 413 | | | | 57± | 16 ± | pB; irreg R; psmbM; 15" .................. | 171 | | | | 61·2 | 18 11 | pB; lE; gbm; 25". The obs makes the P D 13°, but there can be no doubt that this neb is the same as that of the two preceding observations. | 414 | | 734 | II. 348 | 10 30 37·7 | 65 1 48 | vF; R; gbm; 30" ....................... | 407 | | | | 39·2 | 1 38 | vF; S; has either a * which gives it an apparent elongation in parallel, or is a double nebula. | 58 | | 735 | II. 641 | 10 31 45·0 | 51 48 56 | vF; R; bM ................................ | 401 | | | | ... | 47 ± | F; R; 30". Taken much out of merid. P D only approximate. | 331 | | 736 | III. 317| 10 32 55·9 | 15 45 28 | not vF; R; gbm ....................... | 382 | | 737 | II. 77 | 10 33 6·3 | 75 22 7 | F; E; pL; 60...90" .................... | 24 | | | | 7·3 | 22 39 | F; E; pL; vgbm; follows a * 7 m 10°0 ............. | 242 | | 738 | I. 80 | 10 34 9·6 | 16 15 59 | B; R; psbM; 40"; has * 11 m pos 281°8, ΔRA = 20°0.. | 382 | | 739 | I. 81 | 10 34 10·6| 64 10 58 | pB; L; gbm; has (?) a * excentric within it and a double * closely following it. | 58 | | 740 | I. 26 | 10 34 33·3| 77 7 19 | eF; hardly visible .................... | 243 | | 741 | III. 842| 10 34 45·7| 33 9 7 | pB; S; R; pgbm; 15"; a S * 90" s .............. | 323 | | 742 | Nova. | 10 34 53·0| 58 22 58 | eF; vS; very difficult, but a certain obs; is n of 2 st 9 or 10 m. Sky perfectly clear. | 342 | | 743 | M. 95 | 10 34 54·5| 77 25 9 | vB; L; R; gmbM; 2' diam. RA only approximate .... | 19 | | | | 60·6 | 24 43 | B; R; pgbm; r; 150" diam .................. | 338 | | | | 62·2 | 24 4 | Just seen through a thick cloud .............. | 240 | | | | ... | 26 ± | F; L; gmbM; r; 3' diam. Approx place ............ | 243 | | | | ... | .......... | Viewed; vF; E; r; 30 or 40" (probably cloudy); a star precedes. A very doubtful obs. | 2 | | 744 | III. 107| 10 35 19·1| 82 21 16 | eF; R; bM; 30"; a * 9 m s dist 2' or 3' ............ | 117 | | | | 19·2 | 21 34 | F; S; R; bM; 20" ........................ | 250 | | 745 | V. 52 | 10 35 20·5| 25 53 1 | pF; L; E in merid; glbm; 2½ l, 2' br ............. | 411 | | 746 | III. 318| 10 35 39·6| 16 40 13 | eF; L; R; vgbm; 60"; a coarse d * sf points back directly to it. | 382 | | 747 | Nova. | 10 37 26·8| 87 19 7 | eF; L; 2' l, 20" br; vgvlbm; a ray neb ............ | 144 | | 748 | II. 78 | 10 37 34·4| 75 21 38 | pB; vL; irreg R; vgbm; 2' diam .................. | 338 | | | | 35·2 | 21 34 | pB; L; R; vgbm; the preceding of 3 in a triangle. Pos of 1 and 2 = 68°4; of 2 and 3 = 156°8. | 242 | | 749 | M. 96 | 10 37 42·4| 77 18 11 | vB; L; R; gmbM; r; 2' diam .................. | 19 | | | | 43·1 | 17 34 | vB; pL; smbM; almost to a nucl. Seen at the same time by M. Knorre. | 22 | | | | 46·8 | 17 17 | vF (cloudy); R; psbM; a good obs of place ........ | 240 | | | | 48·5 | 17 0 | vB; vL; E; vsvmbM; 6' l, 5' br .............. | 340 | MDCCCXXXIII. | No. | Synonym | JR 1830-0. | N.P.D. 1830-0. | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 750 | II. 81 | h m s | 10 37 57'9 | B; R; pL; pgbM; 35" | 334 | | | | | 58'4 | pB; R; bM; r | 63 | | 751 | Nova. | | 10 38 1'7 | F; R. The second of 3 in a triangle | 242 | | 752 | III. 701| | 10 38 4'2 | vF; S; R; 12" | 248 | | 753 | Nova. | | 10 38 13'7 | F; R; the last of 3 in a triangle | 242 | | 754 | II. 99 | | 10 38 40'5 | vB; R; sbm to a *; 45" | 418 | | | | | 41'6 | B; R; smbM; 30". Sky clearing after clouds | 241 | | | | | | vB; first Class; vsvmbM; 90" | 419 | | 755 | II. 360 | | 10 38 45'2 | B; R; smbM; 30" | 65 | | | | | 46'7 | pB; R; bm; 25" | 343 | | | | | 48'2 | B; R; sbM; 30" | 66 | | | | | 48'7 | F; S; R; bM | 57 | | | | | 49'7 | No description | 115 | | 756 | II. 565 | | 10 38 49'0 | F; R | 51 | | | | | 54'0 | pB; L; R; vgbM; 90" | 128 | | 757 | I. 17 | | 10 38 50'1 | vB; pL; R; psvmbM; 50" | 338 | | | | | 50'5 | vB; R. The first of 3 | 243 | | | | | 50'7 | vB; L; R; psbM; 50". (Seen also in Sweep 2.) | 240 | | 758 | I. 18 | | 10 39 16'7 | vB; L; R; psbM; 40". The second and most n of 3 | 240 | | | | | 16'9 | vB; R. The second of 3 | 243 | | | | | 17'1 | vB; R; psbM; 30". (Seen also in Sweep 2.) | 338 | | 759 | Nova. | | 10 39 21'4 | vF; R | 142 | | 760 | Nova. | | 10 39 21'5 | eF; E | 238 | | | | | 22'9 | pB; R; bM; 15" | 142 | | 761 | II. 41 | | 10 39 28'1 | F; E; vglbM; the last of 3 | 338 | | | | | 28'8 | F; L; the following of 3 | 242 | | | | | 30± | barely visible; pL. Place estimated from the position with respect to the others. | 243 | | | | | | vF; diluted; E in parallel; 15" | 2 | | 762 | Nova. | | 10 39 29'0 | Suspected nebula. Has a B * near | 238 | | 763 | II. 881 | | 10 39 33'5 | eF; S; psbM; near some stars | 412 | | 764 | II. 872 | | 10 39 57'5 | vF; L; 1E; vgbM; 50" l, 45" br | 412 | | 765 | I. 116 | | 10 40 20'5 | pB; S; E. The sp of two; dist ½ diam | 51 | | | | | 22'6 | B; R; bM | 128 | | | | | | The p of 2; pos of the other 20° n f, dist 80. The first is the brightest. | 125 | | 766 | I. 117 | | 10 40 24'2 | pB; S; E. The second and fainter of 2 | 51 | | | | | 29'1 | pB; E; is n f the nebula I. 116 | 128 | | | | | | The second and fainter of 2; pos 20° n f. Hazy. Place uncertain. | 125 | | 767 | II. 335 | | 10 40 57'1 | pF; L; E; vgbM; 60" l, 40" br | 382 | | No. | Synonym | AR 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|-------------|----------------|------------------------|--------| | 768 | II. 361 | 10 41 22·2 | 60 38 17 | pB; R; bM; 20" | 343 | | | | 23·1 | 38 19 | F; S; R | 57 | | | | 23·4 | 38 11 | pF; R | 66 | | 769 | III. 919| 10 41 23·8 | 27 43 38 | eF; S; R; 6" | 406 | | 770 | III. 913| 10 41 27·5 | 30 40 17 | vF; S; R; is 12" n of 2 p b st forming an isosceles triangle | 323 | | 771 | Nova. | 10 41 29·0 | 38 4 23 | pB; 2nd class; R; pg bM; among many stars | 328 | | 772 | II. 718 | 10 41 48·4 | 45 23 22 | B; S; R; the 2nd and northern of a trapez of stars 11 and 12 m | 248 | | 773 | II. 362 | 10 41 53·5 | 61 7 8 | B; R; gbM | 68 | | | | 53·6 | 7 58 | B; R; smbM; 30" | 65 | | | | 54·5 | 7 27 | B; pL; R; pgmbM | 343 | | | | 55·7 | 8 12 | vB; R; vmbM; 60" | 115 | | 774 | I. 27 | 10 41 53·9 | 75 41 13 | B; R; vsmbM almost to a*; 30" | 241 | | | | 54·9 | 41 30 | B; R; psbM; 50"; r | 340 | | 775 | II. 363 | 10 42 1·5 | 60 59 27 | F; L; R; bM | 343 | | | | 3·4 | 59 58 | pF; R; psbM | 415 | | | | | 59 52 | vF; S; gbM; 20". Too late for RA | 115 | | | | | 59 44 | vF; R; RA missed | 57 | | 776 | III. 522| 10 42 10± | 101 57 ± | vF; R; bM. RA from working list | 129 | | 777 | IV. 6 | 10 42 21·0 | 83 15 36 | F; vL; irr R; vg bM; r; 2' diam; no other seen. This neb is identical with III. 88 and II. 131. | 250 | | | III. 88 | 24·1 | 15 34 | F; vL; R; vg bM; at least 4' diam; no other near | 117 | | | II. 131 | 25·7 | 15 22 | vL; R; 3' diam; vg bM; r. Directing the eye aside, the stars in it were seen as infinitely minute points. In the 40-feet reflector it would no doubt be seen as a globular cluster. | 251 | | 778 | II. 494 | 10 42 21·1 | 56 12 22 | B; E in a wisp; the sp of 2 | 128 | | | | | 13 ± | F; the sp of three. PD very rough | 337 | | 779 | Nova. | 10 42 47·1 | 56 8 40 | B; L; E; gbM; the nf of 2 | 128 | | | | | 7 ± | pB; pmE; the second of three. PD rough | 337 | | 780 | I. 172 | 10 42 50·1 | 52 29 5 | vF; a long ray pos = 40°8'; has a D class 4 in middle, and one more. | 401 | | | | 57·1 | 28 52 | pB; vme; 90° l, 12" br; pos = 44°2'. Its southern extremity touches the L * of a D *. Can this nebula have moved? | 331 | | 781 | II. 887 | 10 42 58·9 | 27 48 51 | eF; 1E; S; vg bM; 15" | 406 | | 782 | Nova or I. 118 | 10 43 ± | 56 1 ± | B; L; the nf of three in a line. This neb may possibly be I.118, as none exists in the place indicated by my Father (1°32' s of 46 Ursae). | 337 | | 783 | III. 20 | 10 43 6·1 | 78 57 17 | eF; vL; R; vg lbM; 2' diam | 120 | | 784 | III. 497| 10 43 10·1 | 85 18 46 | pB; R; vg lbM; 30" | 142 | | 785 | III. 914| 10 43 18·7 | 31 58 57 | No description | 323 | | 786 | II. 47 | 10 43 21·2 | 66 9 48 | B; pL; E 30° np to sf = pos 120° | 59 | | | | 21·8 | 10 13 | pB; 1E; gbM | 244 | | | | | 10 8 | pB; 1E; bM; 40". RA lost | 246 | | 787 | I. 267 | 10 44 6·5 | 32 6 47 | pB; L; R; vg lbM; has * 10 m 2' nf | 323 | | No. | Synonym. | R 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|----------|------------|----------------|-------------------------|-------| | 788 | I. 283 | 10 44 15·2 | 34 47 17 | B; mE; g b M; no nucl; 1¾' l, 20'' br; pos = 67°.0 ........ | 324 | | 789 | II. 364 | 10 44 56·0 | 61 51 22 | p L; E; b M; 90'' l ........................................... | 115 | | | | | | e F; R; 40'' .................................................. | 65 | | | | | | F; L; R; v l b M; 60'' ....................................... | 66 | | | | | | p B; S; R; b M ................................................ | 57 | | 790 | Nova. | 10 45 24·8 | 71 45 1 | p F; 1E; the n p of two ...................................... | 334 | | 791 | II. 82 | 10 45 26·8 | 71 48 41 | p B; E; g b M. The s f of 2; a * 9.10 m between them .... | 334 | | | | | | No R A observed ............................................... | 63 | | 792 | IV. 29 | 10 45 42·8 | 105 7 25 | A * 12 m with an extremely F neb appendage. At first it seemed to envelope the *; but Mr. Dunlop, to whom I showed it, considered it to be detached. | 111 | | 793 | Nova. | 10 45 45·6 | 71 29 22 | Stellar. 2 or 3 stars with a nebulous burr observed by Mr. Baily. | 63 | | 794 | II. 16 | 10 46 28·0 | 81 24 9 | v F; S; R; p s b M; 12'' ..................................... | 250 | | 795 | Nova. | 10 46 36·9 | 13 54 6 | e F; p L; R; v g l b M; 30''; a D * n f points to it ...... | 413 | | | | | | e F; a D * points to it ....................................... | 414 | | 796 | Nova. | 10 47 23·3 | 79 21 15 | v F: has another still fainter following; has also a * 9 m preceding in the same parallel. | 120 | | 797 | III. 632 | 10 47 51·0 | 48 8 18 | F; S; R; g b M; 15'' ......................................... | 335 | | | | | | not v F; S; R; p s b M; 12''; a * 13 m near ................ | 248 | | 798 | Nova. | 10 47 51·8 | 79 20 15 | v F; R; v s m b M to a * 12 m ................................ | 120 | | 799 | II. 888 | 10 48 12·8 | 29 35 13 | e F; R; v g b M; 15'' ......................................... | 406 | | 800 | III. 332 | 10 49 12·2 | 64 51 43 | v F; R; g b M; 2' s of a * 13 m ................................ | 407 | | 801 | III. 705 | 10 49 34·1 | 42 58 42 | F; S; R .......................................................... | 139 | | 802 | III. 967?| 10 50 8·9 | 13 16 11 | A very doubtful object ....................................... | 414 | | 803 | I. 269 | 10 50 59·7 | 31 25 17 | e F; 1E; 40''. It is n of a * 13 m, just at the edge of the neb | 323 | | 804 | II. 100 | 10 51 0·9 | 74 16 54 | F; L; R; g l b M; 85'' ....................................... | 418 | | | | | | p B; L; E; has a * 11 m 7·5 s p ................................ | 419 | | | | | | F; p L; 90'' .................................................. | 24 | | 805 | I. 87 | 10 51 3·2 | 60 7 2 | B; L; R; p s b M; 2' ......................................... | 343 | | | | | | v B; v L; R; s m b M; 90'' .................................. | 65 | | | | | | p B; v L; R; g b M; r ....................................... | 68 | | | | | | v B; E; p s m b M; 60'' l, 40'' br ................................ | 415 | | | | | | No description ................................................ | 416 | | | | | | F; L; b M; 50'' .............................................. | 57 | | | | | | p B; R; p g m b M; r ....................................... | 341 | | | | | | v B; L; R; s b M; 90'' ....................................... | 66 | | | | | | B; L; R; g m b M; 50''; r. No doubt a distant globular cluster | 342 | | | | | | p B; R; r; seen through cloud ................................ | 56 | | 806 | II. 101 | 10 51 21·0 | 75 11 28 | v B; first class; 1E; p s b M, r ................................ | 338 | | | | | | v B; first class; R; v s m b M, almost to * 11 m ............ | 241 | | 807 | III. 21 | 10 51 39·8 | 76 55 39 | e F; R .......................................................... | 242 | | No. | Synonym | RA 1830°-0 | N.P.D. 1830°-0 | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 808 | Nova. | 10 52 10·2 | 61 22 17" | vF; R; bM | 343 | | | | | | eF; has a S * sp | 115 | | 809 | III. 498| 10 52 26·4 | 85 27 8 | No description | 143 | | | | | | F; mE, 60° with merid.; 60" l; 15...20" br | 141 | | | | | | eF; sky perfectly clear | 142 | | 810 | I. 88 | 10 53 55·0 | 61 6 20 | pB; E. Pos by diag 120°±. Nucleus has stars in and about it | 68 | | | | | | B; E; vs vmbM, to nucl.; many vS stars about it | 343 | | | | | | vB; a * 10 m with an E neb and a S * 25" f | 415 | | | | | | B; pL; R; smbM to a *; 60"; r; st seen | 65 | | | | | | pB; S; E; comes up to nucleus | 57 | | | | | | Viewed past merid. vB; E; smbM; has a : f involved | 115 | | | | | | B; mE; comes up to a nucleus | 66 | | 811 | III. 22 | 10 54 18·9 | 78 0 15 | F; R; bM | 340 | | | | | | F; S; R; vgv1bM | 120 | | | | | | eF; R | 242 | | 812 | IV. 7 | 10 54 22·4 | 70 56 52 | a * 9 m with vF neb attached; pos 70° sp = 200°-0 ± dist 30" | 63 | | | | | | vF neb with a vF nucl.; has * 10 m, n f dist ½ diam of n from edge; pos = 30°-0, and another sp of 10 m dist 3' | 334 | | 813 | II. 365 | 10 54 26·9 | 60 11 41 | Has a * 7 m dist 8' pos 40° np | 66 | | | | | | pB; mE; nearly in merid.; bM | 115 | | 814 | II. 507 | 10 54 34·8 | 105 22 24 | F; 1E; bM; vL; involves a * 45° nf from the nucleus | 111 | | 815 | Nova. | 10 54 49·9 | 61 2 9 | F; R; pgbM; 35"; sky dull | 416 | | 816 | II. 336 | 10 54 53·8 | 16 30 42 | A singular object. A burred star 11 m diam 12"; vsmbM; a D * follows. | 382 | | 817 | II. 884 | 10 55 24·4 | 32 33 47 | eF; R; 12"; vg1bM | 323 | | 818 | I. 13 | 10 57 6·4 | 89 7 17 | vB; L; mE (pos by diag = 140° ±); 4' l, 1' br; vs vmbM. The nucleus is rather excentric, being rather towards the s p side. | 144 | | 819 | III. 23 | 10 57 39·0 | 77 41 28 | pF; S; 1E; sf a * 12 m | 338 | | | | | | vF; R; bM; has 2 st exactly in a line with centre (by diag np), one 11.12 m, the other 13.14. | 242 | | | | | | not vF; E; psbM; sf a * 11 m | 340 | | 820 | III. 350| 10 58 0·9 | 60 33 41 | eF; has a * 10.11 m, 60" p | 66 | | | | | | eF; a * 10 m precedes, and a D * points downwards (to s) between them. | 68 | | | | | | The faintest imaginable. Follows 1' a * 11 m | 65 | | | | | | Follows a star. (Evidently a hurried obs.) | 57 | | 821 | III. 915| 10 58 32·3 | 31 51 47 | eF; S; R; pgbM; 10" | 323 | | 822 | Nova. | 10 59 41·1 | 60 37 32 | F; S; R; bM; 15...20" | 115 | | 823 | III. 111| 10 59 44·0 | 84 15 3 | F; R; bM; sky perfectly clear | 143 | | 824 | Nova. | 10 59 52·6 | 53 3 2 | pF; R; psbM; 20"; a * 7 mp dist 7'...8' | 331 | | 825 | Nova. | 10 59 53·4 | 60 24 47 | eF | 343 | | 826 | III. 920| 11 0 38·8 | 27 44 18 | eF; S; 15"; appears hairy | 406 | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|----------|-----------|---------------|-------------------------|-------| | 827 | Nova. | h m s | 53° 2′ 52″ | e F; R; a * 8 m precedes | 401 | | 828 | II. 42 | 11 1 4′8 | 78 21 15 | F; S; 1 E; of nearly uniform brightness | 120 | | 829 | III. 351 | 11 1 25′4 | 60 18 33 | p B; has a * foll, dist 1′ | 415 | | | | | 25′4 | p F; R; 25″; the first of a group of 4 | 343 | | | | | 25′8 | v F; S; R | 115 | | | | | 26′3 | F; S; R; b M; 20″, a B * follows, dist 1′ | 66 | | | | | 27′4 | B; S; precedes a * 9 m dist 1′. The first of a group | 65 | | | | | 34′9 | e F; 1′ preceding a * 9 m | 68 | | 830 | II. 337 | 11 1 25′4 | 16 12 16 | p F; 1 E; g b M; 20″; a * 15 m dist 70″; pos from neb = 22°1 | 382 | | 831 | V. 46 | 11 1 26′4 | 33 25 0 | B; v l; p b r; v m E; pos 79°0. Has a distinct * in centre and 1 or 2 v S st elsewhere. | 324 | | 832 | III. 352 | 11 1 29′4 | 60 24 37 | v F; the second of 4 | 343 | | | | | 30′9 | e F | 415 | | | | | 35′8 | So excessively F as hardly to be discerned on long attention. The second of a group of 3. | 65 | | 833 | Nova. | 11 1 34′4 | 60 26 37 | e F; the third of a group of 4 | 343 | | | | | ... | F; R; b M; not v S; P D mistaken 10′; corrected | 115 | | 834 | III. 79 | 11 1 51′9 | 77 53 50 | F; R; g b M; 20″ (conspicuous). The P D of the working list is 6′ out, owing to which I have often before looked for it in vain. | 340 | | 835 | Nova. | 11 1 57′9 | 60 24 37 | v F. The last of a group of 4 | 343 | | | | | 58′3 | F; p L; 8′ dist from another (III. 351) and 30° s f it | 66 | | | | | 59′4 | e F; the last of 3 | 65 | | 836 | III. 89 :: | 11 2 27′9 | 83 15 34 | v F; wind furious; perhaps only F stars | 251 | | | | | 30′5 | e F; R; s b M; with an appearance of stars | 117 | | 837 | Nova :: | 11 4 24′8 | 105 2 ± | A doubtful object, but probably a nebula | 111 | | 838 | M. 97 | 11 4 49′4 | 34 3 52 | A large uniform nebulous disc, diameter 19°0 of time in RA. Quite round, v B; not sharply defined, but yet very suddenly fading away to darkness. A most extraordinary object. See fig 32. | 324 | | 839 | III. 921 | 11 5 3′3 | 28 22 43 | v F; L; v g v l b M; 45″; situated in the centre of gravity of a triangle of 3 large stars 5′ distance. | 406 | | 840 | I. 29 | 11 5 39′2 | 76 16 23 | B; E; p s m b M; 40″1, 30″ br | 22 | | | | | 42′4 | No description | 242 | | | | | 43′9 | No description | 338 | | | | | ... | v F; b M; E in parallel; 20″; viewed and only a rough place taken. | 2 | | 841 | II. 102 | 11 6 9′2 | 74 17 14 | No description | 418 | | | | | ... | p F; v L; g b M; 2′ diam | 419 | | 842 | II. 709 | 11 6 26′4 | 47 28 42 | p B; S; 1 E; v g b M; 20″ | 248 | | 843 | II. 49 | 11 6 29′0 | 70 57 56 | B; R; p s m b M; 35″ | 334 | | 844 | III. 27 | 11 7 44′0 | 71 5 7 | p F | 63 | | | | | 49′5 | F; S; R; 12″ | 334 | | No. | Synonym | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|------------|----------------|------------------------|-------| | 845 | II. 50 | 11 7 54'0 | 71 2 12" | vB; R | 63 | | | | | 57'0 | vB; L; R; vmbM; 35" | 334 | | 846 | II. 51 | 11 7 59'5 | 70 56 2 | vB; R | 63 | | | | | 61'0 | pB; pL; R; psbM; 30" | 334 | | 847 | I. 270 | 11 8 21'5 | 30 17 43 | vB; pS; lE; vsvmbM | 406 | | | | | 26'1 | B; R; vsvmbM to a * 11m| 344 | | | | | 27'7 | pB; pS; R; psbM. Thick haze | 226 | | 848 | I. 271 | 11 8 34'9 | 31 4 52 | vB; mE; pos 305°.0, a nucl and F branches | 323 | | 849 | II. 521 | 11 8 42'9 | 84 31 3 | pB; R; psbM; 30" | 143 | | | | | 43'6 | B; S; R; smbM; has a * 10m, 60° np, dist 3' | 141 | | 850 | II. 729 | 11 8 48'9 | 43 19 17 | F; pL; glbM; r | 139 | | 851 | III. 333| 11 9 3'6 | 65 39 58 | pF; smbM; stellar | 407 | | 852 | II. 885?| 11 9 24'0 | 31 20 22 | pB; R; psmbM; 45". The PD differs 7' from that assigned by my Father; query therefore if the same object. | 323 | | 853 | II. 879 | 11 9 40'4 | 21 49 43 | pF; S; R; gbm; 15" | 412 | | 854 | M. 65 | 11 10 1'0 | 75 59 16 | B; R; gbm. Cloudy, but place well taken. (See fig 53.) | 241 | | | | | 2'4 | F; L; E with a R nucleus; gbm; 4'1 | 243 | | | | | 4'1 | a L, res centre with 2 F branches, E in a pos 45° np to sf | 242 | | | | | | Place very rude. R; gbm; 20...30". (It must have been very ill seen.) | 3 | | 855 | Nova. | 11 10 7'2 | 81 33 4 | eF | 117 | | 856 | II. 52 | 11 11 8'2 | 70 43 6 | B; R; smbM; 20" | 334 | | 857 | M. 66 | 11 11 16'9 | 76 5 47 | vB; vL; smbM; 3'1, 2'br; E 60° np to sf in direction of 2 st 10m, p. | 22 | | | | | | pB; gbm; E towards 2 stars np | 2 | | | | | | F; gbm; E; has 2 stars np | 3 | | 858 | I. 226 | 11 11 18'6 | 35 54 17 | pB; L; R; smbM; 2' diam | 324 | | 859 | V. 8 | 11 11 22'4 | 75 27 42 | A v long narrow ray vgbm; 15' long, a most curious object. E by diag in pos 105°.0. (See fig 51.) | 24 | | | | | 22'4 | pB; vLong; pos 100°.5; 6'1, 1'br; vgbm | 340 | | | | | 24'0 | F; vL; vme; vglbM; 8'1, 2'br; pos 103°.3 | 338 | | | | | 24'1 | pF; L; vme, pos = 101°.0; vgbm; a ray | 242 | | 860 | II. 338 | 11 11 25'0 | 62 5 52 | F; pL | 68 | | | | | 26'2 | F; L; R; vgbm; 2' diam | 343 | | | | | 26'5 | F; L; bM; 2' or 2' diam | 66 | | | | | 26'6 | vF; R; vgbm; has * 14 msf dist 60" | 416 | | | | | 27'0 | not vB; vL; irreg R; vglbM | 115 | | | | | 28'4 | vF; L; R; vglbM | 415 | | | | | 29'6 | F; pL; R; has a small * sf | 57 | | 861 | II. 32 | 11 11 32'3 | 86 6 30 | B; R; smbM to nucl; 25" | 141 | | | | | 32'6 | pB; R; bM almost to nucl | 238 | | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 862 | II. 550 | 11 11 50'8 | 99 20" 42 | F; v S; R; 10" | 136 | | | | | 51'1 | p B; R; stellar; n p a * 7 m | 129 | | 863 | II. 551 | 11 12 5'1 | 99 19 29 | p B; R; n f a * 7 m | 129 | | | | | 5'3 | F; v S; R; p s b M; 10" | 136 | | 864 | II. 33 | 11 12 21'2 | 85 50 3 | B; R; p s b M; 30" | 143 | | | | | | B; R; p g b M; viewed past merid | 238 | | 865 | I. 245 | 11 12 22'8 | 29 59 58 | B; R; g b M; r; 45" | 406 | | | | | 24'6 | v F; R; g b M; 30" | 404 | | | | | 24'7 | p B; R; g b M; 40"; windy | 344 | | | | | 26'0 | v F; R; g b M; haze thick | 226 | | 866 | III. 15 | 11 12 45'2 | 68 54 30 | F; L; E; 2' long. The s p of two | 59 | | | | | 46'4 | p F; v L; R; g b M; 60"; the p of 2 | 334 | | 867 | II. 32 | 11 12 48± | 86 7 ± | p B; S; E; b M | 143 | | 868 | Nova. | 11 13 13'0 | 49 12 46 | p B; p m E; S; has a suspicious nucleus, as if a v F close D * | 335 | | 869 | III. 16 | 11 13 16'4 | 68 52 1 | v F; p L; R; g b M; 30". R A estimated from that of III. 15. | 334 | | | | | 18'4 | v F; S; R; the n f of 2 | 59 | | 870 | III. 335| 11 13 25'7 | 64 46 13 | F; R; g b M; the n p of 2 | 58 | | 871 | II. 775 | 11 13 28'4 | 51 17 59 | F; p L; wires visible in twilight | 73 | | 872 | III. 336| 11 13 30'4 | 64 47 58 | v F; the s f of 2 | 58 | | 873 | I. 5 | 11 13 57'6 | 72 28 1 | p B; l E; g b M; 18" | 421 | | | | | 59'5 | B; R; p s m b M; 35" | 419 | | | | | 59'8 | B; R; p s b M; 25"…30" | 418 | | 874 | II. 782 | 11 13 58'0 | 35 13 32 | p B; R; v g l b M; 20"; a * 12 m p | 324 | | 875 | Nova. | 11 14 11'5 | 76 5 3 | v L; 6' l, 4' br; first v g, then v s v m b M | 338 | | | | | | Viewed; v B; v L; v s b M. (See fig 54.) | 340 | | 876 | III. 768| 11 14 16'3 | 36 8 53 | Not v F; v S; R. Approaching to stellar | 328 | | 877 | IV. 59 | 11 14 45'1 | 50 32 11 | F; R; about a stellar point 17 m | 335 | | | | | | Viewed. Nothing remarkable in its character to place it in the 4th class. | 73 | | 878 | II. 53 | 11 14 47'5 | 71 15 37 | v F; R | 63 | | 879 | IV. 4 | 11 15 7'8 | 90 10 2 | A star 13.14 m with a F, S, nebulous brush. | 144 | | 880 | II. 845 | 11 15 26'9 | 25 37 11 | F; R; g b M; 15". A * 9 m is 16° p, 3' n | 411 | | 881 | I. 219 | 11 15 30'9 | 50 18 22 | p B; R; p s b M; 45" | 401 | | | | | 33'3 | v B; R; p g m b M; 50"; r. AR 16m 33°3 by obs, but the minute must have been mistaken as my father makes it 15, with which Sw 401 agrees. | 335 | | 882 | I. 20 | 11 15 37'0 | 77 44 8 | F; p L; p m E nearly in parallel. It precedes the * 1341 A. S. C. 34°0. Pos with * 234°8. | 338 | | | | | 37'4 | F; 2nd class; E in parallel | 243 | | | | | 38'4 | e F; 2nd or 3rd class. The B * 1341 A. S. C. follows it. This neb must have changed greatly if it ever belonged really to the 1st class. | 242 | | 883 | II. 829 | 11 15 40'5 | 31 21 2 | v F; m E; v l b M; 60" | 323 | | No. | Synonym | AR 1830-0. | N.P.D. 1830-0. | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 884 | III. 337 | 11 15 49·7 | 65 6 43 | e F; v S; R | 407 | | 885 | III. 922 | 11 16 9·1 | 28 35 18 | This must be my father's neb, but it is a suspicious object, and I doubt whether it be not a little knot of 3 or 4 stars. | 406 | | 886 | I. 131 | 11 16 27·3 | 98 52 ± | p B; p L; E in merid. | 136 | | | | | 51 55 | F; L; E in direction of merid. | 129 | | 887 | I. 194 | 11 16 46·8 | 45 28 33 | Seen through thick cloud | 249 | | | | 48·0 | 28 47 | v B; L; m E; v s m b M; 2' l, 40" br. Many stars 14 & 15 m precede. | 248 | | 888 | Nova. | 11 16 53·7 | 42 4 57 | S; R; v s b M to a * 16 m | 139 | | | | 55·7 | 4 12 | e F; v s b M to * 16 m; 2 st 11 m, n f, point to it at twice their distance. | 330 | | 889 | Nova. | 11 17 11·7 | 61 11 52 | v F; R; p s b M; 25". Is 2' s p a * 12 m. | 343 | | 890 | I. 262 | 11 17 30·8 | 22 28 41 | p B; R; v s m b M almost to a *; 30". | 412 | | 891 | II. 159 | 11 17 34·6 | 72 12 20 | v B; R; p s b M; 40"; has st foll. | 419 | | | | 34·7 | 12 21 | p F; R; g b M; 20...25" | 421 | | | | 35·3 | 12 19 | v B; R; p s b M; 50...60" | 418 | | 892 | I. 246 | 11 17 49·9 | 32 11 5 | E; haze so that I can barely be certain that a nebula exists | 226 | | 893 | Nova. | 11 18 16·0 | 72 1 46 | p F; R; g b M; 25" | 421 | | | | 20·5 | 3 41 | c B; L; E; v g b M; 100" diam | 334 | | | | | 1 54 | p F; R; g b M; 45"; AR observed 3°·6, but was taken past merid by comparison with a distant star, by a process liable to great errors. | 418 | | 894 | II. 160 | 11 18 49·2 | 71 51 7 | B; L; R; b M; has a L * n and a smaller one s | 63 | | | III. 28 | 49·8 | 50 36 | B; v L; E; v g b M; 2' diam. Near a * | 334 | | | | | 50 0 | p B; p L. (N.B. II. 160 and III. 28 are probably identical.) | 61 | | 895 | II. 770 | 11 18 53·7 | 59 32 51 | F; R; 30" | 64 | | | | 55·3 | 33 11 | B; L; R; r | 66 | | | | 56·8 | 32 27 | p B; R; 40...50" | 68 | | | | 57·4 | 33 4 | Not v F; R; g b M; 25" | 341 | | | | 57·8 | 33 21 | p B; R; s b M; 30...40" | 65 | | 896 | I. 147 | 11 19 1·6 | 30 31 52 | B; R; p g b M. Query whether there be not a * excentric towards the s f side. (N.B. The obs makes P D = 31°, &c., but this must be a mistake. See next obs and my Father's place.) | 323 | | | | | 29 55 | F; S; R; b M; has a * near, s | 226 | | 897 | II. 339 | 11 19 10·2 | 63 24 43 | B; p L; g b M; 1 E | 58 | | 898 | II. 54 | 11 19 14·8 | 72 8 39 | No description | 418 | | | | 15·7 | 8 55 | F; E; 40"; has a * 10 m 5' s p | 419 | | 899 | Nova. | 11 19 45·9 | 53 38 47 | Not v F; R; s b M almost to a *; 20" | 331 | | 900 | Nova. | 11 19 55·3 | 68 15 58 | e F; v S; E in parallel | 59 | | 901 | II. 349 | 11 20 30·2 | 64 57 58 | p B; 1 E | 407 | | 902 | II. 13 | 11 21 20·4 | 79 47 10 | F; p L; v s b M; haze troublesome | 123 | | 903 | Nova. | 11 21 27± | 79 42 25 | p B; S; E in parallel; 40" l. Taken for II. 13, and the AR set down from the working list, being missed. But it appears to be a different nebula. | 120 | MDCCXXXIII. 3 G | No. | Synonym | R 1830°. | N.P.D. 1830°. | Description and Remarks | Sweep | |-----|---------|----------|---------------|-------------------------|-------| | 904 | II. 350 | 11 22 8·9 | 66 17 45 | F; has a * 7.8 m n f dist 5' | 244 | | 905 | Nova. | 11 22 39·6 | 60 34 11 | v F; R; s m b M | 64 | | | | | 36 ± | F; v S; R; b M. Rough P D, being past meridian | 68 | | 906 | II. 367 | 11 22 41·0 | 60 54 13 | No description | 68 | | | | | 41·7 | F; R; s b M. No companion seen | 66 | | | | | 42·2 | S; R; s b M, almost to a nucleus | 57 | | 907 | III. 353| 11 22 52·2 | 60 42 27 | F; S; R; 12''; no other near on the same parallel | 343 | | | | | 53·6 | Not v F; R; p s b M; 15'' | 416 | | | | | 53·7 | Not v F; S; R; p s b M; 20'' | 417 | | | | | ... | Rough PD, being much past merid | 115 | | 908 | I. 221 | 11 23 5·5 | 35 59 58 | F; v L; R; v g l b M; 2' diam; near a double star | 328 | | | | | 6·7 | p B; v L; 1E; v g b M; 5' diam; has a coarse double * s p | 324 | | 909 | II. 836 | 11 23 59·3 | 27 10 51 | Not v F; R; g b M; 40'' | 406 | | | | | 60·4 | e F, but sky not perfectly clear. The obs makes the R 23m 0·4, but it is clear from the former obs and my father's, which agree, that it should be 24m 0·4. | 344 | | 910 | II. 730 | 11 24 5·6 | 42 1 36 | p B; v L; E in merid; v g b M; 4' l, 2' br; has a * at its northern extremity. | 329 | | | | | 6·4 | p B; v L; 1E; at first v g and then v s b M to a * 15 m. 2' l, 90'' br; a * 11 m to n. | 330 | | 911 | I. 222 | 11 24 22·3 | 35 55 52 | Not B; L; 1E; a * 12 m s p very near the edge | 324 | | 912 | II. 351 | 11 24 27·2 | 64 37 3 | F; S; R; b M | 58 | | 913 | II. 552 | 11 25 36·1 | 98 54 4 | S; R; p s b M; 15''; has a * 14 m, 45° s p | 129 | | | | | 37·3 | F; R; b M; has a * 14 m s p | 136 | | 914 | I. 287 | 11 25 56·3 | 18 31 37 | F; m E, in pos 130°·4; b M; 90'' l, 12'' br | 377 | | 915 | III. 847| 11 26 42·2 | 29 5 18 | v F; R; v g b M; 20'' | 406 | | 916 | Nova. | 11 26 56·0 | 43 46 27 | v F; R; v g b M; 20'' | 139 | | 917 | III. 905| 11 27 9·7 | 13 47 1 | e F | 414 | | 918 | II. 784 | 11 27 24·9 | 34 45 47 | F; L; 1E; 4' diam; brighter and larger than I. 222 | 324 | | 919 | III. 843| 11 27 27·7 | 30 39 22 | v F; R; 15''. Has a v S * s f rather more than a diameter from edge (by diagram). | 323 | | 920 | Nova. | 11 27 28·6 | 52 39 7 | e F; p m E; p L; g b M | 331 | | 921 | II. 837 | 11 27 47·7 | 27 19 5 | e F; R; g b M; sky not quite clear | 344 | | 922 | Nova. | 11 28 7·4 | 64 57 30 | v F; R; 30'' | 407 | | 923 | III. 29 | 11 28 21·0 | 71 13 52 | Stellar; a burred star | 63 | | 924 | Nova. | 11 28 22·0 | 72 10 41 | v F; S; b M | 334 | | 925 | II. 731 | 11 28 30·9 | 41 9 16 | B; S; m E; p g b M; 30'' l | 329 | | | | | 33·2 | p B; m E; g b M; 60'' l, 30'' br | 330 | | 926 | II. 338 | 11 28 31·6 | 29 27 3 | B; R; g b M; r; 30'' | 406 | | | | | 32·7 | e F, but a sure obs. Sky growing dull. Mirror tarnished | 404 | | 927 | II. 352 | 11 28 52·5 | 66 22 45 | e F; E | 244 | | | | | 54·7 | v F; S | 59 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 928 | III. 81 | 11 29 25·1 | 76° 56′ 39″ | F; S; R; bM ........................................... | 242 | | | | 28°0′ | 56° 55′ | pF; R; p s b M. The only object in the sweep. The place reduced by the obs of the preceding and following sweep, ∴ precarious. | 339 | | 929 | I. 227 | 11 30 0·8 | 32 47 37 | F; L; R; v g b M; 60″. (Twilight.) .................. | 345 | | | | 3·6 | 47 22 | eF; L; v g l b M; 90″................................. | 323 | | 930 | II. 732 | 11 30 24·7 | 42 35 37 | A * 15 m with a nebulous tail n f which touches another star. | 139 | | 931 | Nova. | 11 30 42·9 | 57 9 12 | pB; p m E; p g b M; 50″ l, 30″ br. The first of 2 .... | 342 | | | | 43·3 | 8 41 | The s p of 2; less B and smaller than the n f ........ | 74 | | | | 44·6 | 8 35 | B; p L; E; g b M; 40 or 50″ 1 ....................... | 337 | | 932 | Nova. | 11 30 45·9 | 57 7 22 | pB; m E; p g b M; 90″ l, 40″ br; the second of 2 .... | 342 | | | | 46·3 | 7 31 | pB; E in merid; g b M; 40 ... 50″ l; the n f of two. | 74 | | | | 47·6 | 7 15 | B; p L; p m E; 50 ... 60″ l; 40″ br .................. | 337 | | 933 | III. 109| 11 30 55·2 | 71 22 1 | The first of 3 ........................................ | 61 | | | | 56·2 | 20 16 | F; v S; p m E; s b M; the first of 3 ................ | 334 | | 934 | Nova. | 11 30 59·6 | 73 43 45 | F; R; the preceding of 2; has 3 st s ................ | 419 | | | | 80·8 | 43 54 | F; R; forms an appendage to II. 103, which it precedes. One or other of these right ascensions has some mistake, which pervades the observations of both nebulæ. (See below.) | 418 | | 935 | III. 609| 11 31 3·8 | 98 25 17 | vF; R; g b M; 20″; has a * 8 m 6′ s, on same merid .... | 136 | | 936 | II. 103 | 11 31 4·1 | 73 42 55 | F; m E; g b M; the f of 2. This and the next AR are probably affected by the mistake above noticed. | 419 | | | | 8·8 | 42 26 | pF; p L; 1E; g b M; near a B st ..................... | 421 | | | | 23·5 | 42 49 | F; En f to s p; has another F neb attached to its preceding extremity. (See fig 79.) | 24 | | | | 24·8 | 42 39 | pB; E; p g b M; has another s p...................... | 418 | | | | 24·9 | 42 29 | pB or not v F; 1E; g l b M.......................... | 422 | | 937 | II. 839 | 11 31 4·7 | 28 46 16 | vF; p s b M; by obs AR = 30m 4s·7; but this is proved to be erroneous by the coincidence of Sw 406 with my father's AR. | 344 | | | | 10·3 | 46 18 | pB; R; 35″; pg b M .................................. | 406 | | 938 | II. 340 | 11 31 20·2| 64 21 38 | pB; S; R; r; 20″ .................................... | 58 | | 939 | II. 161 | 11 31 25·4| 71 20 17 | pB .................................................. | 63 | | | | 27·2 | 19 18 | The second of 3 ...................................... | 61 | | | | 27·6 | 19 51 | pB; p L; g b M; the second of 3 ..................... | 334 | | 940 | III. 30 | 11 31 30·1| 71 17 26 | The last of 3 ....................................... | 61 | | | | 31·6 | 17 51 | The last of 3 ....................................... | 334 | | | | 32·3 | 20 38 | An obs snatched between clouds and probably a mistaken bisection in PD. | 62 | | 941 | III. 375| 11 31 52·2| 68 43 12 | Not v F; S; R; b M .................................. | 59 | | 942 | II. 737 | 11 32 7·5 | 41 21 6 | F; R; b M; 15″ ....................................... | 329 | | | | 9·6 | 20 32 | F; E; g b M; 20″..................................... | 330 | | No. | Synonym | R 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|---------|-------------|------------------------|-------| | 943 | I. 21 | h m s | 77 35 9 | No description | 242 | | | | 11 32 12'4 | | | | | | | 12'5 | 35 5 | No description | 340 | | | | 12'9 | 35 24 | p B; L; 1E; v g b M; 3' diam | 338 | | | | ... | 35 12 | F; R; g b M; 30...40''; the R of this sweep and both the R and P D of the next obs too roughly determined to be set down. | 3 | | | | ... | | v F; R; v g b M; a * 9 m 15' dist in parallel | 2 | | 944 | III. 320| 11 32 14'0 | 64 14 13 | F; R; has a * 6.7 m s f, dist 3'. | 407 | | 945 | I. 94 | 11 32 17'1 | 52 29 46 | p B; p L; 90'' 1, 60'' br; E in parallel; hazy | 72 | | | | 18'1 | 31 2 | B; p L; 1E; 40'' 1, 30'' br; v g l b M | 331 | | | | 18'5 | 30 31 | v B; L; m E nearly in parallel; 3' long; m b M; a * f | 70 | | 946 | III. 329| 11 32 46'0 | 64 15 33 | Not v F; p L; 30'' | 407 | | 947 | Nova. | 11 33 7'4 | 78 45 45 | F. The first of 4 | 120 | | 948 | III. 284| 11 33 15'9 | 95 13 16 | B; R; p s b M; 30''. At least 2nd class | 147 | | 949 | III. 376| 11 33 18'3 | 68 43 47 | v F; S; R; p s b M; a * 11 m prec 10°-O | 246 | | | | 19'2 | 45 10 | Not v F; S; R; g b M | 59 | | 950 | Nova. | 11 33 18'9 | 78 44 45 | v F; the second of 4; place estimated from the others | 120 | | 951 | II. 153 | 11 33 25'4 | 78 47 15 | p B; the third of 4 | 120 | | 952 | III. 774| 11 33 32'5 | 36 16 53 | v F; p m E | 328 | | 953 | II. 154 | 11 33 38'4 | 78 48 5 | p B; the last of 4 | 120 | | 954 | II. 341 | 11 33 39'7 | 62 34 17 | No description | 343 | | | | 39'9 | 33 35 | p B; R; p s b M; 15''. Good obs | 417 | | | | 40'8 | 34 17 | No description | 115 | | 955 | III. 775| 11 34 13'7 | 36 19 53 | e F | 328 | | 956 | Nova. | 11 34 22'3 | 62 33 34 | Cloudy; hardly discernible | 416 | | 957 | Nova. | 11 34 40'3 | 101 55 24 | F; v S; R; b M. Well observed | 129 | | 958 | Nova. | 11 34 44'0 | 28 57 0 | p F; 1E; g b M; precedes * 8 m, 5' dist | 344 | | | | 46'3 | 56 38 | p B; p m E; p g b M; has a D * 8 m, n f | 406 | | 959 | II. 831 | 11 34 49'5 | 31 5 50 | v F; p m E; p s b M to nucl = * 12 m. Twilight | 345 | | | | 51'7 | 6 57 | B; S; a nucleus with an extended burr; 15'' long. PD by Sw 32°, corrected to 31, which is the true degree. | 323 | | 960 | Nova. | 11 34 56'4 | 69 5 47 | F; R | 63 | | | | 61'6 | 6 1 | v F; S; the first of 4 | 334 | | 961 | Nova. | 11 35 3'4 | 69 10 27 | F; R | 63 | | | | 7'6 | 10 0 | v F; p S | 334 | | 962 | III. 377| 11 35 8'1 | 69 6 41 | p B; v g b M; the third of 4 | 334 | | | | 10'4 | 8 7 | p B; R; the last of 3 | 63 | | | | 13'2 | 6 57 | v F; R; the s p of two | 59 | | 963 | Nova. | 11 35 13'1 | 69 4 11 | v F; p S; the last of 4. There are however 3 or 4 more nebulae in this neighbourhood. | 334 | | 964 | Nova. | 11 35 15'4 | 33 24 42 | F; p L; R; v g b M | 324 | | 965 | Nova. | 11 35 18'8 | 55 32 20 | Not v F; S; R; p s b M | 337 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 966 | III. 378 | 11h 35m 32.7s | 69° 5′ 35″ | vF; R; the n f of 2 ........................................... | 59 | | 967 | Nova. | 11h 36m ± | 55° 57′ ± | eF; R; g b M. The preceding of 3 forming an equilateral triangle. Place very rough. | 337 | | 968 | Nova. | 11h 36m ± | 55° 54′ 0″ | eF; R; g b M. The second of 3 .................................. | 337 | | 969 | Nova. | 11h 36m ± | 55° 57′ ± | eF; R; g b M. The last of 3 .................................... | 337 | | 970 | Nova. | 11h 36m 12.2s | 69° 4′ 21″ | F; S; R; b M. Doubtful .......................................... | 61 | | 971 | Nova. | 11h 36m 54.8s | 78° 14′ 2″ | F; S; s b M; irreg fig; r ....................................... | 19 | | | | 59° 9′ | 13° 52′ | F; R; p s b M .................................................................. | 22 | | 972 | III. 833 | 11h 36m 55.0s | 38° 51′ 13″ | vF; a doubtful object. Query if not a D * 6″ dist involved in a nebula. | 328 | | | | 57° 6′ | 51° 31′ | F; S; R; p s b M ................................................................ | 329 | | | | 60° 9′ | 51° 17′ | Foggy .............................................................................. | 330 | | 973 | II. 104 | 11h 37m 1.1s | 75° 17′ 0″ | B; S; R; p s b M; 10″ ................................................ | 419 | | | | 2° 9′ | 17° 49′ | B; R; v s m b M, to a * 11 m; 40″ .................................. | 242 | | | | 3° 4′ | 17° 51′ | pB; S; R; s m b M; 15″; compact .................................... | 338 | | 974 | Nova. | 11h 37m 21.9s | 55° 51′ 21″ | vF; R; the first in an unequally divided line of 3. More suspected. | 74 | | 975 | Nova. | 11h 37m 26.9s | 55° 53′ 21″ | vF; R; b M; the second of an unequally divided line of 3 .. | 74 | | 976 | Nova. | 11h 37m 40.4s | 55° 57′ 6″ | vF; R; the third of an unequally divided line of 3 ............. | 74 | | 977 | Nova. | 11h 37m 57.4s | 68° 39′ 40″ | pF; n f a * 7 m; Δ AR = 4°.5; dist 5″ ............................ | 409 | | | | 60° ± | 40° 49′ | vF; R; g b M. (Taken past merid. AR estimated. PD too great.) | 59 | | 978 | II. 785 | 11h 38m 27.0s | 33° 5′ 17″ | pB; E; g b M .................................................................. | 323 | | | | 31° 5′ | 5° 32′ | pB; lE; p g b M. Twilight ........................................... | 345 | | 979 | I. 120 | 11h 38m 27.1s | 105° 54′ 55″ | F; L; has * 11 m 5° n f. Twilight .................................. | 149 | | 980 | II. 723 | 11h 39m 11.1s | 58° 41′ 51″ | B; R; s b M; 20…30″ .................................................. | 65 | | | | 11° 5′ | 41° 19′ | eF. Seen through cloud ............................................... | 341 | | | | 11° 5′ | 41° 24′ | not vF; R; g b M; 40″ ................................................ | 342 | | 981 | II. 553 | 11h 39m 22.0s | 100° 0′ 35″ | L; R; g b M; 60″; r .................................................. | 129 | | 982 | II. 738 | 11h 39m 37.1s | 40° 20′ 26″ | B; pL; R; g b and p s m b M; 60′ .................................. | 329 | | 983 | I. 248 | 11h 39m 40.7s | 29° 38′ 36″ | B; pL; R; p g m b M; the prec of 2 ................................ | 406 | | | | 41° 6′ | 38° 50′ | F; R; g b M; 20″ ...................................................... | 344 | | 984 | II. 832 | 11h 39m 52.3s | 29° 37′ 51″ | F; pL; E; g b M. The foll of 2 .................................... | 406 | | 985 | I. 228 | 11h 40m 5.1s | 32° 59′ 5″ | B; R; s m b M; 30″; hazy ........................................... | 346 | | | | 6° 1′ | 57° 45′ | B; pL; R. Seen through thick haze .................................. | 226 | | | | 11° 2′ | 58° 22′ | pB; E; g b M; like II. 785, but brighter .......................... | 323 | | | | 13° 1′ | 58° 32′ | B; pL; R; p s m b M; 60″ ........................................... | 345 | | 986 | II. 408 | 11h 40m 6.6s | 54° 1′ 47″ | pF; R ............................................................................. | 331 | | | | 6° 9′ | 0° 48′ | F; S; R; near a small * .............................................. | 72 | | | | 8° 0′ | 2° 11′ | F; S; R; b M .................................................................. | 70 | | 987 | Nova. | 11h 40m 17.8s | 62° 36′ 31″ | pB; R; s m b M ................................................................ | 64 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 988 | I. 82 | h m s | 62° 2′ 1″ | B; L; R; p g b M; fading away to nothing; 40″ diam | 65 | | | | | 19° 2′ | R; b M to nucleus; ζ and haze | 67 | | | | | 19° 4′ | p F; s b M; ζζ | 415 | | | | | 19° 9′ | B; p L; R; s b M to nucleus; 40″ | 57 | | | | | 20° 3′ | B; R; s b M; 40″ | 66 | | | | | 2° 39± | a L and B neb. Imperfect obs past mer | 68 | | 989 | III. 321| 11 40 26′7| 62 56 28 | F; p L; E; v l b M | 58 | | | | | 28° 4′ | p F; l E; v g b M; 25″ | 417 | | 990 | Nova. | 11 40 47′8| 90 9 7 | e F; S; p s b M | 146 | | 991 | III. 341| 11 41 15± | 64 7 48 | v F; p L; AR by working list; past mer | 407 | | 992 | II. 342 | 11 41 15′1| 62 33 50 | p B; R; p s b M; 30″ | 417 | | | | | 15° 2′ | p B; p L; R; g b M; 60″ | 343 | | | | | 15° 9′ | v F; R; p s b M; ζ | 415 | | 993 | II. 787 | 11 41 44′1| 33 54 32 | e F; R; g b M | 324 | | 994 | II. 824 | 11 41 44′7| 37 13 43 | F; v m E; v g b M; 150″ 1, 30″ br | 328 | | 995 | III. 90 | 11 41 45′2| 82 29 7 | F; R; 15″; has * 13 m, 70″ dist, n p | 253 | | | | | 50° 9′ | F; R; near a * 13 m. Wind outrageous | 251 | | | | | 29 ± | F; R; b M; 1′ s of a * 9.10 m | 117 | | 996 | Nova. | 11 42 0± | 64 7 48 | No desc. Follows III. 341 on same parallel | 407 | | 997 | II. 788 | 11 42 1·0 | 33 58 32 | p B; R; p s b M | 324 | | 998 | III. 379| 11 42 38′0| 67 2 20 | e F; R; S; near a star | 244 | | 999 | II. 740 | 11 42 49′6| 40 21 56 | not v F; S; R; p s p m b M | 329 | | 1000| III. 616| 11 42 53′0| 51 3 24 | e F; g l b M; a * 7 m foll nearly in the parallel | 335 | | | | | 58° 1′ | e F; precedes a * 7 m in the same parallel, dist about 3′. Place uncertain. | 331 | | 1001| Nova. | 11 43 33′1| 56 39 1 | p B; R; p s b M | 74 | | | | | 35° 6′ | p B; S; p m E; p s b M | 337 | | | | | 36° 8′ | F; R; p s b M; 20″ | 131 | | 1002| I. 203 | 11 43 54′4| 44 56 2 | A superb nebula; B; v L; R; 3′ diam; v g b M; r; is probably a globular cluster. | 248 | | | | | 57° 7′ | p B; v L; R; v s b M to a v S star, and very dilute at the borders; 4′ diam. | 139 | | 1003| III. 389| 11 43 55′8| 68 25 6 | v F; S; R | 423 | | 1004| Nova. | 11 44 1·2 | 68 4 0 | e F; R | 59 | | 1005| I. 173 | 11 44 3′5 | 52 3 19 | v B; p L; R; p s m b M | 73 | | | | | 3° 9′ | v B; R; s b M, fading to nothing; 90″ | 72 | | | | | 5° 5′ | v B; R; s m b M, almost to a * 9 m; 60″ | 70 | | 1006| I. 251 | 11 44 11′8| 28 23 3 | not v B; R; p g b M; r | 406 | | | | | 16° 5′ | B; R; p s b M; 60″; a star precedes, Δ AR = 8° 0, pos from neb = 215° 9. | 344 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1007 | III. 322 | h m s | 62° 50' 49" | Not vF; R; sbM; 35" | 343 | | | | | | pB; R; bM | 115 | | | | | | B; R; psbM; 35" | 417 | | 1008 | II. 403 | 11 44 34.9 | 68 18 0 | F; mE; bM; a coarse D * precedes | 409 | | | | | | Seen in its place as per working list | 244 | | 1009 | I. 202 | 11 44 46.9 | 41 12 46 | B; mE; vg bM | 329 | | | | | | pL; R; gbM; barely visible for fog | 330 | | 1010 | III. 342| 11 44 49.2 | 65 39 28 | vF; S; R | 407 | | 1011 | V. 45 | 11 44 52.3 | 36 43 3 | B; L; vsbM; r; 3' diam. Fine object | 328 | | 1012 | III. 612| 11 44 55.2 | 93 3 9 | pF; R; bM | 21 | | | | | | F; lE; nearly in parallel r::: Sky perfectly clear | 147 | | | | | | vF; lE. Sky not quite clear; PD rough, being taken beyond meridian | 146 | | 1013 | Nova. | 11 44 57.0 | 68 10 44 | eF; R | 59 | | 1014 | II. 833 | 11 45 23.6 | 30 41 7 | pF; lE; gbM; 40" 1 | 345 | | | | | | pF; E; vg bM; 60" 1 | 323 | | 1015 | IV. 67 | 11 45 50.2 | 30 34 7 | F; vL; R; pglbM | 323 | | | | | | F; L; R ill defined nebulous mass; obs difficult, owing to haze | 226 | | 1016 | Nova. | 11 46 5.2 | 60 47 41 | vF; E45 sp from a * 10m dist 40" | 66 | | | | | | A * 10m with eF neb 45° sp; 30". The neb by a diag made at the time is oval, and forms a kind of appendage to the star | 65 | | 1017 | IV. 62 | 11 46 31.5 | 33 56 0 | F; R; near a * | 417 | | 1018 | II. 162 | 11 46 42.9 | 77 5 14 | B; pL; R; nearly uniform, but hazy; diam 25" | 324 | | | | | | pB; R; vg bM; a * 10m 25° nf, dist 4'..5' | 242 | | | | | | pB; L; psmbM; 3' diam | 338 | | 1019 | II. 724 | 11 46 46.7 | 59 3 39 | pB; R; bM. An exact obs. | 67 | | 1020 | Nova. | 11 46 47.1 | 101 5 54 | F; S; R; psbM; 15". The p of 2 | 129 | | 1021 | Nova. | 11 47 0.6 | 101 2 44 | vF; S; R; bM; 15". The f of 2 | 129 | | 1022 | II. 132 | 11 47 12.6 | 82 18 19 | B; E 30° nf to sp; vsmbM to nearly a star. The arms very faint | 117 | | | | | | B; E; psbM; 25" l, 15" br | 251 | | | | | | vB; mE; vsmbM; 30" l; nucleus equals a star 10 m | 250 | | 1023 | II. 840 | 11 47 18.6 | 28 32 8 | Not vF; lE; has * 8m following in the parallel | 406 | | | | | | vF; a * 9mf, dist 6'; another precedes 10' dist to the s | 344 | | 1024 | III. 343| 11 47 37.2 | 65 10 54 | F; S; R; psbM | 407 | | 1025 | III. 707| 11 47 49.6 | 40 42 56 | No description | 329 | | 1026 | Nova. | 11 47 50.2 | 60 3 25 | eF; R; bM; 25". Supposed at the time to be II. 724, but on reducing the obs it differs 1m in RA and 1° in P D, both which can hardly be mistakes | 342 | | 1027 | Nova. | 11 47 56.5 | 57 1 32 | F; S; E; near a * | 131 | | | | | | E nearly in parallel; a * 11m near | 74 | | | | | | pB; mE; psbM; 30" l; near a * | 337 | | No. | Synonym | RA 1830°-0 | N.P.D. 1830°-0 | Description and Remarks | Sweep | |-----|---------|------------|---------------|------------------------|-------| | 1028 | Nova. | h m s | 61 0 42 | vF; R; g b M. The first of 2 .................................. | 343 | | | | | | vF; S; R; s b M like a *. The p of 2 with several stars between them. | 417 | | 1029 | II. 791 | 11 48 39'9 | 33 36 30 | vF; R; p s l b M; 35''; sky dull .................................. | 346 | | 1030 | IV. 61 | 11 48 41'3 | 35 40 33 | vB; vL; R; s m b M; 3' diam ...................................... | 328 | | 1031 | I. 229 | 11 48 59'9 | 33 36 20 | B; R; s m b M; 40''; sky dull .................................... | 346 | | 1032 | Nova. | 11 49 0'6 | 74 45 10 | vF; p L; R; has two st s f ....................................... | 419 | | | | 1'9 | 43 29 | No description, (probably a hurried obs) .......................... | 422 | | | | 2'2 | 45 46 | No description .................................................................. | 421 | | 1033 | III. 323| 11 49 3'2 | 63 47 33 | F; vS; E pos 25° n f to s p. Between two stars, 80'' dist. (By a diagram made at the time, the neb lies exactly in the line of the two stars which are situated at equal distances from the two extremities, and almost in contact with them. A singular object.) | 58 | | 1034 | III. 344| 11 49 12'8 | 65 50 38 | vF; R; the northern of 2 ........................................... | 407 | | 1035 | III. 345| 11 49 12'8 | 65 54 58 | vF; R; the southern of 2 ........................................... | 407 | | 1036 | Nova. | 11 49 19'4 | 61 10 42 | vF; R; near a * 12 m .................................................. | 417 | | | | 20'6 | 10 0 | pF; 1E; g b M; the f of 2 in parallel, with a star between .. | 343 | | 1037 | Nova. | 11 49 24'2 | 91 11 7 | F; S; R; b M; s p a * 11 m ......................................... | 146 | | 1038 | II. 368 | 11 49 29'7 | 60 51 26 | F; S; R; b M ............................................................. | 64 | | | | 29'7 | 52 1 | vB; p L; R; s m b M; 40''. Clouded suddenly, and obs left imperfect. | 63 | | | | 30'1 | 51 36 | pB; R; s b M .................................................................. | 66 | | | | 31'0 | 51 34 | pB; R; g b M; r ................................................................ | 68 | | 1039 | Nova. | 11 49 31'7 | .............. | vB; m E; m b M. Taken for II. 368, and no P D taken; but the description disagrees essentially, and it can hardly be the same. | 115 | | 1040 | Nova. | 11 49 40'8 | 41 49 9 | F; m E; v g l b M; 100'' 1, 25'' br ................................ | 255 | | 1041 | II. 733 | 11 49 42'3 | 45 6 17 | B; m E; v s v m b M to a * = 10.11 m; pos of extension = 62°-3 by measure. | 248 | | | | 49'0 | 8 ± | A * 11 m with a strong nebulous ray (25° n f to s p by estim from diagram); v s v m b M. | 140 | | 1042 | III. 3 | 11 49 51'5 | 72 52 48 | Not vF; R; p g b M; 35'' ........................................... | 421 | | | | 53'0 | 52 14 | pB; p s b M; 25'' .................................................... | 422 | | 1043 | III. 369| 11 50 7± | 61 34 52 | pB; L; g b M. AR by working list; past merid .................... | 68 | | | | ...........| 34 46 | vF; L; 60''; past merid ............................................ | 66 | | | | ...........| 36 ± | Seen; no descrip. P D very rough .................................. | 115 | | 1044 | Nova. | 11 50 10'3 | 74 50 45 | e F; has a * 9 m 5' sf .............................................. | 419 | | 1045 | II. 275 | 11 50 11'0 | 58 37 56 | Not vF; bicentral or elongated; v g b M, to a central axis pos = 199°-5, or pos of the two centres = 19°-5; 14'' l, 25'' br | 342 | | 1046 | III. 617| 11 50 24'6 | 51 14 38 | e F; p L; R .................................................................. | 73 | | 1047 | I. 223 | 11 50 33'1 | 38 5 43 | No description .................................................................. | 328 | | 1048 | I. 121 | 11 51 39'8 | 90 9 32 | B; R; 60''; a * 10 m, 50° n p .................................... | 146 | | | | 40'3 | 8 40 | B; R; p L; p s b M; r; 70''; has 3 or 4 large stars near .... | 145 | | No. | Synonym | AR 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1049 | II. 404 | h m s | 68° 59′ 27″ | B; pL; R; bM………………… | 63 | | | | | 46° 9 | B; pL; R; bM………………… | 61 | | | | | 48° 7 | eF; L; vlbM; a * 12m, nf | 246 | | | | | 49° 3 | pB; R; g bM; 40″ | 423 | | | | | 49° 4 | pB; pL; R; g bM…………… | 409 | | | | | 50° 0 | vF………………………….. | 244 | | 1050 | I. 253 | 11 52 38′6 | 27° 9 58 | pB; R; ps1bM; 25″………… | 344 | | 1051 | III. 77 | 11 52 39′6 | 75 39 9 | eF; R; a * 16m, nf (pos = 80°-0), dist 2′………… | 242 | | 1052 | IV. 28.1| 11 53 11′8 | 107 55 10 | eF; L; R; vgvlbM; 2′ diam; 21°-0 of time preceding a * 8m. | 338 | | 1053 | IV. 28.2| 11 53 11′8 | 107 57 10 | vL; R; vg bM; the chief neb of a fine double nebula. The other is 2′ s. They run together. | 149 | | 1054 | I. 252 | 11 53 25′0 | 26 55 26 | The northern of the double neb. It is the smaller and fainter of the two. | 149 | | | | | 25° 2 | pB; R; g bM; 35″; sky not quite clear …………… | 344 | | | | | | B; R; at first g, then ps vmbM to a nuclear mass which seems resolvable. | 411 | | 1055 | Nova. | 11 53 28′9 | 84 42 ± | S; R; precedes a double * about 30°, and is 3′ south of it. AR a rough estimate only from the double *. | 142 | | | | | 38° 7 | Not B; S; R; psbM; 15″………… | 143 | | 1056 | III. 491| 11 53 46′7 | 89 15 52 | F; vS; R; bM……………….. | 145 | | 1057 | II. 276 | 11 54 0′7 | 87 4 47 | F; R; sbM; 25″; a * sf………… | 141 | | 1058 | II. 741 | 11 54 3′6 | 40 25 6 | B; pL; R; pg bM; 40″………… | 329 | | 1059 | Nova. | 11 54 5′6 | 71 2 1 | vF; S………………………… | 61 | | | | | 7° 3 | vF; S; R; psbM; almost stellar……………… | 334 | | 1060 | III. 390| 11 54 9′4 | 70 18 42 | vF; S; lbM…………………. | 63 | | | | | 18 16 | vF; pL; R; g bM…………… | 334 | | | | | 18 1 | eF; S; too late for transit………………….. | 61 | | 1061 | IV. 56 | 11 54 24′5 | 44 31 9 | E; pos of axis 132°-0; a * 11.12 m, dist 2′, pos 257°-0…… | 256 | | | | | 24° 8 | pF; vL; E; at first vg l b, and then vs vmbM, to a * 14 m. A * is sp. | 255 | | | | | 25° 6 | pB; L; E; 3½′ 1, 2¾′ br; at first vg l b, but then suddenly comes up to a * in centre = 11 m. | 138 | | | | | 27° 5 | E; L; vsmbM to a * 11 or 12 m; has a * 10 m 20° sp … | 139 | | 1062 | Nova? | 11 54 59′8 | 68 ± | pB………………………….. | 423 | | 1063 | Nova? | 11 55 4′3 | 68 ± | pB………………………….. | 423 | | 1064 | Nova? | 11 55 8′3 | 68 ± | pB. On merid with two more………………….. | 423 | | 1065 | III. 394| 11 55 18′8 | 68 49 29 | eF; double neb, both S; R; pos 20° n f………… | 246 | | | | | 19° 1 | vF; a double neb by diag, pos 20° sp, nearly equal. They run together. | 244 | | | | | 19° 4 | vF. The first of 5……………… | 59 | | 1066 | I. 174 | 11 55 17′5 | 57 9 27 | B; vL; mE; pos = 97°; g bM; 6′ long………… | 342 | | | | | 19° 6 | pB; vL; E in parallel; 3 or 4′l, 90″ br………… | 74 | | | | | 20° 4 | F; vL; vg bM; mE in parallel; 4′l, 2′ br………… | 337 | | | | | 25° 5 | pB; vL; mE; 10° np to sf; vg bM; 3′l, 1′ br………… | 131 | MDCCCXXXIII. | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 1067 | III. 395 | 11 55 24·9 | 68 49 30 | p B; v F; R; the second of 5 | 409 | | | | 25·4 | 50 24 | v F; R; the second of 5 | 59 | | 1068 | III. 391 | 11 55 25·8 | 68 41 51 | No description | 423 | | | | 27·1 | 42 5 | Not very F. Another seen. | 424 | | | | 27·4 | 42 0 | p B | 409 | | | | 29·4 | 41 37 | The third of 5 | 59 | | 1069 | III. 37 | 11 55 27·6 | 78 12 11 | F; R; b M; 30" | 19 | | | | 27·9 | 11 26 | v F; L; p g b M; 2' | 338 | | | | 29·1 | 11 57 | F; R; v g b M; 15"; good obs. | 242 | | | | 29·1 | 11 50 | p B; R; b M; 40" | 120 | | | | 30·1 | 11 58 | F; R; b M | 22 | | 1070 | III. 392 | 11 55 29·4 | 68 43 37 | v F; R; the fourth of 5; has another on the same meridian, n. | 59 | | 1071 | Nova. | 11 55 29·4 | 68 38 30 | p B | 409 | | | | 30·1 | 39 55 | Not v F | 424 | | 1072 | II. 277 | 11 55 43·7 | 87 9 17 | Not v F; R; g b M | 145 | | | | 45·3 | 9 13 | F; R; b M; 15" | 143 | | | | 45·5 | 9 54 | p B; L; R; p s b M; 60" | 238 | | | | 45·6 | 9 15 | p F; irr R; p s b M; 40" | 141 | | 1073 | III. 394 | 11 55 48·5 | 68 44 0 | e F | 409 | | 1074 | Nova. | 11 55 48·7 | 86 59 7 | F; S; R | 145 | | 1075 | III. 396 | 11 55 52·4 | 68 53 30 | The last of 5 | 59 | | 1076 | III. 258 | 11 55 57·3 | 87 16 3 | F; R; b M; 20"; the sf of two | 143 | | 1077 | Nova. | 11 56 5·9 | 91 26 7 | Not v F; L; R; 40"; has a * 10 m, 60" n | 146 | | 1078 | III. 355 | 11 56 8·9 | 62 3 16 | e F | 66 | | | | 9·3 | 3 14 | F; R; g b M | 68 | | | | 10·0 | 2 51 | v F | 64 | | | | 10·6 | 4 22 | F; p L; R; b M | 115 | | 1079 | II. 382 | 11 57 13·1 | 68 28 1 | e F | 423 | | | | ... | 28 ± | No description | 409 | | 1080 | III. 400 | 11 57 19·6 | 52 10 38 | e F; v S; like a *; is n f a * 11 m, 2' dist | 72 | | | | 22·1 | 11 27 | v F; R; v s b M; has * 10 m, 45° sp, 90" dist | 331 | | 1081 | I. 207 | 11 57 19·7 | 41 34 33 | B; v L; m E, in pos 32°0; seen through much fog | 330 | | 1082 | III. 383 | 11 57 21·6 | 68 25 31 | No description | 423 | | | | 21·9 | 26 10 | v F; R; b M | 244 | | | | ... | 26 30 | No description | 409 | | 1083 | III. 326 | 11 57 26·9 | 63 29 28 | e F; R; v g b M | 407 | | | | 28·9 | 29 58 | v F; R | 58 | | 1084 | III. 717 | 11 57 27·6 | 39 28 46 | p B; v L; m E in pos 166·5; 3' l, 1' br; v g y l b M. This cannot be either I. 206 nor I. 207, as neither of these agrees in its angles of position. | 329 | | | | ... | 29 37 | Nearly as B and Las I. 207; and the position is from np to sf. Both therefore exist. Taken past merid. PD therefore precarious. | 330 | | No. | Synonym | AR 1830° | N.P.D. 1830° | Description and Remarks | Sweep. | |-----|---------|----------|-------------|------------------------|-------| | 1085 | I. 225 | 11 57 43·3 | 36 20 33 | B; R; p s b M; has a * 12 m 35'' s p very near the edge | 328 | | 1086 | II. 370 | 11 57 54·3 | 60 52 26 | pB; R; b M | 64 | | | | | 55·8 | 52 29 | pB; 60''; moon and haze | 67 | | | | | 56·3: | 51 31: | pB; R; s b M; 40''. Uncertain obs; between clouds | 65 | | | | | 56·8 | 52 56 | vF; 1E | 66 | | | | | 57·4 | 52 52 | B; R; g m b M; 30'' | 417 | | | | | 59·6 | 53 22 | pB; not v S; E; 1b M | 115 | | 1087 | Nova. | 11 58 7·9 | 21 53 41 | B; R; g b M; 20''; first class | 412 | | 1088 | I. 195 | 11 58 18·7 | 45 59 52 | vB; v m E, in pos 151°·0; v s v m b M; 40'' l, 10'' br | 248 | | | | | 23·0 | 58 57 | B; S; m E; s b M; a double * points to its nucleus | 150 | | 1089 | Nova. | 11 58 28·5 | 55 3 45 | e F | 337 | | 1090 | Nova. | 11 58 29·6 | 74 39 12 | A suspected neb. Extremely faint | 24 | | 1091 | III. 708 | 11 58 55± | 46 2 15± | In a straight line prolonged from I. 195 through a double star near it. | 248 | | 1092 | V. 4 | 11 59 25·4 | 86 10 36 | vF; not v L; E or bicentral; b M | 143 | | | | | 29·1 | 10 40 | F; v L; E; g b M; 3' l, 2' br; has * 16 m in nucl, and 1 or 2 more suspected. | 141 | | 1093 | Nova. | 11 59 27·3 | 56 3 6 | e F; v S; R; m b M | 74 | | 1094 | I. 33 | 11 59 29·1 | 78 40 18 | vB; m E; 30° n p to s f; b M | 120 | | | | | 29·2 | 41 15 | pB; p m E; 30° n p to s f; 2' l | 191 | | | | | | 40 12: | E in a n p direction towards a * | 3 | | 1095 | III. 68 | 11 59 56·2 | 72 55 10 | vF; S; R; ps l b M | 419 | | 1096 | I. 279 | 11 59 57·9 | 12 15 12 | e F; R; v g l b M | 413 | | | | | 60·0 | 15 7 | F; R; 1E; g b M; 20'' | 170 | | 1097 | II. 548 | 12 0 10·4 | 98 5 38 | pF; E; g b M; very ill defined | 137 | | | | | 10·8 | 5 4 | F; v g b M; E in parallel; 30'' l, 20'' br | 136 | | 1098 | III. 356 | 12 0 15·3: | 59 46 11 | vF; S; R; the n p of 3 in a line | 66 | | | | | 16·8: | 46 1 | F; S; R. | 68 | | 1099 | II. 371 | 12 0 18·8: | 59 48 51 | F; S; R; the second of 3 in a line | 68 | | | | | 21·5 | 48 7 | F; the n p of 2 (the third not seen) | 342 | | | | | 22·8 | 49 51 | vF; S; the second of 3 in a line | 66 | | 1100 | I. 278 | 12 0 28·6: | 14 8 57 | F; R; g b M. Strong twilight | 349 | | | | | 30·0 | 9 42 | pB; R; g b M | 413 | | 1101 | III. 357 | 12 0 28·8 | 59 52 41 | pB; 1E | 68 | | | | | 30·3 | 53 31 | F; p L; the third and s f of 3 in a line | 66 | | | | | 30± | 50 ± | B; the s f of 2; place by rough estimation | 342 | | 1102 | III. 795 | 12 0 58·7 | 30 11 59 | F; p L; 1E; g b M; 40'' | 345 | | 1103 | III. 814 | 12 1 0·1 | 35 56 5 | vF; irreg fig; v g l b M; twilight | 347 | | 1104 | IV. 54 | 12 1 12± | 46 34 2 | R; s b M to nucleus | 150 | | 1105 | I. 169 | 12 1 22·9 | 49 10 36 | pB; v L; dilute; v g l b M | 73 | 3 H 2 | No. | Synonym. | AR 1830°.0 | N.P.D.1830°.0 | Description and Remarks | Sweep. | |-----|----------|-------------|---------------|------------------------|-------| | 1106 | I. 19 | h m s | 70 29 41 | B; R; 80''; consists of distinct stars. A globular cluster. PD mistaken 1° in obs; corrected. | 61 | | | | | 24·4 30 47 | vB; resolved ......................... | 63 | | | | | 24·9 30 21 | vB; R; 40''. I see the stars of which it consists ........... | 334 | | 1107 | II. 747 | 12 1 21·8 | 42 36 9 | F; vmE in pos 109° by measure; vg bM 4' long, 30 or 40'' br | 255 | | | | | 23·5 36 27 | pB; gbM; a long narrow ray; 3' l, 30'' broad ............... | 140 | | 1108 | II. 321 | 12 1 34·9 | 59 8 4 | vF; vL; 5 or 6' diam. The minute in AR doubtful; perhaps 0m | 67 | | 1109 | II. 802 | 12 1 51·7 | 30 46 12 | No description .................................. | 323 | | 1110 | I. 73 | 12 1 55·0 | 58 39 4 | B; R; pgmbM; 25''; a * 8m 5' p ..................... | 342 | | 1111 | I. 165 | 12 1 55·2 | 49 38 41 | vsmbM to a * 10m; the sp of 2, 6' distant.............. | 73 | | | | | 55·7: | vB; S; R; pgbM; 30'' ..................... | 335 | | 1112 | II. 83 | 12 1 56·3 | 73 1 26 | vB; R; pgmbM; 40'' ..................... | 418 | | | | | 56·9 1 23 | No description .................................. | 422 | | | | | 57·1 1 31 | pB; S; R; gbM; 20'' ..................... | 419 | | 1113 | II. 642 | 12 2 12·7: | 49 36 51: | vF; 1E; vg bM .................................. | 335 | | | | | 17·3: | The nf of 2. Place by estimation from the other, and of course very rough. | 73 | | 1114 | I. 208 | 12 2 29·8 | 38 33 53 | B; vmE; vg lbM; 4' long .................. | 328 | | 1115 | II. 405 | 12 2 32·4 | 68 52 57 | vF; has a * nf .................................. | 59 | | 1116 | III. 941 | 12 2 36·3 | 12 55 47 | cF; R; makes equilateral triangle with 2 stars .......... | 413 | | 1117 | II. 353 | 12 3 15·2 | 64 55 48 | B; L; E; bM; 60'' ..................... | 58 | | 1118 | Nova. | 12 3 33·1 | 52 33 2 | F; pL; R; vg bM; a D * sp dist 10'. The MS obs makes the PD decidedly 33'; but should it be a mistake for 52', this nebula would be identical with III. 399. | 331 | | 1119 | II. 105 | 12 3 36·7 | 75 51 4 | B; R; psbM; irreg fig; r .................. | 242 | | 1120 | II. 372 | 12 3 40·8 | 59 53 1 | pB. The first of 4 in a trapezium .............. | 65 | | | | | 45·3 53 31 | The first of a trapezium .................... | 66 | | 1121 | III. 358 | 12 3 43·3 | 59 50 ± | The second of a trapezium .................. | 65 | | | | | 48± 50 ± | The second of trapezium. Place estim .......... | 66 | | 1122 | III. 359 | 12 3 44·3 | 59 55 ± | The third of trapezium. Place by estim .......... | 65 | | | | | 50± 56 ± | The third of trapezium; place by estim .......... | 66 | | 1123 | II. 742 | 12 3 46·1 | 32 52 57 | pF; S; E; gbM; 15'' l, 12'' br .............. | 345 | | 1124 | III. 360 | 12 3 53·3 | 59 54 ± | The last and largest (by diag) of trapezium .......... | 65 | | | | | 58± 53 ± | The last of trapez. Rough place .............. | 66 | | 1125 | Nova. | 12 4 5·4 | 78 11 40 | vF; vL; E; a * 7m folls 7' ± dist .......... | 191 | | | | | ... 12 32 | vF; Enf to sp; 40'' ..................... | 3 | | 1126 | I. 9 | 12 4 10·8 | 87 45 27 | pB; S; mE; a ray with a nucleus pos 45° np to sf ......... | 145 | | 1127 | II. 133 | 12 4 19·1 | 82 1 9 | B; R; psbM; 40'' ..................... | 117 | | | | | 21·6 0 43 | No description .................................. | 252 | | | | | 22·4 1 15 | pB; E; vg bM; 20'' ..................... | 250 | | 1128 | III. 697 | 12 4 40·4 | 45 22 47 | vF; L; vmE; 2' l, 30'' br .................. | 150 | | | | | 44·0 22 22 | vF; vmE, pos 170° ±; 90'' l, 30'' br .......... | 248 | | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|---------------|-------------------------|-------| | 1129 | II. 373 | 12 4 42°6' | 60 32°39" | v F; R | 67 | | | | 43°4 | 33 7 | p F; p L; R; g b M | 343 | | | | 45°2 | 33 2 | v F; v L; R; g b M; 2½' diam | 417 | | | | 49°3:: | 34 ± | Place coarsely estim from a neb following | 68 | | 1130 | Nova. | 12 5 5°8 | 81 51 7 | No description | 251 | | | | 7°8 | 51 13 | F; R; near a small * | 252 | | | | 8°2 | 51 7 | v F; R; b M | 253 | | | | 8°7 | 50 41 | No description | 254 | | 1131 | II. 106 | 12 5 6°9 | 75 38 10 | p B; L; 1 E; v g l b M; 2' diam | 338 | | 1132 | M. 98 | 12 5 8°0 | 74 8 12 | B; v m E, a ray, pos 70° s f n p; m b M almost to nucleus; 10' long; 6 comæ entered, bisected by the same horizontal wire. | 24 | | | | 8°1 | 9 0 | p B; v s b M to nucl; a long ray pos = 153°0 by meas; 8'...10'1, 30 br. | 419 | | | | 8°4 | 9 34 | B; L; m E pos 152°1 by meas; v s v m b M 8'...10' long. A fine object. | 422 | | | | ... | 9 16 | B; L; v m E; p s b M; precedes 6 comæ about 30' of space | 421 | | 1133 | II. 409 | 12 5 8°3 | 52 25 27 | v F; p L; R; v g l b M; 40" | 331 | | 1134 | II. 163 | 12 5 12°8 | 75 53 4 | v F; p L; E; v g b M | 242 | | 1135 | II. 867 | 12 5 36°5 | 34 30 45 | F; v s m b M to a * 12 m; 20" | 347 | | 1136 | II. 374 | 12 5 52°2 | 60 37 32 | B; v s v m b M to a * | 417 | | | | 52°8 | 38 37 | p B; S; p s b M | 343 | | | | 54°0: | 37 54 | F; S; R; b M | 68 | | | | 61°0 | 38 54 | B; S; s b M | 67 | | 1137 | II. 134 | 12 5 56°5 | 83 14 53 | p B; E; v g b M; 20"; like II. 133 | 250 | | 1138 | II. 164 | 12 5 58°3 | 76 53 46 | e F; R; b M | 19 | | | | 63°4 | 52 38 | p B; R; p s l b M; 40" | 340 | | 1139 | II. 793 | 12 5 59°8 | 33 2 17 | p F; S; 1 E; g b M; like II. 792 | 345 | | 1140 | I. 175 | 12 6 29°3 | 55 51 26 | B; R; s m b M | 74 | | | | 31°5 | 51 24 | v B; R; p s m b M | 131 | | 1141 | III. 397 | 12 6 36°5 | 68 24 10 | e F; L; v g l b M; 45" | 409 | | | | ... | 23 ± | e F | 424 | | 1142 | II. 107 | 12 6 47°7 | 75 9 24 | v F; p L; R; g b M | 243 | | 1143 | III. 850 | 12 6 55°0 | 23 4 28 | Not v F; p L; R; v g b M; 30" | 412 | | 1144 | II. 108 | 12 6 57°4:: | 75 8 40 | B; L; E; v g b M; 90"1, 75" br | 419 | | | | 61°9 | 9 20 | B; L; 1 E in parallel; at first gradually and then s b M; r; 3' diam | 338 | | 1145 | II. 354 | 12 7 0°2 | 65 3 58 | v F; v S; R | 407 | | 1146 | I. 95 | 12 7 5°1 | 52 44 2 | B; L; g b M; 50"; has a double nucl very indistinct. The diagram makes it a double neb, the two running together. See fig 71. | 331 | | 1147 | II. 135 | 12 7 11°3 | 82 39 6 | B; p L; irreg fig; g b M | 117 | | | | 12°8 | 39 7 | p B; E; p g b M; 25"1, 20" br | 253 | | | | 14°3 | 39 12 | v B; m E; v s b M to a * 11 m | 250 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1148 | I. 109 | 12h 7m 14s.7 | 75° 54′ 4″ | B; E; r .................................................. | 192 | | | | | 15′.4 | vB; vL; a nucleus with two branches extended in pos 75° n f to s p. (See fig 59.) | 242 | | | | | ... | A very remarkable long ray extended 70° n f to s p, 7½′ long, s m b M. It has a * n f the nucleus. Rough place. | 3 | | | | | ... | B; mE; p s b M. (N.B. No neb at 76° 2′. Seen also in Sw 2, but the place and description too rough to be of use.) | 340 | | 1149 | II. 748 | 12h 7m 17s.1 | 41° 57′ 16″ | F; mE; s of 2 bright stars .................................. | 329 | | | | | 18′.8 | pB; v m E in pos = 225°.0 by meas; 5′ l, 1′ br; 2 st near and a L * p. | 255 | | | | | 19′.5 | F; mE; 2′l; has 2 st, 9 and 11 m, n f ....................... | 138 | | | | | 19′.9 | F; L; E; has a * 1° following and another near ............... | 139 | | | | | ... | g b M; E; 70° n f to s p; is s of a coarse double * .......... | 140 | | 1150 | Nova. | 12h 7m 41s.2 | 22° 49′ 23″ | pB; S; R; p s b M; 15″ ..................................... | 412 | | 1151 | I. 209 | 12h 7m 42s.7 | 41° 10′ 33″ | pB; p m E in pos = 314°.4; p s b M. (Foggy.) ................ | 330 | | 1152 | II. 137 | 12h 7m 45s.5 | 82° 21′ 31″ | pB; R; AR estimated from III. 480, which it precedes on same parallel. | 254 | | 1153 | II. 136 | 12h 7m 46s.4 | 81° 35′ 44″ | pB; pL; 1E; g b M ......................................... | 251 | | | | | 53′.3 | pB; R. Hazy, clouding over .................................. | 252 | | 1154 | Nova. | 12h 7m 52s.6 | 101° 21′ 49″| F; eS; R; 5″; has a * 8 m, 80° s f, dist 60″ ............... | 129 | | 1155 | Nova. | 12h 7m 58s.7 | 42° 2′ 32″ | F; S; 1E; the second of 2 in field .......................... | 139 | | 1156 | II. 518 | 12h 7m 59s.8 | 55° 32′ 36″ | pB; R; b M .................................................. | 74 | | | | | 61′.3 | pF; R; p s b M; the s p of 2 ................................ | 131 | | 1157 | Nova. | 12h 8m 1s.5 | 52° 43′ 41″ | vF; L; R; g b M; 90″ ....................................... | 72 | | 1158 | II. 519 | 12h 8m 4s.8 | 55° 30′ 1″ | The n f of 2 ................................................ | 74 | | | | | 7′.3 | F; R; p s b M; 65° n f the neb II. 518 ...................... | 131 | | 1159 | II. 17 | 12h 8m 24s.2 | 81° 51′ 24″ | pB; 1E; g b M .............................................. | 251 | | | | | 29′.1 | vB; p m E; v s b M; among small st ........................ | 253 | | 1160 | Nova. | 12h 8m 27s.5 | 85° 22′ 30″ | pB; L; R; g b M; 60″ ....................................... | 141 | | 1161 | II. 496 | 12h 8m 27s.8 | 81° 25′ 59″ | pB; R; v s b M to a S nucleus; 20″ .......................... | 254 | | 1162 | II. 11 | 12h 8m 31s.5 | 73° 45′ 2″ | eF; but haze and strong twilight ............................ | 27 | | | | | 33′.0 | B; L; 1E; v g b M .......................................... | 422 | | 1163 | V. 17 | 12h 8m 37s.3| 19° 38′ 0″ | Immensely L; v F; m E; v g b M; it fills more than a field, but is hardly distinguishable. Hazy. | 377 | | 1164 | III. 851| 12h 8m 37s.5| 25° 38′ 56″ | vF; not v S; R; v g l b M; 15″...20″ ...................... | 411 | | 1165 | III. 480| 12h 8m 45s.5| 82° 23′ 11″ | vF ............................................................ | 254 | | | | | 45′.7 | vF; v g b M; a * 7 m to south ............................... | 250 | | 1166 | III. 725:| 12h 8m 48s.9| 43° 26′ 9″ | F; vL; R; v g b M; diam in AR = 15°.0 of time. Sky quite clear. C illuminating wires. | 256 | | | | | 51′.9 | F; L; R; v g b M; r; has * 10 m, 2′ f ...................... | 140 | | 1167 | V. 41 | 12h 8m 56s.7| 51° 15′ 12″ | F; v m E; a v long narrow ray pos = 43°.2 by meas, at least 9 or 10′l, extends across the field. | 331 | | | | | 57′.8 | pB; v m E; a long ray, 50° n f to s p ± by estim; 12′ l, 90″ br | 73 | | No. | Synonym | R 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|-----------|----------------|-------------------------|--------| | 1168 | I. 74 | 12 8 59'6 | 59 26'' | B; pL; r | 66 | | | | | 62'1 | vB; R; sbM; 60'' | 65 | | | | | 62'9 | vB; pL; R; psbM | 342 | | 1169 | II. 742 | 12 9 17'8 | 41 38 46 | eF; hazy | 329 | | | | | 20'0 | vF; pmE; psbM | 255 | | 1170 | I. 264. | 12 9 31'3 | 18 15 17 | pF; S; R; pgbM; 15'' | 377 | | 1171 | I. 89 | 12 9 31'7 | 60 52 52 | vB; vsmbM; has *6.7 m 1½ min (of time) following | 417 | | | | | 33'2 | vB; S; mE; vsmbM; nucleus elliptic | 343 | | | | | ... | vB; R; bM | 68 | | 1172 | III. 702| 12 10 0± | 59 13 ± | vF; R; 20'' | 342 | | 1173 | M. 99 | 12 10 9'9 | 74 38 36 | Not vB; R; vgbM; 5' diam | 421 | | | | | 10'0 | pB; vL; R; gBM; r; 5' diam | 422 | | | | | 10'8: | B; R; gBM; r; 5' diam | 419 | | | | | ... | B; L; R; gBM. Seen through cloud | 418 | | 1174 | II. 846 | 12 10 29'1| 23 9 23 | pB; vmE in pos = 218°2; 90'1 | 412 | | 1175 | V. 43 | 12 10 30'8| 41 45 18: | vB; vL; vsvmbM to an oval nucl; 8 or 9' long, 4 or 5' broad. (See fig 55.) | 330 | | | | | 32'7 | vB; vL; vsbM to an oval nucleus which is not in the middle of its length; 6' l, 3' br. | 255 | | | | | 32'7 | vB; vL; sbM to a *; 6' l, 4' br | 329 | | | | | ... | vB; L; vmE | 256 | | 1176 | II. 139 | 12 10 32'7| 83 13 51 | vB; pL; R; psmbM; 40'' | 250 | | 1177 | II. 138 | 12 10 40'7| 82 57 33 | pB; through thick haze | 252 | | | | | 41'3 | B; E; psbM | 253 | | 1178 | Nova. | 12 10 41'1| 83 43 ± | Precedes four more, nearly in parallel | 117 | | 1179 | II. 110 | 12 10 50'6| 74 10 51 | B; S; R; like a * 11 m with a burr | 421 | | 1180 | II. 140 | 12 10 54'4| 83 12 30 | pF; R; gBM; 30'' | 250 | | 1181 | II. 166 | 12 11 5'2 | 76 16 15 | pB; R; sbM | 191 | | | | | 7'7 | pB; R; vsmbM, almost to a * | 243 | | 1182 | III. 299| 12 11 14'3| 58 42 49 | eF; vS; R; 10'' | 342 | | 1183 | Nova. | 12 11 16'3| 83 43 34 | B; L; E; gBM | 238 | | 1184 | II. 376 | 12 11 18'2| 61 26 17 | F; R; gBM; 20'' | 343 | | | | | ... | F; 1E; near a * 15 m | 417 | | 1185 | I. 75 | 12 11 16'6| 59 26 15 | vB; vL; Ein parallel; 2' 1, 1½' br | 65 | | 1186 | I. 90 | 12 11 32'6| 59 46 21 | vB; R; smbM; r | 66 | | | | | 32'7 | vB; pL; R; gmbM; 90'' | 67 | | 1187 | II. 573 | 12 11 40'6| 83 40 34 | vB; vL; R; pgBM; 3'; 3 more seen | 238 | | 1188 | II. 377 | 12 11 47'7| 59 44 29 | B; R; S; bM; 30'' | 67 | | | | | 48'1 | B; R; sbM | 66 | | 1189 | Nova. | 12 11 53± | 83 44 ± | vF; S | 117 | | 1190 | Nova. | 12 12 3'1 | 83 42 34 | vB; R; the central neb of 4 in a trefoil | 117 | | No. | Synonym | AR 1830°. | N.P.D. 1830°. | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1191 | III. 726 | h m s 12 12 10'0 | 42 45 34 | p F; R; v g b M; 60'' | 138 | | | | | | v F; L; v g b M; irreg R; r | 140 | | | | | | e F; p L; R | 139 | | 1192 | I. 275 | 12 12 14'5:: | 13 41 2 | p F; S; E. The reductions of the AR in this sweep are precarious. | 348 | | | | | | F; S; s b M; 10''; a * 15 or 16 m precedes | 170 | | | | | | p B; stellar; v s m b M. The first of a trapezium of stars | 413 | | | | | | p F; R; g b M; 20''; followed and almost surrounded by 3 stars | 349 | | | | | | 10 m, one of which is double; has also a v S * s p dist 30''. | | | 1193 | II. 805 | 12 12 20'2 | 30 57 37 | p B; L; R; g b M; 60'' | 345 | | 1194 | Nova. | 12 12 28'6 | 83 40 34 | v B; E; b M; 60''. | 117 | | | | | | p F; R | 251 | | 1195 | V. 5 | 12 12 32'2 | 70 39 36 | F; v L; E; b M; 5' 1, 1½ br | 61 | | | | | | L; E; 1b M | 63 | | 1196 | Nova. | 12 12 34'2 | 84 27 32 | F; R; v g l b M; has a * 70° n p; 1' dist. Taken for I. 139, but this neb does not exist, or is identical with M 61. | 143 | | | | | | F; S near a B *; precedes M. 61 about half a field | 141 | | 1197 | II. 61 | 12 12 33'8 | 77 33 19 | p B; p L; E n p to s f; has another f in same parallel. | 19 | | | | | | F; L; b M; E 45° n p to s f; 2' l, 1' br | 22 | | | | | | F; v m E; like a double neb composed of 2 R nebulae. | 242 | | | | | | F; m E; L; v g b M; 3' long | 338 | | 1198 | II. 111 | 12 12 53'2 | 74 27 16 | F; L; E; v g b M; a star follows; the p of 2 | 421 | | | | | | The p of 2; by diagram E in merid, nearly parallel to the other | 422 | | | | | | L; v m E nearly in merid; the f of 2 | 421 | | | | | | The f of 2; both m E and nearly parallel | 422 | | 1200 | II. 62 | 12 13 0'7 | 77 33 0 | F; p L; E. (Seen also in Sw 19.) | 242 | | | | | | v F; L; 1E; v g b M; 3' | 338 | | 1201 | II. 572 | 12 13 1'2 | 83 40 23 | F; 1E; v g b M | 250 | | 1202 | M. 61 =I.139 | 12 13 12'8 | 84 34 55 | B; v L; v s b M to a * 11 m, with a v F atmosphere about it. This nebula is probably identical with I. 139. (See fig 69.) | 141 | | | | | | B nucleus in a v F atmosph 2' diam, gradually fading away | 142 | | | | | | Viewed; v faintly bicentral. The two nuclei 90'' dist pos 45 ... 50° n f. | 143 | | 1203 | Nova. | 12 13 25'2 | 76 19 35 | v F; R | 191 | | 1204 | I. 76 | 12 13 53'0 | 59 9 46 | v B; E; s b M; points to * 60° n p | 65 | | 1205 | II. 378 | 12 13 54'± | 59 50 ± | v B. The n p of 2 | 68 | | | | | | Past merid. No AR procured | 67 | | 1206 | Nova. | 12 13 54'0 | 59 51 8 | F; the s f of two | 68 | | 1207 | II. 63 | 12 13 58'0 | 77 17 12 :: | e F; E 45° n p; r in middle | 3 | | | | | | v F; L; R; 60'' | 243 | | 1208 | Nova. | 12 14 5'7: | 80 51 20 | e F; a * 8 m 5' dist, on merid, to n | 120 | | 1209 | II. 628 | 12 14 9± | 73 30 57 | p B; p L; E; g b M; AR by working list | 419 | | No. | Synonym. | AR 1830-0. | N.P.D. 1830-0. | Description and Remarks. | Sweep. | |-----|----------|------------|----------------|-------------------------|--------| | 1210 | I. 276 | 12 14 10·5 | 13 43 48 | pB; S; sbM; 15" | 170 | | | | 16·9 | 44 27 | pB; pL; bM. Follows I. 275 | 413 | | | | 19·7 | 43 42 | F; R; bM; 18"; the f of two in field | 349 | | 1211 | M. 100 | 12 14 17·9 | 73 14 34 | pB; R; psmbM. Not a very remarkable nebula. II. 84 was not seen. | 422 | | | | 19·3 | 13 39 | Barely visible through cloud | 418 | | | | 20·8 | 13 26 | vL; smbM; a nucleus with dilute borders | 25 | | | | ... | 13 56 | vF; vL; R; vsbM to a pB nucleus | 421 | | 1212 | II. 85 | 12 14 30·0 | 72 20 5 | pB; R; psbM. | 419 | | 1213 | II. 141 | 12 14 30·2 | 82 58 51 | vF; S; R; bM; 10"; the first of 3 in a triangle | 254 | | 1214 | Nova. | 12 14 35·8 | 101 35 29 | F; vS; R; bM to nucleus | 129 | | 1215 | II. 142 | 12 14 40·7 | 83 1 1 | F; pS; R; bM; 15"; the second of 3 in a triangle | 254 | | 1216 | II. 847 | 12 14 41·3 | 23 12 43 | F; R; vgbM; 20" | 412 | | 1217 | II. 806 | 12 14 41·6 | 30 36 52 | pF; S; bM | 323 | | | | 41·9 | 37 12 | pB; S; E; gM; good obs of place | 345 | | 1218 | Nova. | 12 14 44·3 | 81 35 7 | pF; R; S; close to a * | 253 | | 1219 | II. 406 | 12 14 47·2 | 69 38 22 | vF | 63 | | | | 52·8 | 37 56 | F; pL; R; bM | 61 | | 1220 | III. 942 | 12 14 52·1 | 12 53 7 | eF; hardly discernible | 413 | | 1221 | II. 86 | 12 14 52·5 | 72 21 5 | vB; mE; vsbM; 35" long | 419 | | 1222 | II. 143 | 12 14 54·2 | 82 58 31 | B; R; pL; psbM; 30"; the third in a triangle | 254 | | | | 54·8 | 57 44 | B; R; gM; neat and bright, but only one seen. (This must therefore be the brightest.) | 251 | | | | 55·3 | 58 14 | pB; R; has a * 10 m 1' s | 117 | | 1223 | III. 94 | 12 14 58·3 | 82 6 59 | pB; E, or has a F neb on the sf side | 250 | | 1224 | III. 31 | 12 15 1·6 | 71 31 1 | F; not vS; R; vglbM; 25" | 334 | | 1225 | I. 210 | 12 15 4·5 | 42 3 23 | pB; S; pmE; psbM; 40" | 330 | | | | 5·8 | 5 34 | B; S; E; vsbM; 50" l, 20" br | 255 | | | | 6·5 | 3 59 | vB; S; mE; vsmbM | 138 | | | | 6·5 | 4 13 | vB; a* with a short sharp ray; by diagpos 10° sf to np. (See fig 57.) | 140 | | | | 6·6 | 3 52 | vB; S; mE in parallel; vsmbM to nucleus | 139 | | | | ... | 3 46 | B; S; R; psbM; hazy | 329 | | 1226 | II. 625 | 12 15 4·6::| 92 30 4 | F; irreg R; a small * p. (AR reductions in this sweep considerably uncertain.) | 21 | | | | 10·8 | 30 32 | F; pL; E; vlbM. (AR to be preferred.) | 146 | | 1227 | II. 64 | 12 15 25·4 | 77 50 13 | vF; S; 1E; (nisi AR = 12h 16m 25·4) | 338 | | | | ... | 49 30 | No description or observed AR | 340 | | 1228 | I. 123 | 12 15 37·5 | 84 7 32 | B; visible in strong twilight; has a * 8.9 m 20° sf dist 3'; (nisi AR = 12h 16m 25·4). | 153 | | 1229 | III. 648 | 12 15 40·1 | 57 32 25 | F; pmE, nearly in parallel; vlbM; 25" | 342 | | 1230 | III. 799 | 12' 15 42·1| 30 40 32 | F; 1E; the p of 2 | 345 | | 1231 | I. 65 | 12 15 43·4 | 107 50 4 | vB; L; R; vsmbM to nucl = *11 m 90" diam. r with power 320, and is no doubt a globular cluster; fades away to nothing. | 149 | MDCCXXXIII. | No. | Synonym. | R 1830°. | N.P.D. 1830°. | Description and Remarks. | Sweep. | |-----|----------|----------|---------------|--------------------------|--------| | 1232 | I. 30 | h m s | 12 15 49° | v B; R; at first g b, then s m b M; 50'' | 251 | | | | | 50° | Just visible through cloud | 252 | | | | | ... | No description | 253 | | 1233 | III. 800 | 12 15 50° | 30 41 32 | e F; the last of 2. (The other was III. 799; III. 801 not seen.) | 345 | | 1234 | I. 166 | 12 16 10° | 49 40 39 | p B; R; s m b M almost to a * | 73 | | | | | 11° | v B; R; p g m b M; 30''; r | 335 | | 1235 | I. 22 | 12 16 14° | 77 21 32 | g b M; 20''. Rough place. | 3 | | | | | 14° | B; R; g b M; 30'' | 22 | | | | | 15° | B; R | 191 | | | | | ... | v F; R; v g b M; 20''; very rough place. | 2 | | 1236 | II. 144 | 12 16 14° | 81 36 29 | p F; R; b M; 40'' | 117 | | | | | 14° | p B; S; E | 253 | | 1237 | M. 84 | 12 16 26° | 76 10 9 | v B; R; p s b M; 60''; r | 192 | | 1238 | II. 379 | 12 16 29° | 60 30 13 | F; R; has a S * 35° n f, 90'' dist. | 66 | | | | | 29° | F; R; b M | 68 | | 1239 | I. 12 | 12 16 36° | 74 17 44 | B; S; v s m b M | 422 | | 1240 | Nova. | 12 16 41° | 73 25 31 | p L; R; s m b M to nucleus | 25 | | 1241 | Nova. | 12 16 45° | 79 3 1 | v F; p L; R; 1 b M | 19 | | 1242 | M. 85 | 12 16 47° | 70 51 56 | v B; R; b M; 2' diam; has a * 80° n p dist 30'' from edge | 61 | | | | | 49° | v B; v s b M; 60'' | 334 | | 1243 | III. 879 | 12 16 54° | 34 32 50 | e F; hardly sure that I see it. Sky very dull | 346 | | | | | 56° | p B; S; R; g b M; 12...15'' | 347 | | 1244 | Nova. | 12 17 9° | 76 24 34 | v F; E; the p of 2, dist about 30° in R A | 192 | | 1245 | II. 749 | 12 17 11° | 43 22 29 | F; v L; E; v g l b M; 2' l, 1½ br. | 255 | | | | | 11° | p B; p L; irreg R; g b M | 140 | | | | | 14° | p F; p L; m E | 139 | | 1246 | III. 361 | 12 17 18° | 61 29 50 | F; irreg fig; has a line of B st preceding. | 68 | | 1247 | I. 277 | 12 17 18° | 13 32 17 | p B; 1 E; p s m b M; 25'' | 348 | | | | | 18° | B; 1 E; p s m b M | 349 | | 1248 | III. 852 | 12 17 18° | 24 7 18 | v F; S; R; s b M. Has a triple * s p. | 412 | | | | | 20° | p B; S; b M; 12''. Near a p B triple * | 411 | | 1249 | III. 729 | 12 17 19° | 43 15 21 | F; S; R; v g b M. AR from II. 749, which it follows 10° | 140 | | 1250 | II. 167 | 12 17 20° | 76 19 2 | These and several more seen | 3 | | | II. 168 | | | | | | 1251 | II. 55 | 12 17 20° | 70 50 41 | p B; 1 E; b M. In field with M. 85 | 61 | | | | | 21° | p B; 1 E. Follows M. 85. | 334 | | 1252 | V. 29.1 | 12 17 22° | 55 30 36 | Two nebulae running into one another; both e F; v L; the f rather the brighter. Place that of the preceding. (See fig 68.) | 74 | | | V. 29.2 | 12 17 29° | 55 32 36 | The following nebula of V. 29 | 74 | | | | | 33° | v L; extremely ill defined, may perhaps be 10' l, 3' br; p s l b M to an irregular centre. On closer examination bicentral; pos of the nuclei 30° n p; dist 2'. | 131 | | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 1253 | Nova. | 12 17 28'9 | 76 7 6 | vB; R; g b M to nearly a star | 22 | | | | 35°0:: | 7 14 | vB; L; p g m b M; r. (RA precarious.) | 243 | | 1254 | II. 88 | 12 17 32'3 | 72 53 11 | pB; R; v s b M; 30'' | 421 | | 1255 | Nova. | 12 17 39'8:: | 76 25 ± | The following of 2 | 192 | | 1256 | Nova. | 12 17 43'0 | 80 2 45 | eF; vL; R; g b M; 2½ diam | 120 | | 1257 | II. 34 | 12 17 53'9 | 85 6 0 | F; pL; g b M | 141 | | | | 54'8 | 5 49 | F; L; R; v g b M | 238 | | 1258 | I. 77 | 12 17 59'5 | 57 50 3 | vB; L; p m E, first g b and then v s v m b M to a nucleus | 342 | | | | ... | 50 38 | = * 11 m; 3'1, 90'' br. | 74 | | 1259 | II. 169 | 12 18 1'1:: | 76 29 32 | B; L; lE; s m b M; 4'1, 3' br. | 3 | | 1260 | Nova. | 12 18 5'6 | 81 8 24 | vF; L; R; 60''; has * 7 m, 5' sp | 117 | | 1261 | III. 492 | 12 18 12'4 | 89 56 37 | F; S; R; near a * | 146 | | | | ... | 56 42 | F; R; b M | 145 | | 1262 | II. 113 | 12 18 18'2 | 74 0 52 | B; E, n p to s f; s b M | 24 | | 1263 | II. 23 | 12 18 18'3 | 86 33 33 | vF; lE; 30''. This may possibly be identical with III. 17 | 143 | | | | 19'2 | 33 56 | pB; r | 142 | | 1264 | II. 89 | 12 18 26'5 | 73 35 46 | pB; R; p g b M | 422 | | | | 30'8 | 34 36 | A star n p | 25 | | 1265 | III. 492 | 12 18 26'9 | 94 53 1 | vF; S; R; p s b M | 147 | | | | 27'5 | 53 21 | Not vF; R | 234 | | 1266 | II. 145 | 12 18 29'9 | 83 10 43 | vF; vS; E | 250 | | 1267 | II. 170 | 12 18 31'2: | 76 20 22 | pB; S; R; b M | 19 | | | | 36'1 | 19 59 | No description | 242 | | 1268 | II. 171 | 12 18 36'9: | 76 45 45 | vF; oval; g b M; 50'' | 340 | | 1269 | Nova. | 12 18 43'4 | 97 14 15 | pL; vF; very ill defined | 137 | | 1270 | II. 146 | 12 18 46'3 | 82 48 37 | vF; L; R; g b M; 90'' | 253 | | | | 49'1 | 47 24 | vF; vL; R; v g b M; 50'' | 251 | | 1271 | Nova, or II. 65 | 12 18 48'3 | 77 57 15 | B; L; p m E; p s b M; has * 10 m n f, 1' distance | 191 | | | | 50'3 | 58 26 | vB; L; E; has * n f; 2' dist, pos = 29°·4 by micrometer | 245 | | 1272 | II. 172 | 12 18 50'9: | 76 43 55 | vF; g b M; 40'' | 340 | | 1273 | Nova. | 12 18 53'4 | 97 20 50 | Not vF; pL; lE; very ill defined | 137 | | 1274 | M. 86 | 12 18 57'9:: | 75 60 1 | The preceding of 2 | 22 | | | | 62'4 | 58 19 | No description | 338 | | | | 62'6 | 59 24 | vB; R; 30'' | 242 | | 1275 | I. 28 | 12 19 2'9: | 76 3 46 | B; R. The f of 2 | 22 | | | | 6'1 | 3 34 | pB; L; lE; 60'' | 242 | | | | 7'4 | 2 34 | pB; vL; the f of 2 | 338 | | 1276 | II. 173 | 12 19 3'9 | 76 45 50 | B; R; b M; 50''; r | 340 | | 1277 | Nova. | 12 19 7'2 | 88 55 42 | F; v m E, pos 15° n f to s p; a long ray; it is s p a * 10 m. The place is that of the star. | 145 | | No. | Synonym | N.P.D. 1830-0. | R 1830-0. | Description and Remarks | Sweep | |-----|---------|----------------|-----------|------------------------|-------| | 1278 | II. 848 | 12 19 24·1 | 24° 15' 0" | p F; R; v g b M; 25" | 411 | | 1279 | II. 156 | 12 19 26·6 | 79 14 55 | v B; R; s m b M; 30" | 120 | | 1280 | I. 91 | 12 19 43·8 | 60 26 41 | B; L; 1E | 65 | | | | | 45·4 | 26 42 | p B | 417 | | | | | 45·7 | 26 42 | B; L; m E exactly in parallel; s m b M | 343 | | | | | | 26 11 | No description | 415 | | 1281 | I. 213 | 12 19 47·2 | 44 58 42 | B; L; g b M; E in pos 75° n f to s p a fine cluster; well resolved; I see several of the stars; 3' l, 2' br. | 150 | | | | | 49·4 | 58 8 | v B; resolved; has as it were a forked tail | 151 | | | | | 49·6 | 57 52 | v F; v L; v m E; it is either a double neb, or the n f end is bifid. If double the companion is F; R; b M; nearly north dist 1½' or 2'. A fine object. | 248 | | | | | 50·6 | 57 57 | v B; v L; m E. The centre is fairly resolved; 3' l, 2' br. Borders hazy. | 139 | | 1282 | II. 56=II. 90 | 12 19 53·2 | 71 58 44 | B; p L; R; p s b M; 2' | 422 | | | | | 53·7 | 59 2 | p L; R; b M nearly to nucleus | 27 | | | | | 53·9 | 58 55 | v B; L; R; p s b M; 60" | 419 | | | | | 54·4 | 58 2 | v B; 1E; p g b M; 100". (N.B. II. 90 and II. 56 appear to be identical.) Carefully examined. No other found near the place. | 334 | | | | | 54·5 | 58 6 | B; L; R; g v m b M to a stellar nucleus | 25 | | | | | 54·6 | 58 57 | p B; p L; R; b M | 63 | | | | | | 58 19 | F; p L; has a * 9 m s p; 5' dist | 418 | | | | | | 57 38 | p B; L; b M; 60"; r | 61 | | 1283 | II. 26 | 12 20 7·3 | 82 32 51 | e F | 254 | | 1284 | II. 180 | 12 20 7·9 | 91 0 12 | F; R; g b M; 20"; a stellar point 18 m in the centre; 2 B st precede, distant. | 146 | | 1285 | II. 355 | 12 20 11·0 | 66 14 30 | p B; p m E; g b M; two B stars n f | 424 | | | | | 11·4 | 14 25 | v F; p L; 1E | 409 | | 1286 | II. 35 | 12 20 18·1 | 85 29 19 | B; R; v s b M; 20" | 288 | | | | | 18·2 | 29 3 | B; R; p s b M; 30" | 143 | | | | | 18·5 | 29 14 | v B; S; R; s m b M to nucl = * 10 m | 142 | | 1287 | II. 121 | 12 20 20·4 | 75 49 8 | p B; R; p s b M; the p of 2 | 338 | | 1288 | I. 161 | 12 20 22·1 | 75 4 20 | p B; R; b M; r; has * 8 m 2' dist, 45° s f | 23 | | | | | 24·0 | 5 34 | F; R; b M; 30" | 243 | | 1289 | I. 212=II. 750 | 12 20 24·7 | 44 10 31 | p B; p L; E; p s b M. (I. 212 and II. 750 seem to be identical.) | 255 | | | | | | 13 ± | B; m E; rough place | 140 | | 1290 | II. 122 | 12 20 25·9 | 75 52 23 | p B; R; p s b M; the f of 2 | 338 | | | | | | 51 3 | v F; R; v g b M; 15" | 2 | | 1291 | II. 848? | 12 20 41·0 | 24 15 43 | p B; R; g b M. (N.B. My Father's P D; if this be the nebula, II. 848 is nearly 6' in error.) | 412 | | 1292 | III. 483 | 12 20 43·9 | 80 54 5 | p B; v S; p g b M; R; 10" | 250 | | No. | Synonym | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|-------------|----------------|------------------------|-------| | 1293 | II. 18 = II. 498 | 12h 20m 58s.1 | 81° 14' 14" | B; L; irreg R; b M; r ........................................... | 117 | | | | | 59° 6' | v F; R; b M ...................................................... | 251 | | 1294 | M. 49 | 12h 21m 7s.0 | 81° 3' 32" | R; p g m b M; 40". Through cloud; twilight .................. | 153 | | | | | 7° 3' | Seen in strong twilight; a very good obs of place; has a * 13 m 0° f; 60". | 154 | | | | | 8° 1' | v B; R; v s b M; 2' diam; a * 4° 0 f .......................... | 250 | | | | | 8° 7' | e B; L; R; p s m b M; insensibly fading away, has a * 13 m f; by diag the star is just beyond the nebula. | 253 | | | | | 10° 1':: | B; L. Cloudy .................................................................. | 252 | | 1295 | II. 629 | 12h 21m 17s.1 | 74° 59' 22" | p B; R; b M; 20" .................................................... | 24 | | 1296 | II. 123 | 12h 21m 17s.8 | 76° 44' 23" | The first of 3 ................................................................ | 19 | | | | | 23° 4' | F; R; S; b M .................................................................. | 245 | | | | | | v F; R; place estimated, but too roughly to be of any use .... | 191 | | 1297 | III. 362| 12h 21m 18s.8| 61° 48' 37" | e F; R; 15" .................................................................. | 417 | | | | | | e F; no R A procured ................................................ | 343 | | 1298 | II. 124 | 12h 21m 36s.6| 76° 45' 23" | No description; R A precarious .................................. | 19 | | | | | 39° 3' | p B; R ......................................................................... | 191 | | | | | 41° 7' | No description. (Obs probably hurried.) ......................... | 192 | | | | | 42° 0' | B; S; R; p s b M; 30"; the f of 2 ................................ | 245 | | | | | 49° ± | RA roughly estimated from M 87, mistaken for II. 123 ........ | 22 | | 1299 | III. 531| 12h 21m 45s.9| 84° 48' 45" | F; S; E ......................................................................... | 141 | | 1300 | Nova. | 12h 22m 4s.1 | 100° 41' 54" | Not v F; R; g b M; 20" ............................................... | 129 | | 1301 | M. 87 | 12h 22m 8s.7 | 76° 40' 9" | v B; R; 60". (Mistaken for II. 124.) .......................... | 22 | | | | | 12° 3' | v B; v L; R .................................................................. | 191 | | | | | 12° 7' | p B; L; R ..................................................................... | 192 | | | | | 17° 7' | v B; v L; R; p s m b M; r; 3' diam ................................ | 245 | | | | | | v B; R; b M. (Taken past merid; P D too great.) ............... | 19 | | 1302 | III. 484| 12h 22m 13s.1| 80° 41' 40" | v F; v S; 1E ................................................................ | 120 | | 1303 | II. 91 | 12h 22m 17s.0| 72° 18' 15" | F; R; g b M .................................................................. | 419 | | | | | 17° 1' | B; S; R; 25" ................................................................ | 421 | | | | | 17° 8' | F. In other respects like II. 56 .................................. | 25 | | 1304 | III. 41 | 12h 22m 18s.8| 77° 35' 5" | p B; L; R; 40" ....................................................... | 247 | | 1305 | III. 499| 12h 22m 21s.7| 80° 59' 16" | p B; p L; v g l b M; near two small stars ...................... | 254 | | 1306 | I. 197 | 12h 22m 49s.7| 47° 26' 40" | S; R; is 70° n p and 3' n of I. 198 .............................. | 150 | | 1307 | I. 83 | 12h 22m 54s.4| 63° 16' 58" | v B; R; v s m b M to a nucl; 40...50" ............................ | 58 | | 1308 | I. 198 | 12h 22m 55s.5| 47° 29' 28" | v B; v L; m E; 40° n p to s f; easily r .......................... | 150 | | 1309 | II. 36 | 12h 22m 55s.9| 85° 7' 23" | No description ................................................................ | 143 | | | | | 57° 7' | A double neb; v F; p L; both R; pos 45° s f by diag; the two are in contact; unequal. | 141 | | | | | 60° 5' | Not v F; v L; R; v g b M ......................................... | 142 | | No. | Synonym | R 1830-0 | N.P.D. 1890-0 | Description and Remarks | Sweep | |-----|---------|----------|--------------|------------------------|-------| | 1310 | III. 301 | h m s | 12 22 56·8 | 59 55 1 | F; R; 30" .................................................. 65 | | | | | | ... 55 20 | p F; R; ps lb M ........................................... 417 | | 1311 | I. 234 | | 12 23 16·7 | 31 6 17 | p B; E; pg b M; a * 9 m f 30" dist in parallel ............ 328 | | 1312 | M. 88 | | 12 23 28·4 | 74 38 19 | B; v L; v m E; 8' 1, 1' br. The northern half is brighter than the southern. | | | | | | 23·5 38 17 | B; L; E; b M to nucl; pos (by diag) = 140° 0 ±; has a * just at its sf extremity. | | | | | | 24·0 38 50 | v B; v L; E; g b M. Seen through cloud .................. 23 | | | | | | ... ...... | Viewed; m E in pos = 143° 4 by microm; ps mb M; 7' 1, 1' br | | | | | | 37 9 :: | A mere glimpse through a cloud .......................... 418 | | | | | | 38 ± | pos = 145° 3 by microm; 8' 1, 1' br; s v m b M; has a double star sf. | | 1313 | II. 66 | | 12 23 26·0: | 77 53 32 | R; g b M; 30" .............................................. 3 | | | | | | 28·7 53 4 | p B; R; g b M; 30" ....................................... 242 | | 1314 | II. 92 | | 12 23 28·6 | 72 22 26 | e F .......................................................... 421 | | 1315 | III. 18 | | 12 23 35± | 85 4 56 | e F; the following of 2 in the field ..................... 142 | | 1316 | II. 631 | | 12 23 35·8 | 75 38 26 | v F; p m E in parallel; g b M; a * 9 m, 8' f ............ 340 | | 1317 | Nova. | | 12 23 38·2 | 83 14 4 | v S; R; a * 13 m with a burr ............................. 251 | | 1318 | Nova. | | 12 23 45·4 | 56 58 2 | v F; S; R; l b M .......................................... 131 | | 1319 | III. 834 | | 12 24 8·9 | 32 35 57 | Not e F; S; R; v g b M; 12" ................................ 345 | | 1320 | III. 302 | | 12 24 17·5 | 59 20 22 | v F; R; b M; 15" ......................................... 342 | | | | | | 23·9 21 29 | e F .......................................................... 68 | | 1321 | Nova. | | 12 24 23·1 | 25 19 53 | p B; R; ps b M; 20" ....................................... 412 | | 1322 | Nova. | | 12 24 31·6 | 81 12 34 | F; S; R; b M; 20" ......................................... 117 | | 1323 | III. 78 | | 12 24 32·2 | 74 28 45 | F; R; v g b M; 40" ....................................... 419 | | 1324 | II. 93 | | 12 24 33·3 | 72 46 26 | F; an extremely dilute nebulosity, with a centre almost stellar. | | 1325 | Nova. | | 12 25 1·6 | 79 52 50 | e F; p L; 1E; vl b M ..................................... 120 | | 1326 | Nova. | | 12 25 4·7 | 25 27 21 | p B; p m E; pg b M; 20" 1, 12" br; a * 9 m near ......... 411 | | 1327 | Nova. | | 12 25 4·9 | 101 4 29 | v F; irreg R; b M ....................................... 129 | | 1328 | II. 325 | | 12 25 24± | 58 48 ± | p F; L; R; 60". (RA by working list.) .................... 342 | | 1329 | I. 38 | | 12 25 24·4 | 81 22 2 | v B; m E; ps mb M; r; a L * follows ..................... 253 | | | | | | 24·9 21 54 | v B; m E; ps mb M; a * 8 or 9 m p ...................... 251 | | | | | | 25·3 22 3 | B. Follows a * 9 m. Good obs of place in a glimpse among clouds. | | 1330 | II. 37 | | 12 25 27·7 | 86 24 28 | p B; p L; g m b M; E in pos 30° n f to sp ................ 143 | | | | | | 29·4 24 30 | F; L; E; s b M; C ....................................... 238 | | 1331 | II. 67 | | 12 25 26± | 77 45 32 | R; s m b M; stellar 10...12"; has 2 st n p and one s f .... 3 | | | | | | 29·6 44 39 | F; S; R; ps b M ......................................... 243 | | | | | | 30·9 44 4 | F; v S; has a * 9 m about 30° foll ..................... 192 | | | | | | 32·4 45 26 | p B; R; pg b M; 20" .................................... 245 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1332 | Nova. | h m s | ° ′ ″ | 8 Canum. Not the least doubt of a considerable nebulous atmosphere round this star. | 151 | | | | 12 25 38·9 | 47 42 38 | | | | | | 39·2 | 43 31 | 8 Canum. Certainly misty though the twilight is strong. | 155 | | | | 40·1 | 42 37 | 8 Canum. Involved in a considerable nebula 3′ in diam, exactly R; v g b M. | 150 | | | | 41·5 | 41 41 | 8 Canum. Nebulous. (See the remarks on this phenomenon in the Appendix.) | 335 | | 1333 | II. 157 | 12 25 39·4 | 75 59 21 | p F; p L; R; v g b M; 80″ | 339 | | | | 39·8 | 59 24 | v F; p L; R; 50″ | 242 | | 1334 | II. 147 | 12 25 40·2 | 82 36 16 | Not v F; E; v g b M; r | 254 | | 1335 | II. 94 | 12 25 43·5 | 73 30 32 | F; R; b M; r | 27 | | | | 44·9 | 30 24 | p F | 422 | | 1336 | II. 410 | 12 25 44·5 | 53 31 33 | e F; E; hardly visible for haze | 72 | | | | 44·6 | 32 52 | v F; L; R; v g l b M; 45″ | 331 | | 1337 | V. 2 | 12 25 47·7 | 86 52 50 | p B; v L; m E in pos 20° n p; s b M | 141 | | 1338 | Nova. | 12 26 2·3 | 70 51 26 | p B; p m E | 334 | | 1339 | I. 160 | 12 26 40·3::| 92 51 9 | B; E 25° n f to s p; v s m b M to nucl; 60″ | 21 | | | | 42·9 | 51 21 | v B; m E; v s m b M to a r nucleus, 2′l, 90″ br | 147 | | | | 46·4 | 51 13 | v B; m E, in pos 5° s p to n f; s m b M to a nucleus | 146 | | | | 51·9:: | 51 0 | B; E, in pos 30° s p to n f; v s m b M to nucl 60″ | 20 | | 1340 | Nova. | 12 26 40·6 | 82 56 41 | p F; R; b M; 40″ | 117 | | 1341 | Nova. | 12 26 41·0 | 38 15 23 | e F; p L; R; 30″ | 328 | | 1342 | III. 493| 12 26 43± | 89 18 7:: | v F; R; g b M; 20″ | 145 | | 1343 | I. 36 | 12 26 50·5 | 76 50 17 | B; R | 22 | | | | 55·8 | 51 41 | p B; R; b M; 20″; the s p of 2; pos of the other from this by microm = 33″·5. | 245 | | | | ... | 50 32 | The first of 2 nebulae 3′ asunder; v F | 3 | | 1344 | III. 802| 12 26 50·6 | 30 9 7 | p F; p L; E; v g b M; precedes a * 9 m | 345 | | | | 53·9 | 9 42 | e F; a * follows 2′ dist | 323 | | 1345 | II. 120 | 12 26 51·8 | 74 33 45 | B; L; p m E; g b M | 419 | | | | 51·9 | 34 2 | p B; R; b M; 60″ | 24 | | | | 52·0 | 33 40 | B; R; p s l b M; 60″ | 422 | | 1346 | II. 850 | 12 26 52·2 | 25 32 6 | v F; L; wedge shaped, or has a v F * n f, which gives it a distorted appearance. | 411 | | 1347 | III. 807| 12 26 59·1::| 30 7 37:: | By long and careful attention I think I see III. 807. Place estimated from III. 802. | 345 | | | | 61·1 | 7 57 | e F; p L; sky not perfectly clear | 344 | | 1348 | M. 89 | 12 26 59·8:| 76 31 25 | B; S; R; m b M; 30″. (RA precarious by reason of a fluctuating zero.) | 19 | | | | 64·2 | 30 24 | B; R; g b M; 40...50″. (This RA to be preferred to the rest, which are very uncertain.) | 192 | | | | 29 3:: | | F; R; g b M; 25″; has a * n f; rough P D | 2 | | | | 31 32:: | | R; m b M; rough P D | 3 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1349 | I. 37 | 12 27 05' | 76 48 12" | F; R; 10° of time following I. 36 | 22 | | | | | | p B; R; b M; 25". The n f of 2; place by comparison with the preceding. | 245 | | 1350 | II. 343 | 12 27 14'4 | 62 32 17 | B; R; s m b M; 30" | 417 | | | | | | B; irreg R; v s m b M to a * 12 m | 343 | | 1351 | II. 380 | 12 27 20'9 | 62 9 10 | F | 68 | | | | | | No description | 65 | | 1352 | I. 92 | 12 27 28'0 | 61 6 6 | v B; v L; m E; 4' l, l' br; 2 or 3 stars near it. | 64 | | | | | | v B; v L; m E; pos 60° n p to s f; 3 st follow | 65 | | | | | | v L; g b M, but not to a nucleus; m E; has 3 stars s f. By a diagram, the southern end is broader than the northern, giving it a clubbed appearance. (See fig 83.) | 66 | | 1353 | I. 119 | 12 27 29± | 81 23 25 | B; L; R; g b M | 154 | | 1354 | Nova. | 12 27 30'9 | 62 6 10 | v F; the n f of 2, (the p is II. 380.); a third suspected | 68 | | 1355 | III. 407| 12 27 34'7 | 69 44 1 | No description | 61 | | | | | | p B; p L; R; b M; r | 63 | | 1356 | II. 68 | 12 27 50'4 | 77 37 7 | B; S; l E; p s m b M | 338 | | | | | | No description | 242 | | 1357 | V. 24 | 12 27 51'7 | 63 4 30 | v L; an immensely long ray; pos = 134° 6 by microm. (See fig 37.) Both Lord Adare and Mr. Hamilton, who viewed it with me, agreed that a feeble parallel band extends below the nucleus, as represented in a drawing made at the time, from which that of the engraved figure is (principally) taken. Has a * 10.11 m 45° n f, Δ R.A = 5° 0. (See fig 37.) | 407 | | | | | | v L; 15' long, pos = 136° 4 by microm; pos of a * 12 m from nucl = 43° 8. The nucleus = a * 10.11 m. | 417 | | | | | | An uncommonly long narrow ray; E a full diameter of the field = 15' long; 30" broad; s v m b M; pos by ext 45° n p to s f. | 58 | | | | | | B; enormously long and very narrow. Pos of the long axis = 137° 4 by microm, very exact. A full diam of field = 15' long, v s b M. I cannot divest myself of the idea of an appendage n of the nucleus running parallel to the lower edge, which seems more sharply cut than the upper. A fine object, but not very bright. | 343 | | 1358 | Nova. | 12 27 54'8 | 77 47 35 | The n p of a fine double nebula; both F; R; g b M; pos 70° n p to s f; dist 1'. | 191 | | | | | | A curious bicentral nebula; both the component neb which run together are v F, v L, v g b M. | 338 | | | | | | v L; e F; like a v L double neb rubbed out; 4' diameter | 243 | | 1359 | Nova. | 12 27 56'3 | 77 48 35 | The s f of the double nebula | 191 | | 1360 | III. 880| 12 28 1'5 | 34 50 5 | p B; irreg R; g b M; 20". (Much out of place by working list.) | 347 | | 1361 | I. 32 | 12 28 13'2 | 81 49 9 | v B; m E; v s m b M, 2' long; pretty bright arms and a resolvable centre. | 117 | | | | | | v B; S; m E; v s m b M | 254 | | | | | | p B; s b M | 154 | | | | | | v B; S; E; p s b M | 251 | | | | | | v B; S; v m E; v s b M; 30" l | 250 | | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 1362 | III. 602 | h m s 12 28 28'4 | 7° 48' 12" | v F; p L; E; v g b M; attached like a tail to a star (place that of the *). (See fig 66.) | 24 | | 1363 | IV. 8 } 9 } | 12 28 32± | 77 52 10 { | A fine double nebula. Both P B; L; R; v g b M; 60'' and 45''; pos estimated from diagram = 315° ±. | 247 | | 1364 | III. 939 | 12 28 43'8 | 14 49 57 | e F; only to be seen with very long attention | 349 | | 1365 | II. 15 | 12 28 55'0 | 79 30 10 | B; R; s m b M to a nucleus; a * n p | 120 | | 1366 | Nova. | 12 28 55'5 | 79 35 26 | F; R; b M. Query, may not this be the same with II. 15, with a mistake of 5' in P D? | 19 | | 1367 | M. 91?? | 12 29 0± | 75 17 ± | A bright * 9 m, and 2 or 3 smaller; close by the B star and s p it, is a small well defined body which may be a close double star, and n p is also a F neb. The place set down is that of Messier's 91st neb, but I do not think this can be that object, whose existence even seems questionable. | 243 | | 1368 | M. 58 | 12 29 3'6:: | 77 14 56 | v B; irreg R; g b M; a B * precedes ½ field | 4 | | | | 5'4 | 14 54 | B; R; g b M | 22 | | | | 8'1 | 15 0 | v B; v L; E; v s v m b M; r; 5'1, 4' br | 247 | | | | ... | 16 ± | v B; L; R; place only rough, being observed past meridian | 242 | | 1369 | I. 124 | 12 29 8'9 | 83 42 0 | v F; L; R; v g b M; 2' diam | 253 | | 1370 | III. 495 | 12 29 44'5 | 55 36 36 | F; S; R; b M | 74 | | | | 46'8 | 36 3 | F; S; 1E | 131 | | 1371 | I. 125 | 12 29 46'4 | 84 44 45 | p B; E | 143 | | | | 47'3 | 44 45 | p B; p m E; p s b M | 141 | | 1372 | III. 504 | 12 30 35'2 | 83 2 34 | No description | 251 | | 1373 | II. 31 | 12 30 35'8 | 89 36 22 | e F; L; p m E; v g l b M | 145 | | 1374 | I. 273 | 12 30 40'2 | 14 52 17 | B; R; p g m b M | 349 | | | | 42'1 | 52 6 | B; R; p g m b M; 30''; a S * n p; dist 1' | 348 | | | | 44'4 | 53 1 | v B; R; p g m b M; 50'' | 382 | | | | 58'4 | 52 32 | v B; 1E; p g b M. The right ascension disagreeing so much with the rest, all the reductions have been carefully re-examined, but no error detected. Perhaps the moveable wire has been mistaken for one of the fixed ones in the obs of the transit, which will sometimes happen. (See Appendix.) | 413 | | 1375 | II. 183 | 12 30 53'5 | 94 24 36 | v s m b M, to a * 11.12 m, with a faint chevelure | 147 | | | | 54'6 | 24 21 | p B; E; s b M to nucleus | 234 | | 1376 | I. 43 | 12 31 10'9 | 100 40 19 | v B; v m E, in pos 2° n p to s f; v s m b M to a nucleus; 5'1, 30'' br, a B * s p. There is a faint diffused oval light all about it, and I am almost positive that there is a dark interval or stratum separating the nucleus and general mass of the nebula from the light above (s of) it. Surely no illusion. (See fig 50.) | 129 | | 1377 | II. 632 | 12 31 18'2 | 73 46 32 | v F | 24 | | | | 19'4 | 46 4 | No description | 422 | | | | 19'7 | 46 5 | p B; L; R; g b M; 40'' | 419 | | | | ... | 46 11 | p B; p L; R; g b M; 30'' | 421 | MDCCXXXIII. | No. | Synonym | RA 1830.0 | N.P.D. 1880.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1378 | I. 24 | h m s | 78° 53' 6" | B; R; g m b M; has 3 small st, f. | 4 | | | | | | B; R; b M; 30" | 19 | | | | | | B; S; R; p s b M; has 3 p B st f. | 191 | | | | | | B; has a * sf; Δ RA = 2° ± | 22 | | | | | | B; R; p s b M; 3 stars near | 120 | | 1379 | II. 577 | 12 31 41°7 | 85 56 38 | Followed by 2 st 8 m, (nisi RA = 12h 32m 12s·9) | 143 | | | | | | F; S; R; precedes 2 st 9 m (nisi RA = 12h 32m 13s·2 — the observations leaving an ambiguity as to the wire employed). | 141 | | 1380 | II. 184 | 12 31 53°9 | 94 11 56 | F; L; E; v g l b M; 50" | 234 | | 1381 | I. 254 | 12 32 22°1 | 27 26 55 | B; L; v m E, in pos = 118°·6 (microm); g l b M; 4'1, 1' br. | 344 | | 1382 | III. 43 | 12 32 22°2 | 77 9 19 | S; E; 1 or 2 stars near or in it | 192 | | | | | | v F; a curious object; 2 or 3 v F st form a line with an oblique ray of neb. | 245 | | | | | | v F; 2 or 3 v S stars in it | 3 | | 1383 | II. 69 | 12 32 38°4 | 78 54 20 | p B; R; p s b M; has * 12 m 1' n p, and a * 5.6 m in field n f | 120 | | | | | | Almost stellar | 22 | | 1384 | II. 20 | 12 32 49°4 | 81 45 1 | F; R; p s b M; has * 9 m 5° f. Twilight | 152 | | | | | | p B; S; R; p s b M; 20"; a * 8 m s f. | 117 | | | | | | v B; S; R; p g b M; a * 10 m 60" f | 250 | | | | | | Seen. P D roughly taken; no RA nor any description | 154 | | | | | | p B; R; b M; has a * f in parallel, ½ radius of neb from its edge. Rough P D. | 254 | | 1385 | I. 178 } | 12 33 19°9 | 47 54 52 { | Double; a B, L neb, g b M, with a large F one attached, 70° s f, so as to run together into one; C. | 248 | | | 179 } | | | F; L; dimly seen in twilight | 155 | | | | | | No description | 151 | | | | | | F; L; R; b M | 150 | | 1386 | M. 59 | 12 33 23°0:: | 77 25 28 | B; irreg R; r. | 19 | | | | | | F; R; g b M; 20"; has a * n p and one s p. Place very rudely ascertained. | 2 | | | | | | v B; S; l E; v s v m b M; 2'1, 1½ br | 338 | | | | | | v F; S; R; v g b M; 15" | 247 | | 1387 | Nova. | 12 33 25°7 | 76 7 15 | p B; R; has a * f Δ RA = 9°·0 | 337 | | 1388 | II. 411 | 12 33 27°1 | 53 60 25 | F; R; 15"; a * 9 m follows, pos = 301°·1; Δ RA = 8°·0 | 331 | | | | | | e F; has s f a * 8.9 m; pos 30° s f by diagram | 72 | | 1389 | II. 149 | 12 33 32°7 | 81 24 1 | p B; E; p s b M | 254 | | 1390 | Nova. | 12 33 35°5 | 86 0 26 | B; E. RA ill observed | 142 | | 1391 | II. 659 | 12 33 40°6 | 56 29 46 | a F neb n p V. 42, and almost close to it | 74 | | 1392 | II. 660 | 12 33 42°6 | 47 46 32 | F; S; R. | 150 | | | | | | No description | 151 | | 1393 | II. 772 | 12 33 45± | 96 8 ± | v F; R; has another nearly n; dist 5'. RA by working list. PD rough. | 147 | | 1394 | II. 773 | 12 33 47± | 96 3 ± | RA by working list. PD rough | 147 | | No. | Synonym | AR 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1395 | II. 532 | 12 33 50'0 | 85° 6' 30" | vF; vS; R .................. | 141 | | 1396 | I. 14 | 12 33 51'7 | 89° 9' 2" | eF; R; g b M. Sky not clear | 145 | | 1397 | V. 42 | 12 33 53'1 | 56° 31' 36" | v m E; a long ray which crosses the whole field, rather curved upwards (to s). Has a v F nucl and a B * nearly in the parallel. A F nebula II. 659 is very near it, n p. (See fig 76.) | 74 | | | | | 55° 0' | Enormously long, extending across the whole field (15'). Nucleus not well defined. Is preceded by a * 10 m, and that again by a S, F, R neb, forming a fine and very curious combination. | 131 | | 1398 | III. 603| 12 34 7'4 | 74 45 51 | vF; v m E; v g b M ........... | 421 | | | | | 7'8 | vF; L; mE; v g l b M .......... | 419 | | 1399 | II. 38 | 12 34 8'4 | 86 22 28 | B; R; b M; 30'' ................ | 143 | | | | | 10'2 | B; L; R; v g v m b M, but not to a nucleus | 238 | | 1400 | Nova. | 12 34 9'7 | 69 7 51 | vF; L; v g l b M; 2' diam ........ | 334 | | | | | 10'2 | eF; L; b M; 3' diam (an over-estimation) | 61 | | 1401 | Nova? | 12 34 10'2| 85 22 21 | vB; R; s m b M; 40''. If a mistake of 1° in P D be supposed in this obs, the place coincides with that of II. 38, and the descriptions agree. | 142 | | 1402 | II. 70? | 12 34 13± | 77 39 12 | F; R; g b M. My Father's P D is 77° 43', if this be the same object. | 3 | | 1403 | II. 125 | 12 34 18'8| 75 48 50 | B; E; has a * 12 m s f; 1' dist | 247 | | 1404 | I. 10 | 12 34 40'2| 87 4 53 | B; S; lE; p s b M ............. | 143 | | 1405 | III. 44 | 12 34 53'0| 77 28 ± | vF. The preceding of the fine double nebula M. 60 ........ | 22 | | | | | 53'3 | vF; p L; lE; the n p of 2 ...... | 191 | | | | | 53'9 | vF; E about 20 or 30° from n p to s f; it precedes M. 60 about 2½' | 19 | | | | | 58'5 | F; L; lE; 2' diam. The n p of 2 | 338 | | 1406 | Nova. | 12 34 53'3| 33 54 30 | eF; vS; R; g b M; 10'' ......... | 347 | | 1407 | II. 794 | 12 35 0'3 | 34 12 30 | Has 4 v S stars s p in a line | 347 | | 1408 | M. 60 | 12 35 2'3 | 77 31 18 | B; R; b M. The brighter of a fine pair, the other is v F; E 30° n p; 2½' dist. (See fig. 74.) | 19 | | | | | 3'1 | A double neb; a very fine and curious object. The p is v F the f v B; both large estimated dist of centres = 4'; pos 45° n p. | 22 | | | | | 3'9 | No description ................ | 4 | | | | | 4'1 | vB; R; has a v F oval neb n p; pos 30° n p, dist 3' by estim. | 191 | | | | | 6'5 | B; R; v s m b M; 90''; the s f of 2 | 338 | | | | | ... | A most curious double neb 3' dist centre from centre, but the nebula join with v F nebulosity. The fainter rather oval. | 3 | | 1409 | II. 12 | 12 35 10'7| 72 40 51 | vB; R; v g b M; r; 30'' ........ | 421 | | | | | 11'7 | Nearly R; g b M; r ............ | 27 | | | | | 13'8 | vB; L; E in parallel; g b M .... | 25 | | | | | ... | p B; E. No RA procured......... | 26 | | 1410 | I. 274 | 12 35 19'5| 14 38 32 | F; S; b M ...................... | 348 | | | | | 21'5 | pF; S; R; p g b M; 15'' ........ | 349 | | | | | 28'0 | pF; S; R; 15'' ................ | 382 | | | | | 32'4 | pF; S; R ...................... | 413 | | | | | ... | Follows a fine D * of contrasted colours | 170 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|--------------------------|-------| | 1411 | II. 126 | 12h 35m 22s.2 | 75° 56′ 44″ | vF; vL; 2′1,90″ br; 3 st near, 1 = 9 m | 192 | | | | | | vL; mE; 5′1. Closer examined, it is a double nebula? near several stars, one of which = 8 m. | 245 | | 1412 | II. 661 | 12h 35m 27s.3 | 48° 2′ 46″ | eF; near a *15 m | 335 | | | | | | eF; almost stellar; has *16 m f very near | 151 | | 1413 | Nova. | 12h 35m 27s.9 | 30° 6′ 26″ | not vF; pL; g b M. It is about 6′ dist n p two B st 8 and 10 m | 345 | | 1414 | I. 176 | 12h 35m 39s.3 | 56° 53′ 46″ | A long nebulous ray pos = 34°.3 (microm). Its southern half is fainter than its northern. It meets and cuts? another neb. A strange object. See fig 75. | 342 | | | | | | The p and s of two neb which run together, not very bright | 337 | | | | | | The s p of 2 which run together or are connected by a narrow curve. Shape just made out through cloud. | 341 | | | | | | A very extraordinary object. Two nuclei (each g b M) joined by a long curved neck or isthmus of nebula. | 74 | | | | | | Two extended nebulae crossing. They run together; the s p is vL; both p F. (N.B. in this obs they appear to have been well seen, and the nature of the object distinctly made out. A good diagram made.) | 131 | | 1415 | I. 177 | 12h 35m 47s.5 | 56° 51′ 29″ | The s p of two which cross; p F. (See fig 75.) | 341 | | | | | | The neb intersected by I. 176 | 342 | | | | | | The f of two which run together in a curve | 337 | | 1416 | II. 127 | 12h 35m 57s.3 | 75° 33′ 42″ | F; R; b M; 30″ | 24 | | 1417 | Nova. | 12h 35m 58s.6 | 77° 52′ 41″ | vB; S; vs vmb M almost to a * | 247 | | 1418 | II. 643 | 12h 36m 15s.6 | 51° 56′ 5″ | pB; pL; R; b M; 40″ | 73 | | 1419 | I. 142 | 12h 36m 26s.1 | 86° 1′ 59″ | B; not vL; vs b M; has a *10 m 45° sp dist 1′ | 141 | | | | | | pB; pL; R; g b M; 20″; has a *11 m pos 235°.5 | 238 | | 1420 | I. 15 | 12h 36m 26s.8 | 89° 31′ 37″ | pB; mE; psb M; pos 45° nf or s p | 145 | | 1421 | Nova. | 12h 36m 41s.6 | 77° 37′ 39″ | B; S; R; psb M; 15″ | 242 | | 1422 | III. 328| 12h 36m 53s.4 | 61° 56′ 31″ | F; vS; R | 64 | | | | | | B; S; R; b M; r | 66 | | | | | | pB; S; R; g b M. The first of 2 | 417 | | | | | | vS; smb M to a *10 m | 65 | | 1423 | II. 774 | 12h 36m 59s.5 | 96° 8′ 11″ | F; R; psb M | 147 | | 1424 | III. 329| 12h 37m 4s.3 | 62° 0′ 31″ | F; vS; R. There is evidently some error in this or the next RA, but it is probably this which is wrong, being observed at quitting the field, and the next being corroborated. | 64 | | | | | | pB; vS; the second of 2; Δ RA = 18°.0 | 417 | | | | | | vS; sb M = a *10 m; rough PD | 65 | | 1425 | II. 326 | 12h 37m 49s.9 | 58° 20′ 14″ | eF; query if not bicentral; sky perfectly clear | 341 | | 1426 | II. 181 | 12h 38m 33s.9 | 91° 48′ 17″ | B; not vL; p m E; p g b M | 146 | | 1427 | III. 398| 12h 38m 43s.3 | 69° 36′ 31″ | pB; S; resolved or resolvable. Has a * in centre | 61 | | | | | | S; stellar, or a * with a burr | 63 | | | | | | S; R; g b M; compact, almost stellar | 334 | | 1428 | II. 795 | 12h 38m 54s.8 | 34° 31′ 20″ | pB; p m E; vsb M | 347 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1429 | III. 543 | 12h 39m 11s | 84° 44' 11" | vF; follows a star | 142 | | | | | | eF; 10° following a * 9.10 m | 143 | | 1430 | Nova. | 12h 39m 12s | 53° 43' 2" | vF; R; p s b M; 15" | 331 | | 1431 | I. 128 | 12h 39m 13s | 75° 18' 46" | eF; vL; E; 4' l, 3' br | 338 | | | | | | pB; vL; E; v diffused | 242 | | | | | | pB; vL; E; vg lb M | 247 | | 1432 | II. 182 | 12h 39m 25s | 92° 23' 57" | B; p m E nearly in the parallel; g m b M; 90" l, 60" br | 146 | | 1433 | II. 381 | 12h 39m 28s | 61° 51' 4" | eF; hazy. RA imperfectly taken | 67 | | | | | | F; vS; R | 64 | | | | | | F; R; b M; (cloudy) | 66 | | 1434 | II. 72 | 22h 39m 39s | 78° 4' 20" | pB; R; g m b M | 4 | | | | | | F; S; R | 191 | | | | | | No description | 22 | | | | | | vF; R | 19 | | | | | | not vF; R | 120 | | | | | | pB; lE; p s b M | 245 | | 1435 | II. 796 | 12h 39m 47s | 34° 41' 30" | vF; R; vg lb M; 25" | 347 | | 1436 | I. 39 | 12h 39m 48s | 94° 52' 6" | vB; L; E; s m b M to nucleus | 147 | | | | | | vB; lE; g m b M; 40" l, 35" br | 234 | | 1437 | I. 129 | 12h 40m 14s | 97° 44' 25" | vB; R; v s m b M to a fine resolvable nucleus, 40". (Doubtless a globular cluster.) | 137 | | 1438 | III. 524| 12h 40m 15s | 100° 28' 6" | pB; m E 50° n f to s p; a B * precedes | 129 | | 1439 | II. 662 | 12h 40m 42s | 47° 8' 24" | F; R; g b M; sky perfectly clear | 151 | | | | | | vF; S; R | 150 | | 1440 | III. 610| 12h 40m 56s | 94° 16' 16" | vF; R. P D by MS 95°, but it was probably found by the working list, which makes its place 95° as from my Father's obs. | 147 | | 1441 | II. 95 | 12h 41m 8s | 73° 54' 22" | mE; 60"; a ray nebula 75° s p to n f; s b M to nucleus (by diag), a * f. | 27 | | | | | | vB; vm E; pos = 28°5 by microm; b M; 90" long | 421 | | 1442 | Nova. | 12h 41m 11s | 63° 35' 53" | vF; p L | 407 | | 1443 | II. 412 | 12h 41m 13s | 53° 44' 27" | pB; E | 131 | | | | | | Viewed; in field with a * 8 m; too F to take the place, owing to haze. | 72 | | 1444 | I. 140 | 12h 41m 19s | 83° 45' 26" | pB; L; lE; 60" l. 50" br; two st s f; 2' dist | 153 | | | | | | pB; R; glb M; 80" | 253 | | | | | | F; L; R; g b M | 152 | | | | | | pF; L; lE; vg lb M | 250 | | 1445 | III. 536| 12h 41m 26s | 102° 24' 47" | pF; p L | 351 | | | | | | pF; S; R; g b M; 12" | 352 | | 1446 | Nova. | 12h 41m 47s | 94° 21' 6" | eF; vS; between 2 st 5' asunder | 234 | | 1447 | III. 611| 12h 41m 53s | 93° 13' 19" | eF; b M | 21 | | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|----------|------------|---------------|-------------------------|--------| | 1448 | III. 424 | 12 41 55·9 | 55 54 45" | e F; easily mistaken for a * 15 m | 337 | | 1449 | III. 280 | 12 42 0·0 | 103 24 37 | F; R; the n p of two, 1' distant | 351 | | 1450 | II. 298 | 12 42 3·4 | 103 25 7 | F; R; the s f and brighter of 2 dist 1' | 351 | | 1451 | I. 84 | 12 42 3·6 | 63 34 23 | v B; v L; a v B nucleus in a wide, F, oval atmosphere, 4' l, 3' br | 407 | | 1452 | I. 41 | 12 42 12·5 | 95 28 16 | v F; p L; E; third class; sky perfectly clear and fine | 147 | | 1453 | II. 73 | 12 42 31·0 | 78 10 0 | e F; L | 19 | | | | 32·6 | 10 12 | p F; p L; irr R; b M; r | 4 | | | | 32·8 | 9 26 | F; R; has a * 12 m immediately p | 22 | | | | 34·7 | 9 24 | F; m E in parallel by diagram; has a * near the centre and another at the p end. (N.B. The MS makes the minute of RA 43; but it is possible, from the discrepancy of the descriptions, that it may be a different nebula, but this is unlikely.) | 192 | | | | ... | 10 32 | v F; E | 3 | | 1454 | Nova. | 12 42 33·7 | 84 13 25 | v F; v S; R | 141 | | 1455 | III. 515 | 12 42 47·5 | 97 29 20 | F; L; R; v g l b M | 137 | | 1456 | M. 94 | 12 42 51·9 | 47 57 2 | v B; L; v s m b M, almost up to a nipple-like nucleus. Not resolved, but strong twilight. (See fig 41.) | 155 | | | | 51·4 | 56 28 | B; L; R or l E; s m b M to nucleus 15" in diam and = a * 8 m, well defined, but not stellar. The nebula 2' diam. | 248 | | | | 52·0 | 56 26 | e B; R; v s v m b M to a nucleus = in its impression on the eye to a * 9 m, but which will not bear illuminating more than 11 m; diam of neb = 21/2. | 335 | | | | 52·2 | 56 42 | v B; R; p s v m b M, to a nipple; with 240, r; glimpses of stars seen. A fine object. 90" or 2' diam. | 150 | | | | 52·9 | 56 51 | The central B part (10" diam) equals a * 9 m, e compressed | 151 | | | | ... | ... | Viewed. v B; v s m b M; 4' diam. Not resolved but resolvable. (A very interesting object, being a neb v s m b M on a great scale.) | 73 | | 1457 | III. 496 | 12 42 52± | 54 55 25 | e F; RA from working list | 337 | | 1458 | III. 721 | 12 43 6·8 | 41 24 6 | v F; R; p s b M | 329 | | 1459 | III. 537 | 12 43 21·1 | 102 28 58 | p F; S; R; g b M; 12" | 352 | | 1460 | Nova. | 12 43 21·9 | 77 0 5 | p B; m E; r | 247 | | 1461 | I. 16 | 12 43 39·3 | 90 16 37 | B; R | 146 | | 1462 | I. 25 = II. 74 | 12 43 42·8 | 77 45 45 | R. (There is no doubt of the identity of the nebulæ I. 25 and II. 74.) | 191 | | | | 44± | 44 ± | F; R; g b M; 20". (Viewed.) | 2 | | | | 44·7 | 46 14 | B; R; p s b M | 192 | | | | 45·3 | 45 41 | v B; v L; p s b M; r; 2' or 3' diam. | 245 | | | | 45·6 | 45 34 | p B; R; p s b M; two small stars point to it | 243 | | 1463 | IV. 78 | 12 43 54·9 | 16 11 49 | p F; L; R; 40"; the central portion up to diam 30" is nearly uniform, so as to give it an approach to the appearance of a planetary nebula. | 382 | | 1464 | III. 281 | 12 44 1± | 104 29 ± | Seen in its place by working list. P D roughly taken. R A from list. | 351 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1465 | III. 70 | 12 44 16·2 | 73 13 36" | vF; mE | 421 | | | | | 16·3 | eF; pL; R | 419 | | | | | 16·4 | eF | 27 | | 1466 | II. 75 | 12 44 20·9 | 77 50 55 | pB; v m E in pos = 34°0 by microm. Remarkably situated under a canopy as it were of 3 bright stars. (See fig 84.) | 191 | | | | | 22·2: | 49 44: | | | | | | 23·4 | 51 14 | 243 | | | | | 24·9 | 51 24 | 192 | | | | | | 49 ± | | | 1467 | III. 544| 12 44 35·0| 84 37 10 | F; E; bM; 30" l; under 3 stars. Rough PD | 2 | | | | | | pB; S; R; g bM; 20" | 141 | | 1468 | II. 535 | 12 44 41·3| 87 48 37 | F; mE; follows a * 9 m in parallel; sky not quite clear | 145 | | 1469 | II. 24 | 12 44 49·7| 86 53 56 | B; s m bM; R; 1' diam | 142 | | | | | 51·7 | pB; R; g p m bM; 18"; Θ | 238 | | | | | | F; R; g bM; sky turbid; (rough PD) | 145 | | 1470 | II. 186 | 12 44 56·7| 95 41 46 | vF; L; R; 90"; vg1b M. Its companion looked for but not seen | 147 | | 1471 | III. 618| 12 45 0·6 | 52 15 17 | eF; S; R; bM. Sky perfectly clear | 331 | | 1472 | III. 106| 12 45 17·4| 79 22 1 | eF; pL | 19 | | | | | 17·6 | vF; R | 22 | | 1473 | II. 345 | 12 46 0·5 | 62 0 11 | F; R; 1's of a * 9 m | 64 | | | | | 2·1 | 0 9 | 67 | | | | | 3·7 | | 68 | | 1474 | II. 21 | 12 46 25·1| 81 1 4 | A neb attached to a B * 1' n, place that of the nebula | 117 | | | | | 29·4 | No P D taken nor any description | 152 | | | | | 30·2 | No description | 253 | | 1475 | I. 93 | 12 46 26·3| 60 8 1 | pB; R; p s bM. Among several stars | 65 | | | | | 27·0 | not vB; 1E; has * 8 m 1' dist 80° n f | 341 | | | | | | pB; S; E. Query if not bicentral. Near a * 9 m | 141 | | 1476 | III. 548| 12 46 36·2| 86 10 30 | F; S; close to a * | 343 | | 1477 | II. 382 | 12 46 38·7| 61 39 26 | pF; R; g bM | 417 | | | | | 39·4 | pB; R; g bM; 40". Minute mistaken, in RA; corrected by comparison with Sw 343 and working list. | 255 | | 1478 | I. 211 | 12 46 46·1| 42 33 19 | pB; R; 40"; has a * 15 m p | 140 | | | | | | B; R; p s bM; 30"; a * 13 m near n p. P D too roughly taken (being much past the meridian) to be of any use. | 347 | | 1479 | III. 816| 12 47 6·1 | 35 58 40 | eF | 142 | | 1480 | I. 141 | 12 47 22± | 84 47 .. | not B; E; g bM. Sky quite clear | 143 | | | | | | F; R; bM; sky perfectly clear | 64 | | 1481 | II. 383 | 12 47 42·2| 61 20 1 | S; R; bM; wind violent | 147 | | 1482 | II. 777 | 12 47 46·9| 95 53 41 | pB; S; R; g bM; 18" | 345 | | 1483 | I. 243 | 12 47 51·3| 30 44 27 | pB; L; 1E; vg bM; 90" l, 75" br | 323 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|-------------------------|-------| | 1484 | II. 549 | 12 48 0'0 | 97 36 47 | p B; p L; 1 E in merid; v g b M | 137 | | 1485 | II. 384 | 12 48 21'4 | 61 54 4 | v L | 67 | | 1486 | M. 64 | 12 48 21'5 | 67 24 0 | B; v L; v m E; v s m b M; well examined. I am much mistaken if the nucleus be not a double star, in the general direction of the nebula: 320 much increases this suspicion; 240 shows well a vacancy below (n of) the nucleus. The neb is 8' or 9' long, and 2' broad. | 424 | | | | | 22'4 | 23 10 | v L, oval neb, with a v S, s B, vivid nucleus. The neb is far feebler; 6'1, 4 or 5' br. I see no "dark recess" in it. | 409 | | | | | 26'1 | 23 17 | B; L; E, 5'1, 3' br; v s v m b M, almost to a *, but magnifying destroys this effect. Resolvable but not resolved. | 246 | | | | | | | Viewed, and the appearance of a vacancy below the nucleus verified. April 21, 1833, a careful drawing taken. (See fig 27.) | | | 1487 | II. 346 | 12 48 39'0:: | 62 4 46 | v F; p L; 35'' | 65 | | 1488 | III. 817 | 12 48 50'7 | 36 46 58 | e F; R; S; b M | 328 | | 1489 | Nova. | 12 49 1'6 | 40 16 26 | A rather doubtful object; haze | 329 | | 1490 | Nova. | 12 49 8'2 | 102 8 10 | v F; has 3 small stars s p | 352 | | 1491 | II. 536 | 12 49 10'7:: | 87 30 37 | F; p L; E; v g b M; has a * 30° n f | 145 | | 1492 | III. 613 | 12 49 14'9 | 92 41 40 | F; 1 E; has a * 30'' dist, 45° s f, 12 m | 146 | | 1493 | II. 387 | 12 49 17'9 | 60 36 22 | p B; R; a v S star makes it elongated | 417 | | | | | 18'7 | 36 8 | p F; double, n f, dist 20'' | 343 | | 1494 | II. 386 | 12 49 28± | 61 40 6:: | F; R; R.A by working list | 68 | | 1495 | Nova. | 12 49 44'3 | 51 42 17 | e F | 331 | | 1496 | II. 385 | 12 50 21'0 | 61 28 52 | p F; v S; R; s b M; 10'' | 417 | | | | | 21'8 | 28 26 | v F; R; p s l b M; 20'' | 343 | | 1497 | I. 68 | 12 50 25'3 | 104 7 47 | p B; R; s b M; 25'' | 351 | | | | | 25'3 | 7 33 | p B; R; p s b M; 20''; a * 13 m pos 140°; dist 1 diam by diag | 352 | | 1498 | I. 162 | 12 50 58'1 | 74 54 40 | B; E from s p to n f; s m b M; has a * involved, p its centre, in the parallel. | 23 | | | | | 58'3 | 54 40 | B; m E; s b M, to nucleus; has a S * n p | 419 | | | | | 58'5 | 54 12 | B; E in parallel; s b M to nucl; 2' 1, has a * in it 15 m, 10° n p the nucleus. | 24 | | | | | 58'7 | 54 41 | B; m E; s b M. The ray passes through a S * | 421 | | | | | 59'2 | 54 30 | p B; v m E; s b M; has a * or 2 14 m near | 247 | | | | | 60'4 | 55 4 | B; v m E in parallel; has * 12 m, 3°0 p, at the n edge of neb. | 338 | | 1499 | IV. 30 | 12 50 56'6 | 54 13 33 | F; S; R; much doubt as to nature of the object. Haze | 72 | | | | | 57'9 | 12 58 | An e F nebulous ray (pos about 30° by diag) connects 2 stars 10 and 12 m by obs. The minute of R A is 51, but this is probably a mistake in reading the chronometer. | 337 | | | | | 61'6:: | 17 ± | a v F neb; E n f to s p, between 2 stars, the southern of which is ill defined. Both seem to belong to the nebula. Place very ill determined, the P D especially being a mere estimation from a v distant *. (See fig 62.) | 131 | | 1500 | Nova. | 12 51 14± | 61 7 ± | The first of 5 south of a * 7 m. Place by configuration with the others. | 343 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1501 | II. 388 | 12 51 21'4 | 61° 8' 1" | F; S; R | 65 | | | | 23'5 | 8 31 | v F | 64 | | | | ... | 8 ± | The second of 5, south of *7 m | 343 | | 1502 | II. 389 | 12 51 33± | 61° 7 ± | The third of 5; place by configuration | 343 | | 1503 | III. 83 | 12 51 38'8 | 76 36 10 | F; v L; R; v g b M; 2' | 245 | | | | 39'7 | 36 54 | v F; p L; R; v g l b M | 192 | | 1504 | Nova. | 12 51 44'2 | 95 56 6 | v F; v S; E | 234 | | 1505 | II. 778 | 12 51 46'9 | 95° 9 16 | p F; v S; E; p s b M | 147 | | 1506 | III. 64 | 12 51 51'3 | 93 40 19 | v F; R; b M | 21 | | 1507 | II. 391 | 12 51 54'5:: | 61° 5 21 | No descrip. The RA very loosely determined | 64 | | | | 59'6:: | 5 58 | B; p m E; b M. The fourth of 5, s of *7 m | 343 | | 1508 | II. 390 | 12 52 1'1 | 62 11 19 | e F | 68 | | 1509 | I. 143 | 12 52 1'9 | 86 35 30 | A *10 m, has an oval neb attached, 45° n p. (See fig 67.) | 141 | | | | 2'4 | 35 18 | A *10.11 m, with an oval brush n p | 143 | | | | ... | 35 ± | A star 11 m, with a fan or brush | 142 | | 1510 | Nova. | 12 52 2'7: | 61° 8 1: | B; S; R; in parallel with another which it follows | 65 | | | | ... | 7 ± | The last of 5, south of a *7 m; more suspected to the south | 343 | | 1511 | I. 69 | 12 52 3'4 | 103 36 12 | p F; R; near some stars | 351 | | 1512 | Nova. | 12 52 13'5 | 41 52 6 | p F; S; R; 10''; g b M | 329 | | 1513 | IV. 47 | 12 52 39'9 | 93 37 39 | p B; R; g b M; nothing very remarkable | 21 | | | | ... | 39 ± | R; rough P D, taken past meridian | 147 | | 1514 | II. 645 | 12 52 45'3 | 51 44 .2 | e F; s f a *17 m, (1 radius from edge by diagram) | 331 | | | | 46'3 | 45 3 | p B; v S; s m b M | 73 | | 1515 | Nova. | 12 53 5'2: | 41 52 8 | e F; S; E; b M | 140 | | 1516 | II. 393 | 12 53 12'5 | 61 12 14 | F. There are several more in the neighbourhood | 67 | | | | ... | 11 52 | F; p L; 40'' | 417 | | 1517 | II. 300 | 12 53 15'9 | 104 3 37 | v F; R; b M | 351 | | | | 16'3 | 3 16 | v F; irreg R; v g l b M. (N.B. My Father has two observations of this nebula; both agree in making the PD 103°, but mine are both correctly reduced, and there is no appearance of any mistake.) | 352 | | 1518 | II. 394 | 12 53 16'0 | 61 15 .4 | v F; one of several. (N.B. One of these must have been II. 392, which is said to precede 393 and 394, dist 8'.) | 67 | | 1519 | II. 779 | 12 53 17'9: | 96 48 0 | v F; RA doubtful | 137 | | 1520 | I. 40 | 12 55 25'7 | 94 38 31 | p F; L; v g b M; E; 60''1 | 234 | | | | 26'5 | 38 51 | F; R; b M; sky very clear | 147 | | 1521 | Nova. | 12 55 28'9 | 37 45 38 | e F; R; p s b M | 328 | | 1522 | II. 395 | 12 55 39'4 | 60 54 0 | F; R; b M; has *9 m 45° n f; 1' dist | 68 | | 1523 | II. 188 | 12 56 17± | 95 35 36:: | v F; R; sky very clear. Wind. RA by working list; PD inaccurate. | 147 | MDCCXXXIII. 3 L | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1524 | II. 396 = III. 303 | 12h 56m 46.6s | 59° 57' 31" | vF; S; R. (N.B. The nebulæ II. 396 and III. 303 are no doubt identical.) | 64 | | | | | | vF; R; III. 303 looked for and suspected; minute in RA = 57 by obs; but this is an evident mistake. | 341 | | | | | | B; R; s m b M to a * = 11 m. | 65 | | | | | | pF; S; p s b M; 12" | 342 | | | | | | Barely visible in twilight. The RA very uncertain from fluctuating zero. (There is also an obs in Sw 341, which may perhaps refer to this nebula; but the minute is wrong, and it is described as "suspected" but not sure.) | 259 | | 1525 | II. 413 | 12h 57m 0.3s | 53° 54' 45" | pB; R; s b M; 25" | 337 | | | | | | pB; R; p s b M; 25" | 331 | | 1526 | II. 397 | 12h 57m 0.5s | 61° 31' 7" | F; R | 67 | | 1527 | Nova? | 12h 57m 30.1s | 13° 41' 13" | vF; S; R; g b M; 12". (The place is within barely possible limits of III. 937.) | 348 | | | | | | vF; R; v g b M | 349 | | 1528 | Nova. | 12h 57m 37.2s | 55° 54' 51" | eF; S; R | 74 | | | | | | eF. Seen in its place as determined by former sweep | 337 | | 1529 | II. 398 | 12h 57m 37.9s | 61° 21' 17" | F; irreg fig; b M | 68 | | 1530 | II. 663 | 12h 58m 3.4s | 47° 21' 22" | vF; R; S; 15" | 248 | | | | | | F; e S; stellar; 5"; has a v S * near it, to s | 151 | | 1531 | III. 304 | 12h 58m 7.4s | 60° 2' 22" | vF; R; g b M; near a double * | 417 | | | | | | F; lE; v g l b M; pos from the double * h 2626 = 34°.9 by microm. | 342 | | 1532 | III. 779 | 12h 58m 12.3s | 32° 46' 17" | vF; lE; pos from a * 7.8 m = 44°.0 | 343 | | 1533 | III. 783? | 12h 58m 17.8s | 35° 31' 0" | eF; S; lE; a sure obs | 345 | | | | | | Either a v F neb and star attached, or a nebulous double star, a doubtful object. The RA differs materially from that of my Father's III. 783. | 347 | | 1534 | Nova. | 12h 59m 3.8s | 94° 6' 21" | vF; vS; R; p s b M; 10" | 234 | | 1535 | Nova. | 12h 59m 28.6s | 70° 40' 16" | vS; R; s b M; stellar | 61 | | | | | | F; vS; R; p s b M | 334 | | 1536 | II. 301 | 12h 59m 57.9s | 104° 36' 32" | B; R; p s b M; 30" | 351 | | | | | | vB; R; p s b M; sky remarkably fine | 352 | | 1537 | II. 189 | 12h 59m 58.9s | 95° 51' 56" | F; p L; R; 50"; has * 9 m, 80" dist sf | 147 | | 1538 | III. 401 | 13h 0m 26.5s | 53° 53' 12" | eF; S; R | 331 | | | | | | F; S; R; b M | 131 | | 1539 | III. 654 | 13h 0m 28.1s | 47° 25' 18" | vF; vS; R; 10" | 151 | | 1540 | I. 42 | 13h 0m 30.4s | 96° 56' 0" | Not vF; R; v g b M; 40"; has a * 8 m, n.p. | 137 | | 1541 | Nova. | 13h 0m 36.5s | 77° 27' 22" | vF; S; lE; north of 2 small *s | 338 | | 1542 | Nova. | 13h 0m 36.7s | 37° 9' 13" | pF; S; R; 8...10" | 328 | | 1543 | II. 537 | 13h 1m 1.2s | 87° 25' 57" | eF; R; 1b M; sky not perfectly clear | 145 | | 1544 | II. 366 | 13h 1m 39.7s | 60° 11' 1" | F; lE | 65 | | No. | Synonym | AR 1830·0 | N.P.D. 1830·0 | Description and Remarks | Sweep. | |-----|---------|-----------|--------------|-------------------------|--------| | 1545 | Nova. | 13 2 20·9 | 35 34 50 | not v F; S; irr R; g b M ........................................... | 345 | | 1546 | III. 305 | 13 2 54·9 | 59 26 31 | e F; v S; R .............................................................. | 64 | | | | | 61·7:: | F; R; distinctly seen in twilight, but RA doubtful to the extent of 10°. | 259 | | 1547 | I. 96 | 13 3 5·0 | 52 1 24 | v B; v L; m E; 4'1, 1' br; v s b M to a nucleus, pos by diagram = 30° n f to s p. | 73 | | | | | 5·2 | v B; m E, in pos 20° n f to s p by diagram; s m b M; 2' long. | 72 | | 1548 | Nova. | 13 3 15·2 | 104 53 33 | v F; R; b M; a * 10 m 45° n p, dist 5' .................................. | 352 | | 1549 | I. 85 | 13 3 21·4 | 66 10 15 | v F; L; double or wedge-formed bicentral; pos 17° 0 per microm. Each neb v g l b M; a large * (the first of a trapez) 24s f. | 409 | | | | | 21·8 | not v B; E; g b M; 50''; has a * 9 m 23s foll, the first of a trapezium. | 424 | | 1550 | III. 820| 13 3 27·2 | 39 0 16 | e F; R; s p a * 15 m .................................................. | 329 | | 1551 | II. 414 | 13 3 38·6 | 52 49 7 | p B; S; p m E; p s b M ................................................ | 331 | | 1552 | II. 637 | 13 3 42± | 93 26 26:: | No description. RA by working list .................................... | 147 | | 1553 | III. 669| 13 3 52·8 | 105 51 16 | v F; R; b M .............................................................. | 354 | | 1554 | II. 746 | 13 3 54·6 | 108 36 28 | B; R; p g m b M; 30'' .................................................. | 355 | | 1555 | III. 545| 13 4 5·4 | 84 21 31 | e F; S; R ................................................................. | 142 | | 1556 | II. 129 | 13 4 12·4 | 76 29 54 | v F; R; p s l b M; 50'' ................................................ | 338 | | | | | 12·8 | L; R; straggling borders; p s m b M .................................. | 242 | | | | | 13·8 | F; p L; E; 30'' long .................................................. | 192 | | 1557 | Nova. | 13 4 26·3 | 42 54 25 | p F; R; 40''; has a * 12 m 1½ n f .................................... | 255 | | 1558 | M. 53 | 13 4 32·3 | 70 55 26 | A most beautiful highly compressed cluster. Stars very small, 12...20 m; with sc st to a considerable dist; irreg R, but not globular. Comes up to a blaze in the centre; indicating a round mass of pretty equable density. | 25 | | | | | 33·4 | extremely compressed. A most beautiful object ....................... | 26 | | | | | 33·5 | Seen by Mr. Baily. A fine compressed cluster, with curved appendages like the short claws of a crab running out from the main body. | 63 | | | | | 34·6 | A mass of close-wedged stars 5' in diam; a few = 12 m, the rest of the smallest size and innumerable. | 61 | | | | | 35·1 | Observed with Mr. Baily ............................................... | 62 | | | | | ............. | Viewed. A most beautiful cluster .................................... | 334 | | 1559 | II. 664 | 13 4 32·9 | 45 3 24 | F; m E; 70° n f to s p; 90'' l, 20'' br ................................ | 151 | | | | | 37·0 | F; a long ray 3'1, 20'' br; v l b M .................................. | 140 | | 1560 | III. 649| 13 4 48·5 | 57 17 49:: | Obs somewhat doubtful. The P D may err 2', as clouds prevented verification. | 341 | | | | | 46·0 | e F; R; has a * 14 m to n ............................................ | 74 | | | | | 46·5 | v F; E; S; 30'' s of a * 13 m ....................................... | 131 | | 1561 | Nova. | 13 4 45·6 | 83 1 58 | v F; R; g b M; 20'' .................................................. | 251 | | 1562 | Nova. | 13 5 7·7 | 42 1 3 | F; R; g b M; 15''; twilight .......................................... | 257 | | No. | Synonym | RA 1830.0 | N.P.D.1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1563 | III. 367 | 13h 5m 18s·1 | 61° 18′ ″1 | F; not v S; R | 65 | | | | 22°2:: | 17 48: | e F; irr R. Sky growing thick | 343 | | 1564 | I. 97 | 13 5 35·2 | 52 29 38 | B; p m E; s m b M; a * n p | 72 | | | | 37·6 | 30 32 | a v B nucleus with F branches, position = 166°·8 per microm. | 331 | | 1565 | II. 510 | 13 5 57·3 | 105 41 52 | p F; R; b M; 25″. A * 12 m l' n p | 354 | | | | 57·4: | 41 3: | No description | 157 | | 1566 | II. 511 | 13 6 21·4 | 105 29 15 | p F; p L; R; 30″ | 354 | | 1567 | Nova. | 13 7 34·9 | 59 24 9 | v F | 342 | | 1568 | II. 513 | 13 7 55·5 | 105 44 13 | v F; R; 20″ | 354 | | 1569 | VI. 7 | 13 8 2·4:: | 71 25 41 | v L; e F; a cluster of stars 19 or 20 m, with 4 or 5 = 15 m; irreg R; v g v l b M; diam at least 8 or 10′. A most curious and interesting object. The stars are just discernible. So faint, might easily be overlooked. RA of working list very much out, by reason of which the obs was nearly lost and quite spoiled. | 334 | | | | ... | 25 32 | v F; v L; 7′ diam; v S stars 15...20 m. Its true RA much precedes that in the working list. | 27 | | 1570 | M. 63 | 13 8 10·9 | 47 4 12 | B; p m E; v s m b M, almost to a * pos 30° n p to s f. Thes f end more diffused. Has a B * n p and a D * f. | 151 | | 1571 | III. 306 | 13 8 13·3 | 58 8 36 | F; S; R; b M. The first of 2 | 74 | | 1572 | III. 307 | 13 8 27·7 | 58 3 43 | F; S; R; b M. The second of 2 | 74 | | 1573 | III. 308 | 13 9 32·8 | 58 0 30 | v F | 342 | | 1574 | III. 282 | 13 10 19·4 | 103 57 22 | v F; p L; E | 351 | | 1575 | III. 309 | 13 10 31·6 | 57 37 45 | e F | 342 | | 1576 | III. 117 | 13 10 32·0 | 101 49 45 | v F; S; R; 15″; the s p of 3 | 352 | | 1577 | II. 193 | 13 10 34·5 | 101 45 2 | B; R; s b M; 20″; the northern and second of 3 | 352 | | 1578 | III. 118 | 13 10 41·1 | 101 48 12 | v F; p L; 1E; 40″; the f of 3 | 352 | | 1579 | II. 313 | 13 11 5·3 | 110 55 7 | B; R; p s b M; 35″ | 355 | | 1580 | II. 327 | 13 11 37·5 | 58 51 21 | p B; p L; g b M | 65 | | | | 39·7 | 52 45:: | No description | 259 | | 1581 | II. 539 | 13 11 46·9 | 103 11 22 | p F; S; R; g b M; 15″ | 351 | | 1582 | Nova. | 13 11 51·9 | 91 24 37:: | v F; R; g b M. It is 40° n f a * 11 m. | 146 | | 1583 | III. 633 | 13 11 59·0 | 48 41 53 | v F; R; b M; 12″ | 155 | | 1584 | III. 650 | 13 12 15·5 | 56 1 31 | F; S; R; b M; the s p of 2 | 74 | | | | ... | ... | Viewed. e F | 337 | | 1585 | Nova. | 13 12 23·2 | 55 58 1 | F; S; between 2 stars; the n f of 2 | 74 | | | | ... | 57 30 | e F | 337 | | 1586 | III. 619 | 13 13 44·6 | 50 32 54:: | v F; 1E; 30″1 | 155 | | 1587 | III. 119 | 13 13 57·4 | 102 5 12 | not v F; R. Nearly lost by looking too late, the RA of the working list being too great. | 351 | | | | 58·3 | 3 58 | F; R; g b M; 20″ | 352 | | 1588 | II. 826 | 13 14 3·4 | 31 27 32 | v F; p m E; 30″ | 345 | | 1589 | II. 646 | 13 14 16·9 | 50 22 1 | v F; L; R; v g l b M; 2′ | 73 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|--------------------------|-------| | 1590 | III. 368 | 13 14 52'9 | 62° 8' 22" | Not v F; p m E; l b M; 30'' l; pos 40° inclined to the parallel. | 417 | | | | | | Not v F; irreg fig; v g b M; sky rather dull. | 343 | | 1591 | III. 925 | 13 14 54'0 | 82 43 6 | F; R; g b M; 20''. | 152 | | | | | | F; R; g b M; 30''. PD only rough, being taken much past meridian. | 153 | | 1592 | Nova. | 13 14 54'2 | 60 47 11 | v F; L; makes an equilateral triangle with 2 stars 11 m, n p. | 65 | | 1593 | Nova. | 13 15 33'1 | 79 23 40 | Not v F; S; R; g b M | 120 | | 1594 | II. 666 | 13 15 40'4 | 46 1 16 | F; R; g b M; 35''. | 151 | | 1595 | II. 653 | 13 15 45'5 | 75 7 40 | F; R; g b M; 15''; a D * follows 7°5 | 420 | | | | | | p B; R; not v s b M; a coarse D * follows. | 338 | | 1596 | II. 328 | 13 15 50'2 | 57 32 38 | p B; R; g b M. No other near | 74 | | | | | | p B; R; follows a D * of the third or fourth class | 259 | | | | | | p B; p L; s f a small group of stars 13 m | 342 | | 1597 | II. 314 | 13 16 6'3 | 110 13 55 | F; p L; 1 E; v g b M. | 355 | | 1598 | III. 84 | 13 16 31'0 | 75 21 5'4 | e F; R; S; p s b M; 15''. | 192 | | | | | | Viewed; v F; R; b M; 15''. | 338 | | 1599 | III. 402| 13 17 7'2 | 52 43 37 | v F; R | 71 | | | | | | p F; R; v s m b M to a *. Has a * 12 m preceding. The s p of 2 nebulae. | 331 | | 1600 | III. 403| 13 17 17'7 | 52 40 1'1 | p B; R; the nf of 2 | 71 | | | | | | p F; R; v s b M to a * | 331 | | 1601 | II. 25 | 13 17 38'7 | 86 61 1 | F; 1 E; v s m b M to a * 12 m; 30''. | 145 | | | | | | B; R; p s b M; 30''. | 142 | | 1602 | II. 667 | 13 17 45'9 | 45 51 12 | Not v F; R; g b M | 151 | | 1603 | Nova. | 13 18 20'5 | 72 14 30 | v F; R; has a * 7 m, 6' north | 420 | | | | | | e F; S; R; has a B * n f | 27 | | 1604 | III. 404| 13 18 25'5 | 53 10 23 | p B; b M; the s p of 2 | 72 | | | | | | Not v F; E; g b M; 40''; the s p of 2. | 331 | | 1605 | III. 405| 13 18 45'5 | 53 7 38 | v F; the nf of 2. | 72 | | | | | | e F; L; R; it is 45° nf III. 404 | 331 | | 1606 | III. 651| 13 19 25'3 | 57 5 36 | e F; R; 30''. | 74 | | | | | | Not v F; p L; E; the p of 2, very similar | 337 | | | | | | F; R; b M | 131 | | 1607 | Nova. | 13 19 32'4 | 71 20 8 | v F; R | 26 | | 1608 | Nova. | 13 20 23'6 | 57 4 55 | Not v F; p L; E; the following of 2, very similar | 337 | | | | | | p F; R; b M; 30''. | 74 | | | | | | p F; E; l b M | 131 | | 1609 | III. 784| 13 20 27'3 | 33 37 40 | v F; R | 347 | | 1610 | V. 22 | 13 20 40'8 | 107 5 26 | F; v m E in pos 128°8 by microm; p g b M; 180'' l, 30'' br. | 354 | | | | | | F; L; E; v g b M; twilight | 157 | | No. | Synonym | RA 1880°0. | N.P.D. 1830°0. | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 1611 | III. 672 | 13 20 51·8 | 42 28 59 | v F; R; 50" | 255 | | 1612 | III. 45 | 13 20 59·4 | 78 6 44 | v F; two close together, or one E nearly in merid. A star 11 m n | 242 | | | III. 46 | 60·3 | 6 40 | e F; E; involves a * at the S end, and has a * 6 m, 15' s and a few seconds preceding. | 120 | | 1613 | Nova. | 13 21 0·0 | 72 3 45 | F; p L; R; p g b M; 40" | 420 | | | | 1·9 | 4 8 | F; p L; R; v g b M | 26 | | 1614 | Nova. | 13 21 11·3 | 42 31 49 | p F; R; v s b M; almost stellar | 255 | | | | 12·3 | 32 19 | p B; R | 256 | | 1615 | III. 70 | 13 21 9·4 | 72 17 37 | v F; has either a star excentric or a double nucleus | 27 | | | | ... | 17 35 | F; S; R; 15"; has a * 7 m nf, 8' dist. No R A procured | 420 | | 1616 | Nova. | 13 21 19·8 | 75 48 44 | e F; R; 20" | 338 | | | | 21·3 | 49 5 | F; R; S; 15" | 247 | | 1617 | II. 679 | 13 21 22·4 | 90 50 37 | F; 1E; g b M; 20"; the first of 2 | 146 | | 1618 | II. 680 | 13 21 27·4 | 90 46 42 | F; nearly R; g b M; 30"; the second and brighter of 2 | 146 | | 1619 | III. 642 | 13 21 40·7 | 75 42 19 | e F; R; 25". (Seen also in Sw 192.) | 338 | | 1620 | III. 652 | 13 21 58·0 | 57 59 17 | v F; R; g l b M; 15" | 342 | | | | ... | 59 16 | F; R; b M; much past merid, and no R A to be procured | 74 | | 1621 | Nova. | 13 22 22·8 | 70 59 21 | p F; R; g b M; 20"; a coarse triple * f | 334 | | | | 22·9 | 58 36 | v F; S; b M; has a considerable triple * following, dist = 8'. | 61 | | 1622 | M. 51 | 13 22 37·1 | 41 56 9 | A very bright round nucleus surrounded at a distance by a nebulous ring. (See fig 25, and the Note on this neb in the Appendix.) | 255 | | | | 38·5 | 56 13 | A most astonishing object, &c. (See Appendix as above.) | 140 | | | | 38·9 | 54 53 | A nucleus and double or divided ring, &c. &c. | 257 | | | | 40·0 | 55 36 | Place of the nucleus. The rings barely discernible for a haze | 329 | | | | 41·5 | ... | p B; E; v g b M; seen through cloud | 138 | | | | 43·8:: | 57 28::: | (See Appendix.) | 256 | | 1623 | I. 186 | 13 22 46·0 | 41 51 ± | B; R; v s b M to a *. This nebula is the companion of M. 51 and is figured with it. | 140 | | | | 47·0 | 51 16 | ... | 329 | | | | 50·0 | ... | ... | 138 | | | | 50·3 | 52 13 | ... | 256 | | 1624 | III. 406 | 13 22 58·8 | 54 17 45 | No description | 337 | | | | 60·5 | 16 37 | No description | 71 | | 1625 | IV. 63 | 13 23 4·3 | 30 42 12 | p B; irreg R; g b M; 90"; r; no nucleus seen | 345 | | 1626 | III. 643 | 13 23 53·5 | 75 13 34 | A F oval wisp attached to a * 11 m. | 192 | | 1627 | III. 9 | 13 23 55·4 | 81 48 17 | F; S; R | 253 | | | | 56·3 | 48 26 | F; S; R; p s b M; 10"; almost stellar | 152 | | | | 57·9 | 48 57 | F; R; like a * with a burr; the first of 2 | 250 | | | | ... | 48 ± | Seen in its place; p B. No R A observed | 251 | | 1628 | III. 10 | 13 24 12·1 | 81 47 37 | F; S; R | 253 | | | | 13·4 | 48 27 | F; R; s b M; 15"; like a burred *. The second of 2 | 250 | | No. | Synonym | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|---------|-------------|----------------|------------------------|-------| | 1629 | III. 99 | 13 24 18'1 | 81 56 57 | F; S; R; psbM; 15" | 153 | | | | | 58 ± | F; not vS; R; psbM. (Past merid.) | 152 | | 1630 | Nova. | 13 24 21'8 | 90 9 32 | pB; S; R; vsmbM; 20" | 145 | | 1631 | Nova. | 13 24 51'8 | 81 49 47 | eF | 253 | | 1632 | III. 656 | 13 25 26'0 | 47 15 18 | vF; R; g b M; 30...40" | 151 | | 1633 | III. 926 | 13 25 37'0 | 82 38 32 | A * 9 m with a F, very dilute nebulous atmosphere. (Possibly the minute of RA should be 26.) | 153 | | 1634 | Nova. | 13 25 51'1 | 71 16 8 | vF; S; R; bM | 26 | | 1635 | Nova. | 13 26 12'6 | 26 24 36 | R or lE; g b M | 411 | | 1636 | II. 841 | 13 26 19'1 | 26 21 26 | Not vF; pL; R; g b M; 35" | 411 | | 1637 | III. 86 | 13 26 35'9 | 75 17 31 | eF; R | 338 | | | | 36'4 | 19 35 | F; R; ps1bM; 25" | 247 | | 1638 | III. 85 | 13 26 36'2 | 75 23 4 | vF; S; R | 192 | | | | 36'4 | 22 38 | pB; S; R; sbM; 30" | 247 | | | | 37'3 | 23 29 | vF; R; vg1bM; 20" | 242 | | 1639 | III. 87 | 13 26 36'9 | 75 28 11 | vF; R; g1bM; 20" | 338 | | | | ... | 28 0 | vF; R; pL; RA not observed, but PD taken in time | 192 | | 1640 | III. 407 | 13 26 43'0 | 54 25 57 | F; S; R; has a * sp | 131 | | | | 45'4 | 25 18 | F; S; g b M; 15"; has * 10 m 30° sp, dist 40" | 72 | | | | 45'9 | 25 27 | F; R; bM. A star very near | 71 | | 1641 | III. 928 | 13 26 52± | 87 44 ± | vF; R; RA by working list; past merid. | 145 | | 1642 | III. 408 | 13 26 54'9 | 54 19 53 | F; S; R; g b M; 15" | 72 | | | | 55'9 | 20 17 | F; R | 71 | | 1643 | Nova. | 13 27 3'5 | 75 26 28 | F; L; E; vg b M; 50°l, 45" br | 247 | | 1644 | III. 100 | 13 27 26'0 | 82 31 2 | F; pL; R; very dilute; nfa * 9 m | 153 | | | | 28'2 | 32 34 | The faintest thing imaginable | 251 | | | | 30'2 | 33 1 | vF; S; R | 253 | | 1645 | III. 425 | 13 27 30'3 | 54 27 32 | F; S; R; has a vS * near | 131 | | 1646 | III. 101 | 13 27 57'9 | 81 45 29 | vF | 250 | | | | ... | 46 ± | vF; R; 25". No RA taken; past merid. | 153 | | 1647 | Nova. | 13 28 29'7 | 86 21 33 | eF; vL; fills the whole field. Strongly suspected; yet a doubt remains. | 143 | | 1648 | III. 620 | 13 28 44'2 | 50 46 26 | pF; E or obscurely bicentral; 1 b M, pos of elongation 25° nf by diagram. | 73 | | | | 45'7 | 47 49 | vF; pL; lE. PD probably erroneous from a shifting of the microscope. | 155 | | 1649 | II. 297 | 13 28 52'8 | 107 0 50 | vF; vL; psb to a brighter kind of nebula; a good type of its class. It loses itself quite imperceptibly. Diam of the faint neb = 2'; of the brighter part or nucl = 10 or 15". (See fig 39.) | 354 | | | | 53'5 | 0 48 | vF; pL; g b M; 40...50" | 157 | | 1650 | I. 34 | 13 29 5'5 | 80 14 18 | pB; vL; E, 60° np to sf; psbM; 3'1, 2' br | 120 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1651 | III. 72 | 13 29 20·6 | 73° 9′ 8″ | e F; S; R; b M; .................. | 26 | | | | | | p F; R; 25″ .................. | 420 | | | | | | v F; S; R .................. | 27 | | 1652 | III. 369 | 13 29 29·1 | 61 42 31 | v F; R; S .................. | 63 | | 1653 | III. 505 | 13 29 50± | 84 37 1 | F; R; b M; 30″. No RA taken, but inserted from working list | 142 | | | | | | e F; S; R; rough P.D. RA per working list | 143 | | 1654 | II. 895 | 13 31 13·7 | 88 17 43 | The first of 2 composing a double nebula; both v F; R; b M. The smaller of the two. | 145 | | 1655 | II. 896 | 13 31 18·2 | 88 18 3 | The second and largest of 2, composing a double nebula. | 145 | | 1656 | III. 673 | 13 31 18·9 | 40 50 23 | v F; R; v S; g b M; 10″; in field with a double star | 257 | | 1657 | Nova. | 13 31 40·3 | 84 4 4 | e F; among stars. Wind extremely troublesome | 251 | | | | | | v F; R; among some p B stars. (N.B. The RA of this obs to be preferred.) | 250 | | 1658 | III. 370 | 13 32 3·6 | 60 44 1 | p B; has a * 9 m 4′ dist; 45° s p | 65 | | 1659 | III. 410 | 13 32 38·6 | 52 16 7 | F; p L; r; has a * near | 71 | | | | | | F; S; irreg R; r | 72 | | 1660 | Nova. | 13 32 44·5 | 14 5 2 | e F; S; sky perfectly clear | 348 | | 1661 | Nova. | 13 33 13·4 | 50 21 6 | p F; R; 20″; has a small * p | 155 | | | | | | F; S; R; g b M; 20″ | 73 | | | | | | e F; R; has a * n p dist 3′ | 335 | | 1662 | Nova. | 13 33 34·7 | 84 52 35 | No description | 156 | | 1663 | M. 3 | 13 34 12·2 | 60 46 22 | e F; S; between 2 stars | 141 | | | | | | A most superb object, diam = 10°*0 of time in RA. Not less than 1000 stars 11 m and under. They run into a blaze at the centre, and form as it were radiating lines and pointed projections from the mass, with many stragglers. | 417 | | | | | | I just see the stars through a cloud so thick as almost to obscure Arcturus; 6′ diam, but in a clear night no doubt more. | 64 | | | | | | Observed with Capt. Smyth, who “saw something remarkable” in a small * 2m or 3m preceding it, which proved on closer examination to be a fine first class double *. | 415 | | | | | | Very beautiful; stars 11 . . . . 15 m; fills field, making lines and irregular rays of stars, and coming up to a blaze in the middle. | 65 | | | | | | A noble globular cluster 5 or 6′ diam, entirely resolved when not a star near it, even Arcturus, was visible to the naked eye for clouds. | 343 | | 1664 | I. 98 | 13 34 35·5 | 53 28 42 | B; R; first g and then p s b M; 50″ | 331 | | | | | | p B; R; g m b M; 50″ | 71 | | | | | | B; R; g m b M | 72 | | 1665 | II. 798 | 13 35 15·6 | 33 28 15 | v F; double neb; pos = 73°·0 by microm; a large star follows dist = 15′ ± | 347 | | | | | | v F; 1 E; s p a bright * | 346 | | 1666 | II. 668 | 13 37 52·5 | 47 38 28 | v F; v S; R; almost stellar | 151 | | 1667 | III. 785 | 13 38 50·1 | 33 51 20 | e F; hardly more than a violent suspicion, owing to auroral light in the sky. | 347 | | No. | Synonym | AR 1830·0 | N.P.D. 1830·0 | Description and Remarks | Sweep. | |-----|---------|-----------|--------------|------------------------|--------| | 1668 | I. 180 | 13 39 16·3 | 45 18 28" | Not vB; E 45° n p to s f by diagram; g b M .................. | 151 | | 1669 | II. 533 | 13 39 38·9 | 85 12 28 | vF; vL; 1E; v g b M; 2'1, 3' br. In the obs the minute of RA comes out 38 instead of 39, but this is an obvious mistake. | 143 | | | | | | vF; vL; R; v g l b M ........................................ | 141 | | 1670 | II. 688 | 13 40 ± | 43 0 23 | p F; R; m E .................................................... | 255 | | 1671 | II. 306 | 13 40 17·1 | 96 23 5 | e F; R ............................................................. | 137 | | 1672 | III. 681 | 13 40 21·8 | 50 51 15 | p B; S; has two nuclei or involves a double star .............. | 155 | | 1673 | III. 621 | 13 40 32·4 | 51 19 7 | e F; S; R .......................................................... | 331 | | | | | 33·2 | 20 39" | e F; a strong haze; PD uncertain ................................ | 28 | | 1674 | I. 255 | 13 41 19·9 | 28 9 57 | p B; S; m E in pos 57°4 by micr; p s b M; 30" 1 ........... | 344 | | 1675 | II. 710 | 13 41 39·5:: | 49 10 41 :: | e F; hardly visible for haze. The preceding of two in parallel. (N.B. As haze cleared, p B.) | 335 | | | | | 40·4 | 10 5 | F; v S; R; s b M ............................................... | 73 | | 1676 | III. 422 | 13 42 16·6 | 55 32 26 | v F; R ............................................................ | 74 | | | | | 18·4 | 32 0 | v F; the first of 3; pos with III. 423 = 241°·5 by micrometer | 337 | | 1677 | Nova. | 13 42 26·5:: | 49 10 41 :: | The f of 2 in parallel; p B; p L; 1E; g b M .................. | 335 | | | | | 29·5 | 10 42 | p B; S; E; 1b M; the f of 2 .................................. | 73 | | 1678 | Nova. | 13 42 37·8 | 84 9 30 | v F; v L; v g b M; R .......................................... | 141 | | 1679 | III. 423 | 13 43 2·4 | 55 27 5 | p B; S; R; p s b M; 15"; the second of 3 ..................... | 337 | | | | | ... | 28 ± | F; S; R ............................................................ | 131 | | 1680 | Nova. | 13 43 8·9 | 55 30 39 | e F; at first sight very like a *, but on long attention a p L neb surrounds it. Pos with III. 423 = 159°·5 by microm. | 337 | | | | | ... | 30 ± | p B; R; s m b M; taken much past meridian. No RA procured | 74 | | 1681 | II. 307 | 13 43 9·7 | 95 12 16 | F; L; R; g b M; 50 or 60" .................................... | 147 | | 1682 | II. 669 | 13 43 10·9 | 47 47 14 | F; R; g b M; 40" ............................................... | 151 | | 1683 | II. 685 | 13 43 19·4 | 91 21 34 | F; R; a * precedes .............................................. | 146 | | 1684 | I. 256 | 13 43 33·0 | 28 57 17 | v B; R; p s b M; 40" .......................................... | 344 | | 1685 | II. 712 | 13 43 33·8 | 49 35 14 | No description .................................................. | 156 | | | | | 34·8 | 35 47 | p B; S; 1E; s b M; 15" ....................................... | 155 | | | | | 39·8:: | 34 28 | F; R; p s b M; 30". Twilight and C; a very doubtful RA, and a presumed mistake of wires. If not, is a new neb. | 357 | | 1686 | III. 549 | 13 43 33·9 | 86 49 28 | p B; R; p s b M; 15" .......................................... | 143 | | 1687 | III. 929 | 13 43 36·8 | 87 3 17 | A very insignificant cluster of v S scattered stars; or a S resolved neb. | 144 | | | | | ... | 5 ± | The faintest thing imaginable; sky turbid. Not found till too late for the transit, and seen with difficulty. | 145 | | 1688 | Nova. | 13 44 18·6 | 86 20 1 | F; irreg R ....................................................... | 142 | | 1689 | II. 899 | 13 44 25·8 | 12 19 22 | e F; R; 15"; sky perfectly clear ................................ | 348 | | 1690 | II. 670 | 13 45 5·4 | 45 54 54 | v F; R; p s b M; 30" .......................................... | 151 | | 1691 | III. 698 | 13 45 9·2 | 49 28 40 | S; irreg R; has a B * 8 m, p .................................. | 155 | | 1692 | II. 308 | 13 45 16·1 | 96 45 15 | v F; S; R; b M. Dull and murky sky ................................ | 137 | | 1693 | II. 686 | 13 45 29·9 | 90 35 42 | p B; S; R; g b M; 15" ......................................... | 146 | | 1694 | III. 849 | 13 45 43·6 | 29 16 59 | e F. Sky nearly perfect ......................................... | 344 | MDCCCXXXIII. | No. | Synonym | R 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|----------|---------------|------------------------|-------| | 1695 | II. 424? | 13 45 47·1 | 55° 40′ 36″ | p B; L; R; 40″. If this be my Father's nebula, there is an error of 6′ in his P.D. | 74 | | 1696 | II. 713 | 13 46 7·3 | 48 48 34 | p B; R; b M | 156 | | | | 11·0 | 46 17 | v F; L; a bright D * p; the first of 4 | 357 | | | | 14·3:: | 49 ± | Place extremely vague | 155 | | 1697 | II. 697 | 13 46 8·6 | 51 15 7 | p B; L; 1E in parallel; v g b M; 90″ l | 331 | | | | 8·8 | 14 29 | v F; L; R; 1b M; 2′ | 73 | | 1698 | II. 714 | 13 46 10·8 | 48 53 29 | The southern of a double neb, dist 1′ in meridian | 156 | | | | 18·5:: | 51 ± | p B; S; the southern of 2 nearly in meridian; the second of a group of 4. Place very loosely taken. | 357 | | | | 20·3: | 57 ± | Place very loose, and P D especially so from fluctuating zero | 155 | | 1699 | II. 715 | 13 46 10·8 | 48 52 29 | The northern of a D neb, dist 1′ in merid | 156 | | | | 19·5:: | 50 ± | F; S; the northern and smallest of 2 in merid; one of a group of 4 | 357 | | | | 20·3: | 56 ± | Place very loose, and P D especially so | 155 | | 1700 | II. 415 | 13 46 13·4 | 53 1 12 | p F; R; 30″; has a * 90″ dist, 25° n f | 71 | | | | 14·1 | 1 8 | F; R; 1b M | 72 | | 1701 | III. 506 | 13 46 24·8 | 83 49 36 | e F, but the sky very dull | 142 | | | | 25·4 | 50 3 | e F; E | 143 | | | | 26·0 | 49 37 | p F; L; m E; r; 80″ l, 30″ br | 253 | | | | 26·3 | 49 29 | F; R; has two stars n and n f | 154 | | | | 27·0 | 49 7 | F; E; g b M; by diagram it is a narrow ray, pos 75° n f to s p | 153 | | 1702 | Nova. | 13 46 26·3:: | 48 49 ± | The last of a group of 4 | 155 | | | | 31·3 | 49 54 | F; the last of 4. There is a * 9 m preceding the group | 156 | | | | ... | 47 ± | v F; L; the last of 4. P D very rough | 357 | | 1703 | I. 6 | 13 47 33·1 | 83 54 41 | p B; R; p s b M; sky not clear | 142 | | | | 34·6 | 54 38 | v B; R; p s b M; 30″ | 143 | | | | 36·2 | 54 59 | B; R; p s b M; a * 8 m n f; 4′ dist | 427 | | | | 36·3 | 54 16 | p B; S; R; s b M; 25″ | 152 | | 1704 | III. 285 | 13 47 59·5: | 94 39 36: | v F; v S; R. Observed too late; place precarious | 147 | | 1705 | II. 534 | 13 48 2± | 84 10 ± | v F; R; p L; g b M; 50″. R A not observed, but set down from working list. | 143 | | | | ... | 8 54 | F; v L; R; v g b M; 2′ | 427 | | 1706 | III. 786 | 13 48 15·5 | 34 49 45 | p F; S; R; g b M; 15″ | 347 | | | | 21·0 | 49 40 | e F; R; s p a * 16 m; sky nearly pure | 346 | | 1707 | II. 716 | 13 48 30·9 | 48 40 47 | No description | 357 | | 1708 | II. 843 | 13 48 40·3 | 28 28 38 | No description | 344 | | 1709 | III. 809 | 13 48 47·7 | 30 30 42 | Not v F; S; E. I almost suspect it to be a double * 13 and 14 m involved in nebula. | 345 | | 1710 | II. 889 | 13 48 55·2 | 83 4 12 | p B; R; v g l b M; has a * 11 m, 5° n p | 253 | | | | 59·4 | 3 47 | F; S; 1E; v g b M; follows a * 4 sec | 154 | | | | 59·8 | 4 4 | F; L; R; follows a * 12 m (whose dist from edge of neb = 1 radius by diagram). | 251 | | | | 61·6 | 4 12 | v F; R; has a * 11 m p, 70″ dist | 250 | | No. | Synonym | RA 1830.0 | NP.D. 1830.0 | Description and Remarks | Sweep. | |-----|---------|-----------|--------------|------------------------|-------| | 1711 | III. 125 | 13 49 12.5 | 59 61 2 | pB; R; g b M; 45''. No other near in the parallel, following pB; pL; R; g b M; 40''. No other in the parallel before or after, for some distance. | 417 | | | | | | Not v F; R; p s l b M; 20''. If this be III. 125, my Father's place is much out in RA. | 342 | | 1712 | I. 187 | 13 49 25.2 | 41 56 32 | B; v m E; v s m b M | 258 | | | | | | B; L; m E; s m b M to nucleus | 256 | | | | | | pB; m E (40° n f to s p, by diagram); s b m to nucleus | 257 | | | | | | v B; m E; p s b M; 50'' l, 15'' br; pos = 40° 4 by microm | 140 | | 1713 | Nova. | 13 49 30.1 | 51 22 42 | pB; 1E; v g l b M | 255 | | 1714 | II. 698 | 13 49 38.1 | 51 33 37 | pB; R; p s b M; 40'' | 331 | | | | | | v F; S; R; r | 331 | | | | | | F; R | 28 | | 1715 | III. 546 | 13 49 45.7 | 82 54 42 | Like a * 15 m rubbed out | 73 | | | | | | A nebula like a hairy star | 153 | | 1716 | III. 547 | 13 49 52.7 | 82 49 32 | A neb like a double * obliterated; pos by diam = 55° or 60° | 250 | | | | | | Like a hairy star | 153 | | 1717 | I. 181 | 13 50 3.0 | 47 19 28 | Not v B; R; g b M; 40'' | 250 | | 1718 | Nova. | 13 50 15.4 | 48 43 46 | F; L; v g b M; has a * 9 m, n f, 4' dist | 151 | | 1719 | I. 240 | 13 50 31.0 | 29 24 36 | v F; sky not perfectly clear | 335 | | 1720 | III. 666 | 13 50 37.9 | 92 22 32 | F; S; R; g b M; 20'' | 344 | | 1721 | Nova. | 13 51 6.8 | 12 59 7 | A cluster of 11 stars 11 m, and 2 of 15 m | 146 | | 1722 | I. 191 | 13 51 17.4 | 51 44 ± | The smaller and n p of 2 which nearly join, constituting a double nebula. The place merely estimated by diag from I. 190. | 348 | | | | | | v F; S; the n p of 2 very near | 331 | | | | | | F; b M; E nearly in merid | 73 | | 1723 | I. 190 | 13 51 20.2 | 51 45 9 | The larger and s f of 2 which nearly join | 28 | | | | | | F; E; 1b M; by diag. The pos of the longer axis is about 60° n p and points towards I. 191, which it almost joins. | 331 | | | | | | v F; v S; p m E in parallel | 73 | | 1724 | III. 411 | 13 52 4.0 | 54 24 17 | e F; v S | 131 | | | | | | e F; v S | 71 | | 1725 | III. 412 | 13 52 22.0 | 52 55 18 | F; S; E; b M | 72 | | 1726 | III. 683 | 13 52 35.2 | 50 59 13 | e F; p L | 155 | | | | | | No descrip. RA hurriedly taken by comparison with a star in parallel and not to be depended on. | 331 | | 1727 | III. 810 | 13 52 43.6 | 29 19 50 | e F; e S | 344 | | 1728 | II. 699 | 13 53 7.4 | 50 14 57 | No description | 357 | | | | | | v F; S; R; b M | 156 | | 1729 | II. 672 | 13 53 45.1 | 48 10 50 | No description | 156 | | 1730 | III. 11 | 13 53 47.3 | 81 8 4 | v F; S; R; p s b M | 154 | | | | | | Not v F; S; R; p s b M; 12...15'' | 153 | | | | | | F; R; g b M. Follows several stars | 251 | | | | | | p F; R; p s b M | 250 | | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|----------|-------------|----------------|-------------------------|-------| | 1731 | Nova. | 13 53 50-7 | 81 29 37 | vF; R; bM; well seen | 253 | | 1732 | III. 684 | 13 53 58± | 50 0 31 | vF; vS; R; bM; among a cl of st 10 m. RA by working list | 73 | | 1733 | Nova. | 13 54 21-1 | 24 15 46 | pF; pS; R; ps1bM; 20''; has a * 7.8 m; ΔRA = 37s; ΔPD = 60'' ±. | 411 | | 1734 | II. 309 | 13 54 25-7 | 95 9 52 | The first of 2. Both L; F; vg bM; R; r; 3' dist; 70° np. The larger taken. | 147 | | 1735 | II. 310 | 13 54 29-7 | 95 12 41 | The second and larger of 2 | 147 | | 1736 | I. 230 | 13 54 38-6 | 34 0 30 | pB; mE; vsbM; 50''1 | 347 | | | | | 43-3 | pB; S; pmE; psbM | 346 | | 1737 | III. 653 | 13 55 6-8 | 56 40 17 | vF; S; E in merid | 131 | | | | | 8-0 | F; S; R; bM; 20'' | 74 | | 1738 | II. 827 | 13 55 15-7 | 29 49 50 | pF; R | 344 | | 1739 | II. 416 | 13 55 39-5 | 54 24 48 | F; S; R; bM; has a * 11 m sp 1' dist | 72 | | 1740 | Nova. | 13 56 ± | 54 31 57 | Taken for II. 416, which it cannot be if the last obs be correct. vF; S. | 131 | | 1741 | II. 417 | 13 56 0-7 | 54 3 15 | pB; R; sbM; 15'' | 337 | | | | | 1-8 | pB; R; vsmbM almost to a * | 28 | | | | | 3-0 | B; R | 71 | | 1742 | III. 413 | 13 56 7-7 | 54 9 50 | pF; near a * 13 m sp | 337 | | 1743 | II. 691 | 13 56 21-8 | 40 0 33 | pB; L; vmE; psmbM; 4'1, 20'' br; a ray with a nucleus. | 257 | | 1744 | M. 101 | 13 57 9-1 | 34 48 40 | F; vL; R; first g then vsmbM; 5' | 347 | | 1745 | III. 286 | 13 57 40-2 | 94 38 16 | vF; vL; R; gbM | 147 | | 1746 | VI. 9 | 13 57 46-4 | 60 39 44 | a L; v rich cl; 8'...10' diam; stars 12...18 m; roundish figure | 417 | | | | | 49-0 | Fine L cl; stars 14 m downwards to a nebulous appearance; 6'...8' diam. It will bear no illumination. | 65 | | | | | | Viewed; a fine L cl 7 or 8'; vg bM, but no nucleus. The stars 11 or 12 m down to an irresolvable mass; irreg R; excessively compressed. A fine object. Barely discernible in the 20 feet finder (2½' in aperture). | 357 | | 1747 | III. 947 | 13 57 51-1 | 10 57 7 | eF; pL; R; vgvlbM; 35''. RA precarious, owing to a great extra meridian correction. | 348 | | 1748 | I. 231 | 13 58 47-8 | 34 17 10 | pF; R; S; gbM; sky not quite clear | 346 | | 1749 | Nova. | 13 59 4-8 | 83 8 47 | F; mE; vglbM | 250 | | 1750 | II. 800 | 13 59 18-9 | 33 26 45 | pB; S; pmE; bM; 18''1, 12'' br | 347 | | 1751 | III. 287 | 13 59 21± | 95 17 ± | F; pL; R. RA by working list. PD roughly taken, past merid | 147 | | 1752 | II. 32 | 14 1 52-0 | 71 38 26 | pB; vS; has a vF double * in centre among several stars 12m; a doubtful object. | 334 | | | | | 39 ± | vF; S; R; sbM | 61 | | 1753 | II. 890 | 14 2 29-3 | 82 49 40 | pF; pL; gbM; 25'' | 154 | | | | | 30-0 | pF; S; R | 253 | | | | | 30-7 | No description | 250 | | | | | 52 ± | pB; bM; r. Viewed much past merid, and PD extremely vague. | 153 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1754 | II. 876 | 14 2 37·3 | 69° 35′ 11″ | pB; vS; E ......................... | 61 | | | | | | PD taken past meridian ............. | 334 | | 1755 | IV. 46 | 14 2 38·4 | 94 14 16 | pB; R; psmbM; 15″; seems to have *18m involved n.p. | 147 | | 1756 | Nova. | 14 3 41·8 | 87 56 32 | avF neb or avS cluster of eS st .... | 144 | | 1757 | II. 687 | 14 4 25·9 | 92 24 12 | vF; L; lE; gbM ...................... | 146 | | 1758 | IV. 49 | 14 4 32·7 | 92 20 57 | F; S; R; bM ....................... | 146 | | 1759 | II. 877 | 14 5 12·4 | 68 46 10 | pB; R ................................ | 409 | | 1760 | III. 685| 14 5 36·6 | 49 53 20 | F; S; lE; 15″ ...................... | 73 | | | | | | No description .................... | 357 | | 1761 | Nova. | 14 6 50·4 | 84 47 36 | F; irreg fig; seems to have a * in it | 155 | | 1762 | III. 134| 14 7 5·9 | 63 53 17 | F; S; R; bM; 15″ ................... | 143 | | | | | | eF; pL; a *10m 150″ dist n.p ...... | 261 | | | | | | pB; pL; mE; 2′l, 30″ br .......... | 425 | | | | | | pB; mE; 60″l, 20″br; a *10m p .... | 350 | | 1763 | III. 804| 14 8 20·5 | 31 25 57 | eF. Moon rising, but no doubt ...... | 345 | | 1764 | III. 414| 14 8 24·1 | 52 59 7 | pF; vme; a long narrow ray pos=110°3 by microm; vgvlbM; 90″l, 12″br. | 331 | | 1765 | III. 47 | 14 8 34·3 | 78 23 52 | F; R; gbM .......................... | 4 | | 1766 | II. 418 | 14 8 53·4 | 53 52 40 | pB; R; psbM ....................... | 337 | | | | | | R; vsmbM to 2 or 3 stars .......... | 28 | | | | | | No description. (An extraordinary disagreement in P D, yet none of the observations is marked as defective.) | 71 | | 1767 | Nova. | 14 9 14·7 | 81 1 47 | F; irreg fig; pL; gbM; r .......... | 253 | | 1768 | III. 731| 14 9 26·4 | 49 43 9 | F; R; the p of 2, or perhaps of 3 .. | 156 | | 1769 | III. 732| 14 9 34·1 | 49 36 56 | pF; S; R; gbM; 10″ ................ | 357 | | | | | | pB; R; perhaps a third neb near ... | 156 | | | | | | F; S; R; 15″ ...................... | 73 | | 1770 | III. 551| 14 9 44·5 | 81 38 30 | vF; vS; R; sky perfectly clear .... | 155 | | | | | | pB; R; bM; 20″ .................... | 154 | | | | | | pB; R; gbM; 20″ ................... | 250 | | 1771 | II. 419 | 14 9 52·4 | 52 38 15 | E .................................. | 69 | | | | | | F; S; a double nebula or two which run together pos 10°n f by diagram. | 72 | | | | | | F; E ................................ | 71 | | 1772 | III. 552| 14 10 14·5| 81 50 17 | F; R; bM; 20″; only one seen with much attention. Sky perfectly clear. | 153 | | 1773 | II. 194 | 14 10 16·0| 64 4 10 | vF; pL; R; vsmbM, to a *12m, for which it is easily taken. | 261 | | | | | | B; vsmbM; like a * with feeble atmosphere .......... | 425 | | 1774 | Nova. | 14 10 16·9| 76 19 29 | vF; pme; 30″l, 15″br. Just comes into the field with 18 Bootis. | 338 | | 1775 | Nova. | 14 10 51·9| 62 56 27 | vF; lE; 15″ ....................... | 350 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1776 | I. 99 | 14 11 17'0 | 52 42 34" | B; R; v s m b M to a *; v F at the borders | 28 | | | | | | v B; R; m b M | 69 | | 1777 | III. 347| 14 11 29'1| 64 24 20 | v F; R; b M | 425 | | 1778 | II. 579 | 14 11 29'5| 85 12 41 | p B; p L; 1 E; g b M | 142 | | | | | | v F; L; g l b M; 90" | 427 | | 1779 | I. 144 | 14 11 45'3| 85 17 7 | B; R; 40"; g b M; r; has a * 12 m 1 diam of neb (by diagram) dist, n.f. | 426 | | | | | | v B; p L; R; s b M | 142 | | | | | | B; R; p s b M; 18" | 427 | | 1780 | Nova. | 14 12 4'6 | 54 5 35 | p F; R | 337 | | 1781 | III. 12 | 14 12 14± | 81 42 ± | Not v F; S; R; b M. (RA by working list.) | 153 | | | | | | Seen; as also III. 551 in the same parallel, but considerably dist in RA. | 251 | | 1782 | I. 145 | 14 12 21'4| 85 58 33 | F; S; 1 E | 143 | | 1783 | I. 146 | 14 12 30'4| 85 56 48 | v B; R; v s m b M; a star 11 m n p and the neb I. 145 s p make a right-angled triangle with I. 146 at the right angle. | 143 | | 1784 | III. 415| 14 13 14'1| 54 1 47 | e F; L; 30 or 40" | 331 | | | | | | F; p L; the preceding of 2 | 72 | | 1785 | Nova. | 14 13 29'3| 54 0 33 | Not v F; 20"; the following of 2 | 72 | | 1786 | II. 754 | 14 13 48'2| 49 30 51 | B; R; p s m b M; 20" | 357 | | | | | | F; R; b M | 155 | | | | | | p B; S; R; s b M; 10" | 156 | | | | | | p B; R; g b M; 30"; has a * 11 m 50° s p, dist 80". No RA procured, and PD only rough. | 73 | | 1787 | III. 110| 14 14 3'9 | 75 18 20 | v F; R; g b M. Is n p a * 8 m 6' dist. | 338 | | 1788 | III. 416| 14 14 14'5| 53 57 14 | The n p of 2. Pos with the other = 330°-0 by micrometer. | 337 | | | | | | v F; S; R | 71 | | 1789 | Nova. | 14 14 14'7| 54 5 39 | e F | 28 | | 1790 | I. 235 | 14 14 20'8| 32 29 47 | v F; v L; R; v g b M; diam 2' at least; C and haze. | 345 | | 1791 | III. 417| 14 14 26'0| 54 1 20 | p B; R; p s b M; 15"; the sf of 2; C | 337 | | | | | | v F; a stellar nucleus. | 28 | | | | | | p F; R; 20" | 71 | | 1792 | III. 121| 14 14 53'8| 105 56 58 | F; v L; R; v g b M; 2' diam | 354 | | | | | | F; L; R; v g l b M; 60 or 80" diam; the first of 2; Δ RA = 15°. | 157 | | 1793 | III. 122| 14 15 7'8 | 105 59 13 | v F; L; 1 E; v g l b M; 90" | 354 | | | | | | v F; L; R; the second of 2; 60 or 80" diam; Δ RA = 15" | 157 | | 1794 | III. 927| 14 15 23'8| 82 38 32 | v F; E; g b M | 253 | | | | | | v F; R; b M; 12" | 154 | | | | | | p F; S; R | 250 | | | | | | No description | 153 | | 1795 | III. 418| 14 15 26'6| 52 6 7 | e F; S; R; (unless RA = 14° 15m 36s.6) | 331 | | No. | Synonym | RA 1880.0 | N.P.D. 1880.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1796 | III. 733 | 14 15 32'3 | 48 51 16:: | The places of this sweep are bad ........................................... | 155 | | | | 37'1 | 54 14 | F; R; b M; 12...15" .................................................................. | 156 | | 1797 | II. 177 | 14 15 41'8 | 74 35 7 | p B; R; g b M; 40" .................................................................... | 24 | | 1798 | III. 120 | 14 15 53'6 | 102 24 12 | v F ......................................................................................... | 351 | | 1799 | III. 688 | 14 15 54'9 | 92 25 57 | F; p L; v g b M to a stellar point ............................................. | 146 | | 1800 | III. 734 | 14 16 11'0 | 48 51 14:: | p B; R; b M; 15" ....................................................................... | 156 | | | | 13'1 | 49 44 | v F; R; g b M; 12" .................................................................... | 357 | | 1801 | III. 673 | 14 16 36'7 | 47 26 58 | F; R; p L; v g b M; 80". Sky very fine ...................................... | 151 | | 1802 | III. 136 | 14 16 42'2 | 64 37 5 | p F; p m E; g b M; 30"; a * 9 m follows 20s in the parallel ............ | 425 | | | | | 37 35 | v F; R; p g b M; 20" .................................................................. | 261 | | 1803 | Nova. | 14 16 49'3 | 56 10 46 | F; S; R; v s m b M .................................................................... | 74 | | 1804 | II. 420 | 14 16 54'2 | 54 21 47:: | p B; R; 30" .............................................................................. | 71 | | | | | 58'8 | p B; R; s b M; 30" .................................................................... | 72 | | 1805 | III. 419 | 14 17 16'4 | 52 45 52 | v F; S; 1E; v g b M .................................................................. | 331 | | 1806 | Nova. | 14 18 45'9 | 84 25 43 | v F; R; v g b M; 25" .................................................................. | 143 | | 1807 | III. 14 | 14 19 26'2 | 80 59 16 | The faintest possible .................................................................... | 250 | | 1808 | II. 329 | 14 19 55'9 | 55 59 1 | F; S; R; v s m b M; 15...20"; almost stellar ................................ | 74 | | 1809 | III. 677 | 14 19 58'6 | 40 40 37 | v F; p L; R; v g l b M; 30" .................................................... | 257 | | 1810 | Nova. | 14 20 13'4 | 49 16 48 | v F; S; R; g b M; 20" ................................................................ | 73 | | 1811 | Nova. | 14 20 20'4 | 77 51 2 | v F; R; 15"; about 3' f, and 40" n of a * 9 m ............................ | 338 | | 1312 | Nova. | 14 20 37'4 | 63 23 30 | p F; R; g b M; 20". Precedes Piazzi xiv. 97 ............................... | 350 | | | | | 40'7 | p F; R; has a * 7 m f ................................................................ | 425 | | 1813 | I. 70 | 14 20 40'5 | 95 12 19 | A fine small compressed globular cluster. I can barely discern the stars; they are 19 m 80" diam; has a * 7.8 m 90" dist, pos 30° s f, and another 10 m, n p. | 147 | | 1814 | II. 674? | 14 20 52'0 | 47 58 14 | No description ............................................................................ | 156 | | | | | 52'5 | F; E in parallel; 45" l, 30" br ............................................... | 151 | | | | | 53'5 | e F; S; R; sky perfectly clear ................................................ | 150 | | | | | 54'0 | F; p L; g b M; 35" .................................................................... | 155 | | 1815 | III. 132 | 14 21 1'1 | 61 49 51 | p B; S; E; s b M ....................................................................... | 65 | | 1816 | II. 580 | 14 21 4'0 | 85 57 51 | e F; R; the n p of 2 .................................................................. | 142 | | 1817 | II. 581 | 14 21 6'0 | 85 59 51 | v B; R; p s b M; 15...20" ....................................................... | 142 | | | | | 6'4 | p B; R; p s b M; 15...20" ....................................................... | 143 | | 1818 | I. 185 | 14 21 6'6 | 43 4 49 | B; R; v g l b M; 40" .................................................................. | 255 | | | | | 7'1 | Not v F; R; v g v l b M; 20" .................................................. | 256 | | 1819 | II. 357 | 14 21 11'0 | 66 3 0 | e F; v S; R ................................................................................. | 425 | | | | | 16'8 | e F; R; v g b M; 15" ................................................................ | 261 | | 1820 | I. 236 | 14 21 14'1 | 32 39 37 | B; R; p s b M; 30" .................................................................... | 345 | | | | | 14'3 | B; R; p s b M; 25" .................................................................... | 347 | | 1821 | Nova. | 14 21 23'3 | 58 50 12 | v F; R; n of a * 11 m; a * 7.8 m precedes .................................. | 258 | | 1822 | III. 126 | 14 21 51'0 | 59 12 57 | p B; v S; close to and n p a * 12 m; pos from *=333°5 by microm | 342 | | | | | 55'4:: | F; S; has a * in it and a B * foll it ....................................... | 65 | | No. | Synonym. | R 1830°-0. | N.P.D. 1830°-0. | Description and Remarks. | Sweep. | |-----|----------|------------|----------------|-------------------------|--------| | 1823 | II. 150 | 14 22 14·4 | 81 57 53 | v F; L; R; 60'' | 152 | | | | | 15·4 | 57 49 | p B; R; g b M. Wind very troublesome | 251 | | 1824 | III. 645 | 14 22 28·1 | 75 14 13 | The faintest perceivable; the first and northern of 2 | 338 | | 1825 | II. 891 | 14 22 33·9 | 83 15 27 | p B; p L; R; b M | 253 | | | | | 35·2 | 15 54 | p B; p L; R; b M | 153 | | 1826 | II. 330 | 14 22 50·3 | 58 1 38 | F; S; R; b M; 25'' | 74 | | 1827 | Nova. | 14 22 51·5: | 75 19 52: | The s f of 2; the faintest perceivable | 338 | | 1828 | III. 420 | 14 23 0·6 | 52 52 42 | p F; nucleus elongated, or has a F double * in it. Pos = 115°·5 ± (microm). | 331 | | 1829 | II. 421 | 14 23 18·5 | 53 55 20 | (II. 421, not III. 421.) p B; R; ps b M; 20''; a * 9 m follows 18°·5 nearly in parallel, and a * 14 m, pos 155°·0 from neb, dist 50''. | 337 | | | | | 18·9 | 55 0 | B; R; m b M; a star near or in it | 69 | | | | | 21·2 | 54 9 | F; R; r | 28 | | | | | ... | 55 12 | Seen. No description. Working list much out in P D | 71 | | 1830 | II. 892 | 14 23 30·4 | 82 59 57 | v F; p L; irr fig | 250 | | | | | 30·8 | 59 5 | v F (growing hazy) | 154 | | 1831 | III. 289 | 14 23 32·1:: | 63 51 5:: | e F. Place extremely precarious | 261 | | | | | ... | ... | Viewed; v F; R; v g b M. In or near its place per working list. | 425 | | 1832 | II. 695 | 14 23 49·6 | 39 37 45 | p F; v L; R; v g b M; 2'; r; stars = 20 m | 257 | | 1833 | II. 27 | 14 24 3·0 | 81 10 27 | p B; R; g b M; 30'' | 153 | | | | | 3·1 | 9 57 | p B; L; g b M; 90'' | 253 | | 1834 | Nova. | 14 24 52·2 | 78 43 32 | v F; R; 10''. Stellar; hardly distinguishable from a star | 4 | | 1835 | Nova. | 14 24 52·8 | 84 47 46 | v F; p L; R; has a * 15 m, n f, involved or very near | 142 | | | | | 52·9 | 48 0 | F; p L; R; has * 13 m, n f involved | 143 | | 1836 | III. 310 | 14 25 22·7 | 57 34 41 | v F; R; 1 b M | 74 | | | | | ... | 36 ± | Viewed. It is pointed to by a D * preceding | 258 | | 1837 | II. 893 | 14 25 23·2 | 83 47 2 | F; R; g b M | 253 | | | | | 23·8 | 47 7 | p B; p L; g b M | 250 | | | | | 24·0 | 46 59 | v F; R; b M; 20'' | 251 | | | | | 24·8 | 46 55 | v F; R; b M; growing hazy | 154 | | 1838 | II. 696 | 14 25 39·1 | 39 18 13 | v F; p m E; sf a star 15 m | 257 | | 1839 | II. 422 | 14 25 39·5 | 52 56 35 | F; S; E; b M | 72 | | 1840 | III. 289 | 14 26 34·9:: | 63 46 57 | F; R; r; has 3 stars 9.10 m n p | 350 | | 1841 | II. 894 | 14 26 37·1 | 83 52 39 | e F. Third class. Windy, but sky very clear | 251 | | | | | 41·0 | 53 17 | Just following a *. Cloud renders the observation doubtful. (N.B. The obs makes the P D 81°, but it is pretty evident that there is a mistake of 2° in reading the index, and that this belongs to II. 894.) | 153 | | | | | ... | 53 7 | v F; b M; some doubt if it be a nebula | 253 | | | | | ... | 53 17 | Among stars and seems attached to a * 12 m like a wisp | 250 | | | | | ... | 55 33 | e F; S; R. Taken beyond meridian, and probably a hurried observation. | 143 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 1842 | I. 189 | 14 26 48°0 | 39 47 15" | B; L; E; r; p g m b M | 257 | | 1843 | I. 237 | 14 26 58°5 | 31 19 44" | B; lE in merid; g m b M; 50" | 345 | | | | 71°1': | 21 13' | B; L; R; v g b M; 40". Noted in the MS. as a hasty observation, and with a doubtful RA caught in quitting the field. | 225 | | 1844 | III. 421 | 14 28 51°5 | 52 42 48" | F; S; R; b M | 72 | | | | 52°6 | 41 59" | F; R or lE | 28 | | | | 53°1 | 44 2" | p B; R. The preceding of 2 | 331 | | | | 54°6 | 43 17" | v F; E | 71 | | 1845 | Nova. | 14 29 5°1 | 52 45 12" | v F; S; R | 331 | | | | 5°5 | 45 3" | v F; v S. The following of 2 | 72 | | 1846 | III. 582 | 14 29 8°7 | 86 57 51" | e F; E; about 10° following a * 7 m | 142 | | | | ... | 58 12" | F; seems to be a double nebula (pos by diagram = 140° ±) foll a * 6 m. | 426 | | | | ... | 58 34" | a v Fray 60" l; follows a * 7 m dist 5' | 427 | | 1847 | II. 681 | 14 29 10°4 | 89 38 52" | p B; g b M; lE | 144 | | 1848 | I. 188 | 14 29 26°2 | 40 30 48" | B; S; p m E; p s b M; pos nearly in the parallel | 257 | | 1849 | II. 808 | 14 29 29°7 | 34 46 0" | F; irreg fig; r; has * 10 m, 2' s f | 347 | | 1850 | II. 648 | 14 29 59°± | 47 28 7" | F; R; r. RA by working list | 150 | | 1851 | II. 423 | 14 30 23°9 | 52 41 25" | p B; S; b M | 69 | | | | 25°4 | 41 38" | p B; R; b M | 72 | | | | ... | 41 57" | p F; R | 71 | | 1852 | II. 700 | 14 30 26°4 | 50 47 56" | F; S; irreg fig; b M | 73 | | | | 27°2 | 47 49" | No description | 156 | | | | ... | 48 27" | F; p L; lE; 40" l; in a scalene triangle of stars 10.11 m | 331 | | 1853 | II. 675 | 14 30 29°± | 47 38°± | v F; R; b M; follows an arc of 4 B st | 151 | | 1854 | II. 575 | 14 30 41°9 | 83 53 51" | B; R; p s b M; 30" | 143 | | | | 43°0 | 53 27" | p B; S; R; g b M; 25" | 253 | | | | 43°8 | 53 32" | p B; p s b M; 30" | 152 | | | | 44°3 | 53 13" | B; p S; R; b M; has * 11 m 15° prec | 154 | | 1855 | II. 649 | 14 31 16°1 | 48 44 41" | F; S; R | 155 | | | | 36°4 | 47 33°± | v F; p L; R; scarcely visible, for C. (N.B. The great difference of RA from that of the 155th sweep is probably owing to mistaking the moveable micrometer wire for the fixed wire of the eye-piece.—The P D of this obs is also evidently faulty.) | 357 | | 1856 | III. 895 | 14 31 27°4 | 69 13 11" | e F; S; v g b M; the p of 2; a double * between | 334 | | 1857 | I. 182 | 14 31 27°9 | 89 32 52" | B; R; p s b M; r; 20" | 144 | | 1858 | Nova. | 14 31 32°9 | 69 17 1" | e F; v S; the f of 2, close to a D * | 334 | | 1859 | Nova. | 14 31 34°8 | 48 49 14" | No description | 156 | | | | 36°6 | 48 42" | F; p L; E nearly in merid; g b M | 155 | | 1860 | III. 671 | 14 31 38°8 | 106 44 29" | e F; L; R; 60" | 354 | | | | 39°5 | 43 53" | v F; p L; very ill defined | 157 | MDCCCXXXIII. | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|----------|-------------|----------------|-------------------------|-------| | 1861 | Nova. | 14 31 57'5 | 42 36 39 | vF; E; 40''1; S of a coarse D *; the preceding of 2 | 255 | | 1862 | III. 550 | 14 32 9'2 | 85 48 33 | vF; R; vg1bM; has a * 9 m 45° nf | 143 | | 1863 | II. 682 | 14 32 12'8 | 89 34 35 | vF; s p a * 8 m, 1½ diam from edge of nebula | 426 | | 1864 | III. 675 | 14 32 20'4 | 42 35 ± | pB; S; 1E; bM | 144 | | 1865 | Nova. | 14 32 44'5 | 42 33 9 | The second of 3 in a line (two R; one m E) south of a double *. PD from Sw 255. | 256 | | 1866 | I. 184 | 14 32 58'3 | 106 31 5 | Not e F; R; psbM; 20''; the second of 3 | 255 | | 1867 | III. 657 | 14 33 33'5:: | 46 28 23:: | vF; R; psbM; 15''; the third of 3 in a line | 255 | | 1868 | III. 658 | 14 33 43'5 | 46 29 53 | F; R; pg bM; 20''; has a * 15 m nf; certainly not of first and hardly of second class. Sky perfectly clear. | 354 | | 1869 | III. 686 | 14 33 48'4 | 50 37 14 | pB; m E; bM, almost to nucleus; has a * 10 m 90° s | 157 | | 1870 | III. 133? | 14 35 11'2 | 60 33 1 | e F; p L; E; seen only with great attention. Place estimated from III. 658. | 151 | | 1871 | III. 896 | 14 35 19'6 | 70 23 21 | vF; S; R | 151 | | 1872 | II. 538 | 14 35 46'4 | 87 35 32 | No description | 156 | | 1873 | I. 171 | 14 36 3'7 | 47 26 42 | vF; S; R; bM | 73 | | 1874 | I. 126 | 14 36 17'6 | 87 19 17 | vF; L; R | 65 | | 1875 | I. 183 | 14 37 37± | 89 31 ± | vF; pS; R; g1bM | 334 | | 1876 | III. 690 | 14 38 13'3 | 108 22 6 | L; irreg R; gbM; r | 144 | | 1877 | II. 809 | 14 38 27'5 | 35 51 25 | pB; R; sbM; several small stars near | 150 | | 1878 | III. 687 | 14 38 35'4 | 50 32 57 | A long p B ray with a p B nucleus; 3' long | 144 | | 1879 | III. 885 | 14 39 50'0 | 70 46 56 | F; R; gbM; r; 30''; is not entitled to be called first class. Sky perfectly clear. | 144 | | 1880 | Nova. | 14 42 22'7 | 84 10 27 | F; S; R; gbM; 15'' | 355 | | 1881 | II. 576 | 14 44 43'2 | 85 20 21 | vF; 1E in parallel; vg1bM | 334 | | 1882 | III. 129 | 14 45 0'3 | 59 27 35 | vF; a double nebula, both individuals e F | 253 | | 1883 | Nova. | 14 45 7'2 | 48 42 4 | pB; R; sbM; 25'' | 143 | | 1884 | III. 130 | 14 45 17'8 | 59 30 25 | No description. RA lost | 142 | | 1885 | III. 554 | 14 45 28'6 | 85 46 18 | F; S; R; gbM; 15'' | 427 | | | | | | vF; S; R; pg bM; 15'' | 258 | | | | | | B; R; sbM; 15'' | 156 | | | | | | pB; pL; R; gbM; 20''; a * 8 m, np | 155 | | | | | | pF; 1E; psbM; 20'' | 357 | | | | | | vF; R; pg bM; 20'' | 258 | | | | | | Not vF; gvlbM; a narrow ray, 90'' l, 15'' br | 143 | | | | | | Not vF; m E; pos = 140°·0 ±; 90'' l | 427 | | | | | | vF; vm E; a ray, pos = 148°·4 by microm; 90'' l | 426 | | No. | Synonym | AR 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 1886 | Nova. | h m s | 14 47 11·9 | F; S; R; bM; has a * 16 m s p near | 354 | | 1887 | II. 676 | | 14 47 58·5 | S; R; almost stellar; s bM; 15" | 150 | | | | | 59·2 | pB; R; s m bM; 20" | 151 | | 1888 | II. 677 | | 14 48 55·6 | S; R; p s bM; 12"; like a burred star | 150 | | 1889 | III. 691| | 14 49 10·2 | pF; R; bM; 20" | 355 | | 1890 | III. 976| | 14 49 25·1 | eF; pL; 40...50" | 65 | | 1891 | Nova. | | 14 50 22·1 | pF; S; v s bM, to a * 13 m; the first of 3 in a line. A star 6.7 m near. | 257 | | 1892 | III. 131| | 14 50 32·3: | vF; R; v g l bM; 20"; has a * n f | 258 | | | | | 59 21 8: | eF | 65 | | 1893 | III. 679| | 14 50 47·1 | pF; S; v s bM to a * 13 m; the second of 3 in a line. A star 6.7 m near. | 257 | | 1894 | II. 539 | | 14 51 22·9 | B; s bM to nucleus; E pos 75° n p | 144 | | 1895 | III. 678| | 14 51 31·9 | pF; S; v s bM to a * 13 m. The third of 3 in a line; a * 6.7 m near. | 257 | | 1896 | I. 127 | | 14 52 34·3 | B; R; p s bM; 40" | 144 | | 1897 | Nova. | | 14 52 44·3 | vF; vS; R | 144 | | 1898 | II. 756 | | 14 53 36·5 | B; R; s bM; precedes a splendid D * | 347 | | 1899 | II. 539 | | 14 55 40± | No description. RA by working list | 144 | | 1900 | Nova? | | 14 55 56·6 | A very strongly suspected nebula; but I cannot be quite sure (from the low situation) it is not a star. | 353 | | 1901 | I. 128 | | 14 57 52·4 | B; R; p s bM to nucleus; 30" | 144 | | 1902 | II. 543 | | 14 58 31·4 | pF; S; lE; p s bM | 144 | | 1903 | II. 544 | | 14 59 12·2 | pB; R; p s l bM; among many stars | 426 | | | | | 13·7 | pB; S; R; g l bM; 12"; among stars | 427 | | | | | 14·4 | B; S; lE; p g bM | 143 | | 1904 | IV. 71 | | 14 59 52± | A star of fully 6 m, with a supposed nebulous appearance about it, but of whose reality I cannot satisfy myself, as it "blinks" with the star behind the wire. | 334 | | 1905 | II. 751 | | 15 0 0± | A double nebula; pos of the individuals, centre from centre, 20° n p; 2' dist. Both E; RA from working list; rough P.D. (See fig 77.) | 61 | | | II. 752 | | 69 48 ± | | | | 1906 | Nova. | | 15 0 23·3 | F; R; g bM; 20" | 150 | | | | | 24·4 | Not vF; S; R; p s bM; 15" | 151 | | 1907 | II. 585 | | 15 0 58·3 | pB; pL; R; g bM | 426 | | | | | 60·7 | pB; irreg R; g bM; 30" | 427 | | | | | 62·2 | pB; S; E; has a * 14 m closely f | 143 | | 1908 | II. 545 | | 15 1 9·3 | pB; S; E; p s bM | 144 | | 1909 | I. 219 | | 15 1 47·1 | vB; p m E; g bM; 50" l, 20" br; pos 326° 0 by microm. | 347 | | 1910 | II. 757 | | 15 5 23·0 | B; irr R with ray-like appendages; g b M; r; 30" | 225 | | 1911 | Nova. | | 15 6 32·4 | F; R; bM; 12" | 156 | | 1912 | II. 659 | | 15 6 52·7 | pB; R; bM; 15"; the P D differs 5' from my Father's. | 156 | | 1913 | II. 678 | | 15 7 24·5 | F; R; g bM; 30" | 150 | 3 n 2 | No. | Synonym | N.P.D. 18900. | RA 18300. | Description and Remarks | Sweep | |-----|---------|--------------|-----------|------------------------|-------| | 1914 | II. 650 | 15 8 55'4 | 47° 19' 58" | pB; p m E; p s b M | 151 | | | | 55'8 | 19 22 | v B; p L; p m E; g b M; r | 150 | | 1915 | III. 660 | 15 8 55'8 | 47 10 ± | F; R; g b M | 150 | | | | 60'3 | 10 8 | v F; 1 E; b M; small | 151 | | 1916 | M. 5 | 15 9 56'4 | 87 16 27 | A most magnificent, excessively compressed cluster of a globular character. Stars 11...15 m; diam in RA = 10 sec of time; the more condensed part projected on a loose irregular ground of stars. The condensation is progressive up to the centre, where the stars run together into a blaze, or like a snowball; the scattered stars occupy nearly the whole field. The neighbourhood is poor in stars. (See fig 87.) | 144 | | 1917 | II. 759 | 15 11 24'0 | 33 4 28 | p B; g b M; a ray 6' or 8' long at least; pos = 155°·0 by microm | 225 | | | | 26'2 | 2 20 | B; a superb ray nebula, at least 7½' long, and narrow; pos = 159°·9 by meas; at first v g b, then p s m b M. | 347 | | 1918 | III. 374 | 15 12 5'4 | 91 57 22 | v F; R; b M | 146 | | 1919 | I. 148 | 15 13 28'9 | 84 19 13 | B; R; p s b M; diffused at borders; many stars near. | 143 | | | | 29'6 | 18 12 | p B; E; p s b M; 90'' l, 40'' br; among many stars 11, 12, 13 m | 253 | | | | 30'7 | 19 37 | B; R; v s b M to a * 12 m; among stars | 427 | | | | 33'3 | 18 56 | p B; ill defined, roundish fig; g b M; among several stars | 152 | | 1920 | Nova. | 15 13 35'4 | 43 29 44 | p B; p m E; v g l b M; 60'' l, 40'' br | 255 | | | | 36'8 | 30 29 | v F; L; m E; v l b M; n of a D * | 256 | | 1921 | Nova. | 15 15 7'5 | 47 39 42 | v F; R; v g b M; 40'' | 150 | | | | 7'8 | 39 19 | No description | 156 | | | | 8'3 | 40 39 | e F; L; R; 60'' | 357 | | | | 10'3 | 40 8 | F; p L; 1 E; v g b M | 151 | | 1922 | III. 661 | 15 15 43± | 47 44 ± | No descr. RA by working list; PD rough | 151 | | 1923 | III. 874 | 15 18 18'9 | 71 19 7 | p B; S; R; p s b M; a * 7.8 m, 6' n | 334 | | 1924 | II. 651.1 | 15 20 1'5 | 47 44 4 | The s p of 2 very near constituting a double neb. The fainter and smaller. | 156 | | 1925 | II. 651.2 | 15 20 2'5 | 47 43 59 | The n f, larger and brighter of the double neb. Pos of the other 35° s p, dist about 15''. Not described as double by my Father. | 156 | | | | 3'5 | 43 57 | p B; b M; R; has a * excentric | 150 | | | | 5'6 | 43 28 | Not v F; S; bicentral; pos 45° s p ± | 357 | | | | 6'4 | 44 3 | F; R; b M; 30'' | 151 | | 1926 | II. 401 | 15 21 55'4 | 92 14 25 | p B; irreg fig; v g b M; 40'' | 246 | | 1927 | II.178 } | 15 26 38'9 | 74 14 42 { | A fine S double nebula; the individuals are F; R; s b M; r; dist = 1'. Both alike. | 24 | | | II.179 } | | | F; 1 E; g b M | 27 | | 1928 | II. 96 | 15 28 44'4 | 72 49 32 | v F; v L; R; v g b M; r; diam = 9s of time. With long attention it is seen to be composed of excessively minute stars like points rubbed out; and is in fact a globular cluster, but to see it thus requires long and perfect tranquillity of the eye. A very interesting object. (See fig 89.) | 253 | | 1929 | Nova. | 15 29 9'4 | 83 27 7 | F; S; R; g b M; 12''; 2 very L stars follow | 357 | | 1930 | III. 634 | 15 29 41'7 | 49 39 52 | e F; S; R; two *s 8 m, n f, dist 5' | 73 | | No. | Synonym | R 1830-0. | N.P.D. 1830-0. | Description and Remarks | Sweep. | |-----|---------|-----------|----------------|------------------------|-------| | 1931 | II. 762 | 15 30 9± | 32 44 53 | F; L; R; 40''; taken much past merid and P D only rough. RA per working list. | 225 | | 1932 | Nova. | 15 32 13·6 | 57 40 33 | v F; S; R; b M; 12'' | 74 | | 1933 | II. 655 | 15 33 37·5 | 73 39 42 | v F; R | 24 | | 1934 | II. 764 | 15 35 42·2 | 30 6 3 | B; R; p s b M; r; 25'' | 225 | | 1935 | II. 425 | 15 37 43·6 | 87 2 54 | v F; v S; R; 10'' | 427 | | | | | 48·0 | 3 27 | F; R; g b M; 20'' | 144 | | 1936 | III. 635 | 15 38 25·3 | 48 21 6 | F; R; b M | 155 | | | | | 28·3 | 20 44 | No description | 156 | | 1937 | III. 636 | 15 38 29·9 | 48 20 21 | p B; R; b M | 155 | | 1938 | II. 97 | 15 39 17·6 | 71 34 49 | p B; R; p s b M; 20'' | 334 | | | | | 19·3 | 34 34 | p F; R; g b M; 30''; between two coarse double stars | 262 | | 1939 | II. 583 | 15 45 39·4 | 88 56 27 | p B; S; l E in parallel; g b M | 144 | | 1940 | Nova. | 15 47 35·3 | 83 34 7 | p B; p L; E; 30'' 1, 18'' br | 253 | | 1941 | Nova. | 15 48 47·2 | 83 29 57 | S; R; nearly stellar; but about 10'' at the centre has nearly a uniform light, and a burr surrounds it. | 253 | | | | | 55·2 | 30 44 | p F; v S; R; much condensed in the centre. A disc with a burred border. Almost a planetary neb. | 153 | | 1942 | III. 646 | 15 49 43·2 | 73 37 22 | e F; v S | 27 | | 1943 | III. 73 | 15 49 46·2 | 73 32 22: | e F; v S; in the same field with III. 646 | 27 | | 1944 | III. 622 | 15 56 28·7 | 52 10 30 | Not v F; R; S; has * 12 m 40'' dist and 30° sf | 72 | | | | | 29·1 | 10 27 | e F; S; R; has * 10 m 40° sf | 71 | | | | | ... | 11 ± | e F; R. P D a mere guess | 28 | | 1945 | Nova? | 15 57 22·9 | 81 26 22 | A * 7 m which I strongly incline to think has a nebulous atmosphere about 2' diam. | 253 | | 1946 | III. 637 | 15 58 34·2 | 48 51 4 | p B; v S; R; b M; 6''...8'' diam | 156 | | | | | 35·6 | 50 40 | p B; v S; R; almost stellar or p s b M; diam 10'' | 155 | | 1947 | III. 553 | 16 1 17·4 | 88 50 12 | F; L; p m E; v g b M; 2½ 1 | 144 | | 1948 | III. 74 | 16 2 44± | 72 51 2 | e F | 27 | | 1949 | III. 889 | 16 6 9·6 | 56 30 56 | v F; S; R; b M | 74 | | 1950 | III. 888 | 16 9 7·8 | 57 36 35 | v F; v g l b M; 30...40'' | 258 | | | | | 9·7 | 36 21 | v F; S; R; b M | 74 | | 1951 | III. 688 | 16 10 15·1 | 53 52 33 | No description | 72 | | | | | 16·3 | 50 59 | v F; S; R | 28 | | 1952 | II. 151 | 16 10 31·5 | 82 10 35 | F; p L; l E; v g b M; 50'' 1, 40'' br | 153 | | 1953 | II. 402 | 16 12 58·4 | 91 52 32 | e F; v L; oval; 3' 1, 2' br; cloudy; 3m preceding nearly in the parallel is a fine double star. | 146 | | 1954 | Nova. | 16 13 39·9 | 51 48 33 | v F; e S; R | 72 | | 1955 | III. 623 | 16 13 46·1 | 51 49 14 | v F; v S | 73 | | | | | 46·9 | 50 13 | F; S; R | 72 | | | | | ... | 50 ± | Has a coarse double * 10° n f, 2' dist (past merid. No R A observed, and P D rough). | 71 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|------------|---------------|------------------------|-------| | 1956 | III. 624 | 16h 16m 58s.5 | 51° 40' 19" | v F; irreg R; r | 28 | | | | | | F; S; R; b M | 73 | | 1957 | Nova. | 16h 19m 20s.5 | 48 40 29 | F; R; b M; sky very clear | 155 | | 1958 | III. 638 | 16h 19m 25s.8 | 48 42 49 | No description | 156 | | | | | | p B; R; b M; 20" | 155 | | 1959 | III. 639 | 16h 20m 9s.6 | 49 8 53 | F; S; R | 73 | | 1960 | II. 652 | 16h 22m 0s.1 | 48 40 28 | v F; irreg R; among stars | 155 | | | | | | p B; p L; R; g b M; 40" | 357 | | 1961 | II. 875 | 16h 22m 48s.8 | 50 4 26 | F; S; R | 73 | | 1962 | III. 640 | 16h 23m 57s.9 | 48 48 29 | No description | 156 | | | | | | p B; S; R; b M; 12" | 155 | | | | | | Probably a mistake of 5s in reading the chronometer in one or other obs. | | | 1963 | III. 641 | 16h 24m 18s.4 | 48 59 57 | F; v S; R | 73 | | | | | | Rough P.D. Past merid | 155 | | 1964 | III. 890 | 16h 24m 21s.0 | 54 33 57 | F; irreg fig; r; 2 or 3 of its stars seen, also one 13 m 30" dist n.f. RA reduction fluctuating and uncertain in this sweep. | 71 | | | | | | v F; E; near a * | 72 | | 1965 | Nova. | 16h 27m 9s.3 | 54 17 48 | F; S; R; g b M; has a * 11 m 75° n p dist 40" (by diagram). | 72 | | 1966 | III. 893 | 16h 30m 41s.4 | 50 37 31 | v F; R; between 2 stars 14 m | 357 | | | | | | v F; S; between 2 stars | 73 | | | | | | Seen. Rough P.D. No transit | 155 | | 1967 | Nova. | 16h 31m 14s.3 | 53 27 38 | v F; v S; sm b M to a * 12 m; 12" | 72 | | 1968 | M. 13 | 16h 35m 35s.1 | 53 12 57 | Very rich cluster; irreg figure; v L; v g m b M; stars 10 ... 15 m, of which there must be thousands; does not come up to a nucleus; has hairy-looking curvilinear branches. (See fig 86.) | 71 | | | | | | Irreg R with scattered stars in streaky masses and lines. Excessively condensed, to a perfect blaze. *s 11 ... 20 m; 7' or 8' diameter. Most magnificent object. The state of compression indicates a globular form not much denser at the centre. | 28 | | | | | | A very fine and striking object, but nothing to add to the description of Sw 71. | 72 | | 1969 | II. 701 | 16h 37m 18s.± | 52 50 39 | No description; RA a mere guess | 28 | | 1970 | Σ. 5. N. | 16h 37m 18s.± | 65 53 ± | Struve's fifth nebula in the list at the end of the Dorpat Catal of D stars. v B equal to a star 8 or 8.9 m, 8" diameter, and of a uniform light, but with the edges boiling and ragged. A fine object like a star out of focus. Viewed between clouds, Struve's place. | 263 | | 1971 | M. 12 | 16h 38m 24s.8 | 91 38 22 | v rich globular cluster. The stars 10 ... 16 m; v g m b M, but has stragglers in lines and branches extending some distance from the most condensed part, which is 3' diam. Comes almost up to a blaze in the middle, and has a * 10.11 m in the centre. | 146 | | | | | | Irreg R; v L; 10' diam with stars from 10 to 20 m | 5 | | | | | | Viewed June 1, 1833. Very like M. 10, but the stars more separated and fewer. It is also rather larger. A fine object. Stars 10.11 ... 15 m. | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|----------|-----------|--------------|------------------------|-------| | 1972 | M. 10 | 16 48 10.8 | 93 50 ± | A globular cluster of scattered stars, but twilight and moon interfere. (P D from another sweep, not having been taken.) | 75 | | | | | | Is brighter than 12 M and rather larger and looser. (This disagrees with an obs of 12 M.) The bright part = 4', but the cl fills two thirds of the field = 10'. Stars 9...15 m. | 146 | | | | | | L; roundish; g p m b M; 10' stars 15...20 m ............... | 5 | | | | | | Viewed June 1, 1831. A superb cluster of very compressed stars, g b M. The stars are 10...15 m, and run up to a blaze in the centre, but I see no nucleus. Diam about 6'; a noble object. | | | 1973 | III. 689 | 16 48 44.0 | 53 13 47 | e F; v L; E in parallel; 2'1, 1' br ......................... | 71 | | 1974 | Nova? | 16 49 11.3 | 50 6 39 | A suspicious object. It is pointed to by a F double * n f. Doubtful whether a nebula or a v F double star, with perhaps a third star near (of course ill seen). | 357 | | 1975 | M. 19 | 16 52 6.9 | 116 0 0 | A fine globular cluster, stars v S, 12...18 m, with one =10m, and one 10.11 m; nearly R; v g p m b M, but does not come up to a blaze (i.e. to a confusion of the stars with one another). Insulated; 3' diam. It forms a link between 1. 70 and 10 or 12 M. | 148 | | | | | | Viewed July 1, 1823. F; R; g b M; r; fills ¼ field; one or two *s seen, but the twilight too strong. | | | 1976 | VI. 11 | 16 54 7.1 | 114 30 52 | B; L; b M; r; but too much twilight ......................... | 30 | | 1977 | VI. 12 | 16 59 35.7 | 116 20 10 | v B; R; p s b M; 90''; resolved; the stars are 19 or 20 m. This then is entitled to the name of a globular cluster. | 148 | | 1978 | Nova. | 16 59 42.7 | 116 20 5 | F; S; v s b M; is a companion to the globular cluster VI. 12. | 148 | | 1979 | M. 9 | 17 9 6± | 108 20 ± | R; v g l b M; 3 or 4' diam; v faintly seen in strong twilight. RA from Catal. P D very roughly determined. | 269 | | 1980 | II. 767 | 17 13 16.0 | 17 30 2 | v F; R; g b M; 25'' s f a small d * 2' dist .................. | 428 | | 1981 | IV. 11 | 17 18 59.8 | 113 36 9 | p B; R. Planetary? ............................................ | 30 | | | | 64.5:: | 35 39 | p B; R; 40''. Twilight ....................................... | 31 | | 1982 | I. 44 | 17 28 16.8 | 113 47 36 | A neb, with a p B star attached ................................ | 30 | | | | 20.5 | 47 31 | No description ............................................... | 31 | | 1983 | M. 14 | 17 28 42.3 | 93 8 25 | A globular cluster; v L; 8' or 10' diam; the stars so excessively minute as to be scarcely discernible. A striking object. Place probably very inaccurate. | 5 | | 1984 | Nova? | 17 36 55.3 | 114 48 59 | A cl of v S stars. Twilight .................................. | 30 | | 1985 | I. 150 | 17 38 45.5 | 110 17 33 | p B; R; g b M; 60''. Strong twilight .......................... | 269 | | | | | | Viewed; p B; p L; p s b M; 90''; easily found by the working list. | 268 | | 1986 | II. 586 | 17 39 7.5 | 109 57 55 | p B; p L; R; r; 40''.......................................... | 268 | | | | 8.5 | 56 38 | p B; R; g b M; 60''; a star 15 m n p .......................... | 269 | | 1987 | III. 741 | 17 39 43.9 | 17 48 32 | v F; v S; R; b M; 6''; 90'' n of * 8 m ....................... | 428 | | 1988 | Nova? | 17 42 25.6 | 115 20 54 | Suspected; small; twilight .................................. | 30 | | 1989 | Nova. | 17 44 42.5 | 66 52 41 | A S, R, very perceptible disc 1'' or 1½'' diam, with a v F nebula surrounding it—among many stars 12 and 14 m, none of which are so affected. A curious object. (See fig 42.) | 266 | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep. | |-----|----------|------------|---------------|-------------------------|--------| | 1990 | M. 23 | 17 46 41.8 | 108 61 45 | A v L, p rich, coarse, scattered cluster which fills the field. Stars 11 and 12 m. | 276 | | | | | | A star 10 m in centre of a beautiful discrete cluster of 60 or 70 stars 10 and 11 m and one of 9.10. They run in lines and arches. It is loose and straggling, and the sky around has a dotted appearance. | 269 | | | | | | A v large, coarse, straggly cluster of about 100 stars 9.10...13m. It is announced several minutes before by an increased number of stars in the field. | 33 | | 1991 | IV. 41 | 17 51 56.9 | 113 1 29 | The double star Sh 379 in the centre of the trifid nebula IV. 41. (See my 5th Cat of double stars. Mem. R.A.S. and fig 80.) | 275 | | | | | | A careful drawing taken, but the neb is not clear from twilight and clouds. (N.B. This drawing is unfortunately lost, and that engraved in fig 80 is constructed from much less elaborate sketches, aided by memory.) | 32 | | | | | | v L; trifid, three nebulae with a vacancy in the midst, in which is centrally situated the double star Sh 379, neb = 7' in extent. A most remarkable object. | 30 | | 1992 | Nova. | 17 54 3.6 | 78 56 57 | Seen in its place, but clouds prevented observation. | 31 | | 1993 | M. 21 | 17 54 25± | 112 30 2 | A coarse and poor cluster of L stars. | 196 | | 1994 | II. 197 | 17 56 51.5| 115 0 52 | A tolerably rich, sc, coarse cl; one * 9 m, the rest 10...12. | 275 | | 1995 | Nova. | 17 59 5.3 | 108 26 52 | F; L; 1E; b M; resolved. | 30 | | 1996 | Nova. | 17 59 33.3| 114 7 27 | A v coarse and scattered but p rich cluster of L and S stars. Has several double stars in it. | 268 | | 1997 | VIII. 54 | 18 0 40.4 | 106 49 7 | Several stars affected with nebulosity: the brightest taken... | 30 | | | | | | Large poor straggly cluster. No other near the place of VIII. 54. | 163 | | 1998 | VII. 30 | 18 2 32.3 | 111 36 10 | Very coarsely straggling and loose, hardly entitled to be called a cluster. The place (roughly taken) is that of 2 or 3 bright stars. | 36 | | 1999 | Nova? | 18 3 35± | 112 11 4 | A v L, v loose clus, pretty rich, fills the field; stars 11...13 m | 275 | | | | | | A cluster composed of 2 or 3 clusters of very small stars, and loose large ones. Perhaps this is an outlier of VII. 31. | 275 | | 2000 | Σ. Neb. 6| 18 3 50.4 | 83 10 57 | A beautiful round, perfectly well defined and brilliant disc, equalling a * 8.9 m. White equably bright. Well seen in broad morning twilight. A * 9.10 m follows, 2' dist. The sweeping power shows it as a * of large diameter, which could not escape examination in a good night; with 240 the disc seen as described. It cannot be more than 4" diam. | 153 | | | | | | B; R; 8" diam; rather hazy at the borders. It is something between a planetary neb and a B R neb. The light is pale and dull, but stellar, and equals a * 8.9 m. Two stars follow, the nearest distant in R.A 14°.5. A fine and curious object. On long and careful attention I cannot get rid of the hazy border and reduce it to a sharp round disc. | 279 | | | | | | Just caught in the evening twilight and shown to M. Struve the moment of his arrival at Slough, Aug 19, 1830, having travelled together from London. | 282 | | 2001 | VII. 31 | 18 5 37.1 | 112 10 26 | P rich; 3 or 4' diam; irreg fig; the stars v S. | 30 | | 2002 | Nova. | 18 7 1.3 | 109 55 12 | A double star in a faint neb. (See fig 30.) A very remarkable object. | 270 | | | | | | An oval nebula, involving a fine double star (No 2827 of my 5th Catalogue,) for which see further descriptions. | 269 | | | | | | A double * h. 2827 involved in a p B large nebula 50". See description of that *. | 268 | | No. | Synonym. | AR 1830-0. | N.P.D. 1830-0. | Description and Remarks. | Sweep. | |-----|----------|------------|----------------|-------------------------|--------| | 2003 | VIII. 55 | 18 7 44·0 | 106 41 50 | A cluster with a triple * in it | 274 | | 2004 | M. 24 | 18 8 27·5 | 108 28 13 | A glorious concentrated part of Milky Way, almost amounting to a globular cluster. Stars 14 and 15 m. | 269 | | | | 28·9 | 29 2 | Fine cluster of stars 15 m; R; 6'; the stars are all of a size. The cl seems connected with the Milky Way. | 270 | | 2005 | Nova. | 18 8 38·0 | 105 0 8 | Loose straggling cluster; stars 10..12 m | 34 | | 2006 | M. 16 | 18 9 15± | 103 50 34 | No description | 34 | | 2007 | M. 18 | 18 10 ± | 107 11 42 | A poor and coarse cluster. Contains about a dozen stars 10 m and 15 or 20 more 12..15 m. | 270 | | 2008 | M. 17 | 18 10 44·2 | 106 17 55 | The principal star in the preceding arc of the horse-shoe-like portion of the nebula M. 17. See fig 35. | 163 | | | | 46·8 | 14 5 | The small insulated, resolvable knot in the preceding, strait branch of the neb. | 274 | | | | 51·8 | 14 19 | The same knot. See description of this neb in the Appendix. See also the figure. | 358 | | | | ... | 15 48:: | A most curious object, not unlike the nebula in Orion (as it used to be figured, like a Greek capital omega, Ω.) There is in it a resolvable portion or knot distinctly separated from and insulated in the rest as if it had absorbed the nebula near it. (A figure carefully drawn.) (The P D inaccurate, being much past merid.) | 33 | | | | ... | 15 27:: | A large extended nebula. Its form is that of a Greek Ω with the left (or following) base-line turned upwards. The curved (or horse-shoe) part is very F, and has many stars in it. The preceding base-line hardly visible. The following, which is the principal branch, occupies nearly half the field (7½'). Its light is not equable, but blotty. Strong twilight. | 48 | | 2009 | Nova. | 18 13 40± | 102 6 42 | A loose straggling cluster of stars 11..12 m | 34 | | 2010 | M. 28 | 18 14 4·7 | 114 57 29 | Not v B; but v rich, excessively comp globular cl; stars 14..15 m; m b M; a fine object. | 30 | | 2011 | Nova. | 18 21 23·0 | 103 16 16 | A closely clustering portion of the Milky Way, which is one continuous cluster here. | 34 | | 2012 | II. 205 | 18 21 32·8 | 113 34 37 | p B; R; g b M; 40" | 30 | | | | 35·2 | 35 7 | A beautiful little globular cluster of excessively minute stars, 60" diam; seen in twilight. It must be p B when seen in dark night. (Sky very pure.) | 275 | | 2013 | VI. 23 | 18 22 47·2 | 107 0 11 | A rich, p comp cluster; irreg fig having a vacancy in the middle; stars = 11..15 m. | 36 | | 2014 | VIII. 14 | 18 23 20± | 107 27 11 | A very loose parcel of v small stars, hardly noticeable as a cluster | 36 | | 2015 | M. 22 | 18 25 59·1 | 114 1 16 | A magnificent globular cluster; g b M but not to a nucleus. The stars from 12 to 20 m. Those 12 m are equally scattered over it, but those of 20 m form the central mass. | 30 | | | | 61·2 | 1 11 | A superb, v m comp, R cluster. Stars 11..15 m; not very well defined. Rather more comp to the n f side than at centre; admirably seen in twilight. | 275 | | 2016 | Nova. | 18 26 50·6 | 66 33 38 | A v poor cluster 8th class | 266 | | 2017 | Nova. | 18 32 34·3 | 94 55 2 | A L p rich cl of straggling stars, having a vacancy in M and broken into 2 or 3 clusters. Fills field. 70 or 80 stars of all magnitudes from 10 to 18 counted. Extended, in parallel. The most comp part f. | 83 | MDCCCXXXIII. | No. | Synonym. | RA 1880.0 | N.P.D. 1880.0 | Description and Remarks | Sweep. | |-----|----------|------------|---------------|-------------------------|--------| | 2018 | Nova. | h m s 18 33 4·5 | 96 22 46 | A more than usually condensed portion of the enormous cluster of the Milky Way. The field has 200 or 300 stars in it at once. | 84 | | 2019 | M. 11 | 18 42 0·1 | 96 27 42 | A beautiful irregularly R cl 10' or 12' diam. The stars are all 11 m except one = 9 m whose place is taken. Examined with high magnifiers [I have often viewed it with 800 and even 1200]; it is broken into 5 or 6 distinct groups with rifts or cracks between them. | 82 | | 2020 | Nova. | 18 43 27·4 | 79 51 0 | A p considerable cl; 15' diam; irreg fig, 50 or 60 stars large and scattered. The place is that of the double * No. 870 of my third catalogue. | 88 | | 2021 | Nova. | 18 44 31·0 | 110 6 12 | A p rich cluster, figure like the letter S, 7' in extent. Stars 9...13 m. Counted 40 of them. | 268 | | 2022 | III. 143 | 18 44 50·3 | 112 54 20 | A little knot of 8 or 10 stars crowded together. It is 1' 40'' south of v² Sagittarii, and on same meridian. | 30 | | 2023 | M. 57 | 18 47 13·2 | 57 10 37 | The annular nebula in Lyra. The diameter of the ellipse in RA = 6°·5 : : It has a small star f exactly on the parallel of the centre, and distant from the edge rather more than the breadth of the ring. | 198 | | 2024 | Nova. | 18 49 ± | 79 51 30 | Annular neb between β and γ Lyrae. Pos of longer axis of annulus = 57°·0 by microm. The small * f is almost exactly on the parallel of the centre, dist about = breadth of ring. The central vacuity is not black; a nebulous light fills it. The edges are not sharply cut off, very slightly ill defined. See fig 29. | 197 | | 2025 | Nova. | 18 52 0·5 | 90 41 27 | RA not good, the sweeping zero having been interrupted by the disturbing effect of the side motion in viewing objects. | 199 | | 2026 | Nova. | 18 52 13·8 | 108 46 32 | No RA, very rough PD; viewed; diameter in RA = 5°·375 by a mean of 4 careful obs. The star following it = 11 m. It follows the centre 4°·31, and its pos from centre = 96°·4 by microm. The neb has a mottled look. [N.B. This mottled look, however, is something quite different from the appearance called resolvable.] | 168 | | 2027 | Nova. | 18 53 25·7 | 78 37 43 | A cluster discovered with the 7-feet equatorial, Sept 5, 1828. | — | | 2028 | Nova. | 18 54 47·7 | 60 58 3 | A p L, poor cl of stars forming irreg groups or patches, 11.12 m; diam = 8'. | 159 | | 2029 | Nova. | 18 56 25·5 | 88 27 44 | A cluster of loose small stars of various magnitudes; fills the field. | 78 | | 2030 | VII. 19 | 18 59 18·7 | 86 1 39 | A cl of small stars; fig irreg | 78 | | 2031 | | 21·7 | 0 53 | A v L, v rich cl, composed of 2 or 3 clustering groups running together; place that of the most condensed part. | 278 | | 2032 | | 22·8 | 3 22 | L, loose cl; fills field; the most condensed part is 3' in extent. Stars = 12..14 m. | 77 | | No. | Synonym. | RA 1830.0 | NP.D. 1830.0 | Description and Remarks | Sweep | |-----|----------|-----------|-------------|-------------------------|-------| | 2031 | VII. 62 | 19h 0m 16s·4 | 85° 35' ± | Pretty compressed cl; irreg fig, PD by the Sweep 77 being out of the limits of the sector. | 79 | | | | | 18°5 | Pretty rich; S; m compressed; oval or rather fan-shaped. The stars 11...12 m, 4' in extent; the n f side most comp. | 278 | | | | | ... | p comp; irreg fig; 2' diam; st 15 m. | 77 | | | | | | p comp; S; R or irreg; taken out of merid. | 78 | | 2032 | IV. 14 | 19h 5m 39s·1 | 92° 60' 9 | v F; R; v l b M; r; 30''. Nothing observed about it remarkable enough to entitle it to a place in class IV. | 82 | | | | | 42°3 | v F; L; R; v l b M; diam in RA = 4°5. | 83 | | 2033 | Nova. | 19h 6m 34s·7 | 85° 25' 8 | Coarse; not very rich; eighth class | 278 | | 2034 | Nova. | 19h 6m 55s·2 | 106° 33' 35 | A fine, L, loosely scattered cl of large with some small stars. Fills 2 or 3 fields. | 274 | | 2035 | Nova. | 19h 8m 5s·0 | 91° 12' 51 | A very large straggling space full of loose stars, 8, 9, and 10 m | 163 | | 2036 | M. 56 | 19h 9m 46s·± | 60° 6' 6 | A cluster; poor; loose; irreg fig; stars 10 and 11 m. | 81 | | | | | 52°1:: | A * 9 m precedes, about 1' diam. (The RA in these early sweeps is liable to great errors.) | 8 | | | | | 55°8 | Fine; v compressed; m b M; stars 11 m; a * 9 m precedes. Clouds interfered. | 197 | | | | | 56°6 | p rich; S; irreg R; g b M but not to a nucleus; 2½ to 3 diam; stars 13 and 14 m, well seen in full illumination of field. A few scattered stars. | 159 | | | | | 57°1 | L; R; v g b M. I see the stars which are v S and of different sizes. It fades gradually away at the borders. | 7 | | | | | 58°3 | No description | 199 | | | | | | Fine comp cluster; R, inclining to a triangular form; b M; stars 12...14 m. A fine object, diam 3'. | 198 | | 2037 | III. 743 | 19h 10m 9s·4 | 83° 45' 19 | A most beautiful, v L, F planetary nebula. Diameter in RA = 6°5 = 1° 37''. Its light nearly uniform, only very little hazy at the edge and perhaps rather brighter at the southern limb. Its nature seems to have been overlooked or mistaken by my Father, who has placed it in his third class. In Milky Way. Many stars in field, one 11 m near the n f limb. | 280 | | | | | ... | Pos of the small * near the edge, from the centre = 58°0 by microm. | 281 | | 2038 | Nova. | 19h 11m 50s·± | 91° 24' 34 | An e S stellar neb = a * 15 m; it is ¼ of a diam of field (=10') from a double star which it follows, to S. Pos from the star = 240° ±. The RA is excessively loose. | 5 | | 2039 | VIII. 81 | 19h 15m 56s·3 | 68° 9' 23 | Has a double star h. 886 in it | 267 | | | | | 56°9 | Coarse, poor cluster; stars 10...11 m. The southern of a group; is a first class double *. | 266 | | | | | 57°5 | Place that of a double * at the northern extremity of the more condensed part of a L, loose, poor cluster of st 10...15 m. | 90 | | 2040 | Nova. | 19h 17m 36s·7 | 86° 48' 13 | The first of 3 stars 9 m, nearly in the parallel, joined by a rich clustering portion of the Milky Way. | 278 | | 2041 | VIII. 21 | 19h 20m 7s·8 | 65° 11' 55 | v L; p rich; very straggling; stars 10 m; fills field. | 167 | | 2042 | VI. 14 | 19h 23m 10s·0 | 70° 5' 7 | A rectangular cluster, v m comp; 3' or 4', 2' br; stars 14...18 m; among B stars. | 364 | | | | | 10°2 | e F; p L; v g b M; 4', 2' br; composed of stars 17 or 18 m. | 362 | | | | | 12°6 | A curious object, 4', 1½', br, extended in merid. The largest st 16 m | 90 | 302 | No. | Synonym | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep | |-----|---------|-------------|---------------|--------------------------|-------| | 2043 | VI. 38 | 19 23 25·4 | 81 7 10 | A cluster. Has a * 16 m, one or two 18 m, and neb .......... | 89 | | | | | 26·1 7 17 | A very small compressed fan-shaped cluster of stars 11 ... 18 m, diam = 1'; a * 11 m on the n f side forms the vertex of the fan. | 280 | | | | | 26·6 7 22 | Doubtful if a resolved cl or a neb of first class. p L; R; b M; 60"; with 2 or 3 accidental stars of the Milky Way. | 88 | | | | | 28·5 7 22 | A v S roundish cluster, 40" diam, of v S stars, one brighter than the rest and = 15 m. It is like a nebula well resolved, and is a curious object. | 196 | | 2044 | Nova. | 19 32 21·0 | 43 64 41 | A double * in the southern part of a fine, large, pretty rich, coarse cluster of about 100 stars 11 .... 14 m; it fills the field. | 205 | | | | | 64·9 58 50 | The centre of the more condensed part of a considerable cluster, 10' diam, of irregularly scattered stars. | 206 | | 2045 | III. 744 | 19 33 21·0 | 100 42 35 | Not v F; p L; R; b M; r; 50" ......................... | 86 | | 2046 | Nova. | 19 33 53± | 63 35 ± | v L, p rich, straggling cluster; it more than fills the field. Stars 10 ... 15 m. | 167 | | 2047 | IV. 51 | 19 34 20·3 | 104 32 37 | Planetary nebula. B; R; equals a * 9 m in its light; diam = 10" by estimation. Perfectly round; there is no central vacuity (power 320). The light, though not hazy, is turbid, not like stars, but a kind of curdled appearance, very singular. Has two stars very near. The nearer, A, 15.16 m; pos 309°.5, 312°.8, 313°.0; the first measure taken with 320, and better than the others. The further, B, 15.16 m; pos 82°.1, 78°.0 (with 320). Dist of A 30", of B 50". (See fig 46.) | 365 | | | | | 21·3 33 29 | Exactly R; = * 8 m; disc = 10" or 12" in diam; has 2 stars 12 m near. Pos of A = 307°.0, of B = 81°.5. Central measures. Light equable, and disc very lucid, yet a little (not hazy, but) as if boiling at the edges, with a suspicion that it may not be well defined. | 163 | | | | | 22·7 32 54 | Exactly R; diam estimated at 8"; the light equable and equals a * 6.7 m. It is exactly like a planet and two satellites. Distance of A, the nearer, 20"; Pos 45° n p; of B, 25', 20° n f. | 34 | | 2048 | Nova. | 19 35 22·7 | 50 12 7 | A beautiful cluster, v rich, v L; stars 11 ... 15 m and 1 = 7 m n f, a reticulated mass, central part = 4', but fills field with its loose stars. A very fine object. | 359 | | 2049 | VII. 18 | 19 35 56·9 | 67 5 58 | p rich, irreg R; 5' diam; a cl of loose stars; the chief = 10 m, the rest = 11 ... 12. Four or five in centre form a lozenge. | 266 | | 2050 | IV. 73 | 19 40 18·8:: | 39 54 0 | A most curious object. (See fig 43.) A * 11 m surrounded with a v B, perfectly R planetary neb, of equal light throughout. Diameter in RA = 3s.5. Perhaps a very little hazy at the edges. With 320 the * is not seen double. | 207 | | 2051 | VIII. 73 | 19 42 2·6 | 82 30 40 | A * 8 m in a poor cl, hardly to be called a cluster. (Night very bad.) | 89 | | | | | 31 ± | Coarse; straggling; 15'; not remarkable; chief * = 9.10 m.. | 88 | | 2052 | VII. 9 | 19 43 47·2 | 67 20 14 | Fine large coarse cl; fills field. Stars 11 ... 12 m, some outliers = 9, 10 m. | 266 | | 2053 | Nova. | 19 45 11·5 | 31 0 24 | A * 7 m in midst of a field full of 40 stars 10 ... 12 m ...... | 366 | | 2054 | VIII. 16 | 19 45 21·6 | 61 1 38 | Coarse irreg R; with detached portions of smaller stars. Those in the main cluster = 11 or 12 m..................... | 7 | | 2055 | VIII. 18 | 19 45 28± | 78 45± | Viewed. In place by working list? It is a coarse straggling part of the Milky Way. | 196 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 2056 | M. 71 | 19 46 5·7 | 71 41 14' | v rich; m comp; g b M; an irreg R cl of v S stars, inclining to triangular form. In a rich part of Milky Way. | 360 | | | | | 8·0 | v L; loose; fills field; a fine object; stars 11...16 m; the most condensed part = 3', of an acute triangular figure, the angle northwards. | 90 | | | | | 12·1 | An irreg R mass of closely packed st; g b M; 3' or 4' diam; a decided cl; but towards the s p the Milky Way is immensely rich. | 364 | | 2057 | VI. 16 | 19 46 53± | 72 33 + | A quantity of Milky Way stars, immensely close, one small patch of which may be the cluster VI. 16. | 362 | | | | | | An insignificant bunch of little stars in the Milky Way. Hardly more marked than the general mass, which is astonishingly rich here. | 92 | | 2058 | VIII. 19| 19 47 17·0| 78 20 12 | A small, poor cluster; the preceding of two distinct clusters. The stars 11 m. | 196 | | | | | | Viewed. Is a coarsely clustering part of the Milky Way .... | 125 | | 2059 | Nova. | 19 48 7·0 | 78 17 12 | A poor, small cluster. The following of two, just alike .... | 196 | | 2060 | M. 27 | 19 52 8·6 | 67 43 ± | (See fig 26.) A nebula shaped like a dumb-bell, with the elliptic outline completed by a feeble nebulous light. Position of the axis of symmetry through the centres of the two chief masses = (by microm) 30°·0 or 60° n f...s p. The diam of the elliptic light fills a space nearly equal to that between the wires (7' or 8'). Not resolvable, but I see on it 4 distinct stars 1 = 12 m at the s f edge; 2 = 12.13 m, almost diametrically opposite; 3 = 13 m in the n p quarter, and 1 = 14.15 m near the centre. Place that of the centre. | 166 | | | | | 10·0 | Place the most condensed part of the southern head; diameter in RA = 25°·0. A most extraordinary object; v B; an unresolved nebula, shaped something like an hour-glass, filled into an oval outline with a much less dense nebulosity. The central mass may be compared to a vertebra or a dumb-bell. The southern head is denser than the northern. One or two stars seen in it. | 90 | | | | | 13·3 | I showed a friend the oval filling up of the outline of this strange object as delineated in Sw 266, and he saw it well. | 267 | | | | | 15·0 | Like a double-headed shot or a dumb-bell. The light perfectly milky; the s p head is a v l the brighter. The outline is filled up elliptically with a F nebulosity as in figure, which, I think leaves ansae as if inclined to form a ring. Two S st in it and many more near, one close to edge (No. 1 of Sw 166). A most amazing object. Position of greater axis of the elliptic outline = 117°·1; of axis of symmetry 31°·4 (microm). | 266 | | 2061 | Nova. | 19 54 58·2| 79 12 19 | A pretty rich oblong cl; 10' l, 5' br; stars equal and of 13th mag. In Milky Way. Place that of a double *. | 196 | | 2062 | III. 144| 19 55 12·4| 56 54 26 | A small bunch of very minute Milky Way stars, so small as almost to look nebulous; n p is another. | 199 | | | | | 13·9 | A nebulous-looking patch; 12'' diam; in Milky Way; ill-defined; perhaps only some e minute stars mixed with larger which are distinct. | 198 | | | | | 15·0 | F; S; R; among a field full of stars ......................... | 168 | | 2063 | Nova. | 19 55 28·2| 34 20 3 | A small pretty close cluster; irreg R; 3' diam; stars 12...16 m. | 211 | | No. | Synonym. | R 1830°.0 | N.P.D. 1890°.0 | Description and Remarks | Sweep. | |-----|----------|-----------|----------------|-------------------------|--------| | 2064 | M. 75 | h m s | 19 56 2·5 | v B; R; v s v m b M; 2'; a bright R ball 15'' diam, in an atmosphere 2'; 320 does not show the stars but makes it more resolvable. | 369 | | | | | | p B; R; p s v m b M; r; 90'' ........................................... | 298 | | | | | | Not B; S; R; p s b M; 2' diam; r, but not resolved. An insignificant object. | 275 | | 2065 | Nova. | 19 56 12·0| 94 1 59 | A little compact knot of 7 or 8 stars taken at first for a nebula, (and liable to be mistaken for one hereafter). Stars 19 m. | 83 | | 2066 | VII. 59? | 19 58 12·2| 46 28 50 | A coarse rough cluster. Taken for VII. 59, but the place does not agree. | 203 | | 2067 | Σ. 2630 | 19 59 30·6| 54 42 17 | A double ∗ Σ. 2630, in a cluster of 5 bright and many small stars. | 168 | | 2068 | Σ. 2631 | 20 0 45·7 | 69 23 2 | A double ∗ the chief of a coarse straggling group of stars 10...13 m, hardly entitled to be called a cluster. | 362 | | 2069 | VIII. 86 | 20 1 39·0 | 52 14 43 | A coarse scattered cluster of about 60 stars. The largest (10 m) taken. | 200 | | 2070 | Nova. | 20 4 51·5 | 54 39 36 | A double ∗ in a cluster of a good many stars 10...13 m .... | 168 | | 2071 | VIII. 20 | 20 4 51·7 | 64 1 10 | Splendid cluster. More than fills the field; loose and straggling; poor in stars, one = 6.7 m whose place is given; the rest 9, 10, 11. | 167 | | 2072 | IV. 13 | 20 9 31·6::| 59 59 ± | Planetary nebula; diam [by inexperienced estimation] = 1'; light equable, exactly round; v F, a mere ghost; P D roughly taken and of no value. Sept 4, 1825. | 7 | | | | | | e F; 15' diam; strongly suspected to be annular, but the darkness in the centre is not striking. | 199 | | | | | | e F; annular; pretty sharply defined; a very little elliptic; the northern limb is the brightest; the darkness in the middle requires some attention to see, but once seen it cannot be mistaken. A most curious object, resembling much the annular nebula in Lyra, but rounder, smaller (not above half the diameter,) and far fainter. (See fig 48.) | 198 | | | | | | Viewed Sept 7, 1825, past merid, the transit being missed owing to its faintness. It is exactly R, but decidedly brighter at the edges than in the middle. It is a round miniature of the annular neb in Lyra (40'' estim diam,) having a darkness in the middle. I made my assistant come up and look at it. He said it had a hole in it. (N.B. Much better seen than last night (Sweep 7), and more attentively examined.) | 8 | | 2073 | Nova. | 20 13 55·5| 109 50 39 | A ∗ 10 m, with a considerable nebulous appendage s p, in which by glimpses may be fancied a star 15 m. | 268 | | | | | | A ∗ 10 m, with a nebulous wisp, in which by glimpses a ∗ 18 m may be seen; pos = 194°9 by microm. A very curious object. | 297 | | | | | | A ∗ with a nebula attached in which is a small ∗ or nucleus 17 m. | 270 | | 2074 | Nova. | 20 14 29·7| 64 47 10 | A small straggling cluster of stars 10...11 m. One of the 9 m, whose place is taken. | 167 | | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks | Sweep. | |-----|----------|-------------|----------------|-------------------------|--------| | 2075 | IV. 16 | h m s | °′″ | Fine planetary nebula; B; exactly round; rather hazy at the edges, but not materially brighter in the middle, but no hollow. It has four small stars near it like satellites. (See fig 47.) Pos of B = 358°.0 by micr, dist estim 30″, 10 m; of D pos = 41°.2, 60″, 13 m. Clouded suddenly before I could measure the others. | 364 | | | | 20 14 46.1 | 70 26 7 | 48.0 | 25 40 | Exactly R; F; diam = 2″ in RA = 30″±. Its light is a little mottled, but it is well defined. Lies between 2 stars, but nearer to the southern (A) than to the northern (B); A is 85° sf (i.e. pos = 175°), and the centre of the neb is ¼ of its diam to the preceding side of their line of junction. | 90 | | | | | | 48.8 | 26 7 | Fine planetary nebula. R; diam = 18 or 20″; a little hazy at the edges, or rather pretty much so, so as to be ill defined. Has 4 stars near; one of them (B) = 10 m, pos = 359°.0; dist 40″; another (C) = 11 m, pos = 104°.8, 60″; another (A) is very nearly in a line with B and the centre, perhaps a degree or two to the following side; the neb is pretty bright. | 362 | | 2076 | III. 141 | 20 14 56.5 | 115 20 32 | v F; L; R; v g l b M; 3′ diam; r; the sky hazy. | 289 | | 2077 | VIII. 56 | 20 17 0.8 | 49 44 48 | A poor and coarse but rather brilliant cl, 2 st 9 m (the n p taken) and 30 or 40 more 10...12 m. | 183 | | | | | | 2.0 | 49 ± | A fine cluster of about 30 stars, one = 8 m taken, (but very coarsely); one = 9 m, and many stragglers 10...16 m. | 201 | | | | | | 12.9 | 47 7 | p B; S; the stars are 11 m, and two are 7.8 m. Place that of the sf. 40 stars counted, 5′ long, 3′ broad. | 359 | | | | | | ... | 50 ± | A fine close cluster of p L stars, not rich; irreg fig. | 180 | | 2078 | M. 29 | 20 17 45.5 | 52 1 48 | A coarse cluster of 8 large stars (10 m), and a dozen or 20 smaller in a roundish form. (Milky Way.) | 200 | | 2079 | III. 142 | 20 24 16.6 | 92 35 51 | v F; p L; 1E in merid; the n p of 2... | 81 | | | | | | 20.6 | 35 38 | v F; p L; p m E; or two joined; nearly in the meridian. | 288 | | 2080 | Nova. | 20 24 33.1 | 92 36 51 | v F; v S; the sf of 2... | 81 | | | | | | 36.5 | 36 8 | v F; among small stars. | 288 | | 2081 | I. 103 | 20 25 50.8 | 83 9 39 | Globular cluster; diam in RA = 4°; all well resolved; p g b M; a * 9 m precedes 7°5. | 281 | | | | | | 51.9 | 9 55 | Observed with M. Struve the evening of his arrival at Slough. | 282 | | | | | | 52.1 | 9 37 | A beautiful, v compressed, B, R, globular cluster, 3′ diam, well resolved. Stars = 16...20 m. A p B * p. | 280 | | 2082 | VII. 17 | 20 27 15.6 | 68 20 ± | Place of the chief * 10 m of a coarse, poor, straggling cluster | 166 | | | | | | ... | 23 ± | Very poor. The large star taken but carelessly, as it offers no interest. | 90 | | 2083 | VI. 42 | 20 27 56.4 | 29 56 37 | A * 11 m with a rather poor cluster of stars 12...15 m; G near full, but probably in dark night a rich cluster, 5′ in diam, fan-shaped, and a B * at the point. | 218 | | | | | | 59.6 | 55 42 | Fine, rich, p compressed cluster; 5′ diam; stars 11...13 m, rather convex on the p side. | 367 | | | | | | 64.3 | 55 44 | Very fine rich cluster; 5′ diam; stars 12 m and nearly equal; shape rather convex towards the preceding side. | 366 | | | | | | 72.1 | | Very fine rich cluster; stars 11...16 m, (not stated what part of the cluster taken, probably the middle; whereas the foregoing observations evidently refer to the preceding bright star). | 214 | | No. | Synonym | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 2084 | IV. 76 | h m s 20 31 16·9 | 30° 26' 2" | a v F; v L patch, no doubt a cluster 8 or 10' in extent, v g v l b M; but I cannot see the stars. | 367 | | | | | 18·9 | 26 14 | v F; e L; v g l b M; r; 5' or 6'; irreg fig. A curious object; no doubt a great cluster of e F stars. Requires the eye to be well prepared for seeing it. | 366 | | | | | 21·7 | 27 11 | v F; v L; v g b M to near the middle, and then p s b M; 8 or 9' diam; is barely resolvable; seems to be an enormous cluster, immensely distant. | 214 | | 2085 | VIII. 23 | 20 33 17·6 | 73 56 54 | Poor, large, scattered cl; the brightest *= 10 m. | 92 | | 2086 | III. 219 | 20 35 48·6 | 78 5 58 | v F; S; 15" precedes and is attached to the double star No. 1566 of my fourth catalogue. | 196 | | 2087 | II. 426 | 20 38 35·1 | 90 18 16 | p F; S; R; g b M; 15 ... 20" | 81 | | | | | 36·2 | 17 8 | e F; S; R; l b M; 12" | 294 | | 2088 | V. 15 | 20 38 38·6 | 59 53 30 | The place is that of k Cygni, through which the nebula passes. It is very long and winding and runs northward from k full 2 fields' breadth (30'). One branch is pretty conspicuous, even in a little moonlight. The nebulosity is milky, and does not seem to arise from small stars of the Milky Way ill seen. | 178 | | | | | 38·9 | 53 56 | The neb extends southwards far beyond k Cygni, but is e F; the northern part is p B (at least in a very clear night) and extends to two stars. P D = 59° 26' 56". [A drawing made, which with others made since has served for the construction of fig 33, which represents this extraordinary object.] | 199 | | | | | 38·6 | ...... | Northwards from k Cygni 27' extends a curved tail of nebula of a serpentine form, fading very gradually into two tails forming a fork. Its general direction is in the meridian. Barely attains k Cygni, and is there of extreme tenuity. Requires a fine night and the eye well prepared by at least 3m exposure to darkness. | 198 | | 2089 | II. 427 | 20 38 41·1 | 90 19 36 | F; v S; R | 81 | | | | | 41·7 | 18 33 | e F; v S; 6" | 294 | | 2090 | M. 72 | 20 44 5·1 | 103 10 26 | F; R; g b M; resolved into very small stars; 2 or 3' diam. | 10 | | | | | 5·8 | 10 9 | p B; v compressed cluster; irreg R; barely resolved; v g b M; 3' diam; many straggling stars near, but none so small as those of the cluster. | 365 | | | | | 6·5 | 10 13 | F; R; 2' diam; g b M; r, but I do not see the stars separated enough to count them. Sky beautiful. Has a * 9 m 30° s f, dist 3'. Is rather an insignificant object. | 34 | | 2091 | VIII. 76 | 20 48 51·0 | 43 22 10 | A star 9 m; the largest of a cluster | 210 | | | | | 77·6 | 18 22 | A * 11 m. The last of that magnitude in an irregular triangular cluster 6' diam; poor and straggling. | 209 | | 2092 | V. 14 | 20 49 19·1 | 58 57 1 | Place of the southern and brightest star of a trapezium south of the bifurcation of this nebula. The neb is e F, v L, and straggling, extending at least 4 fields (= 1'). Its direction is (by diagram) about 20° n p to s f, and near the middle it forks into two chief branches. (See fig 34.) In the trapezium (or oval) above spoken of arc 6 stars 1 = 11 m; 2 = 10 m; 3 = 12 m; 4 = 14 m; 5 = 15 m; 6 = 12 m. The northern branch of the fork is the principal, and passes s of a double * (7). | 199 | See next page. | No. | Synonym | RA 1830.0 | N.P.D.1830.0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | | | h m s | ° ' ". | | | | 2093 | Nova. | 20 50 4·4 | 60 26 6 | The same star in the nebula V. 14. The nebula is of great extent, passing obliquely through and rather under (to the s of) a small constellation, being densest where under it; but it is extremely F and only to be seen with an eye well prepared and in a very clear night. The whole neighbourhood seems affected with wisps or cirro-stratus-like masses of nebula. (See figure 82.) A most wonderful phenomenon. A very large space 20' or 30' broad in P D, and 1m or 2m in R A full of nebula and stars mixed. The nebula is decidedly attached to the stars and is as decidedly not stellar. It forms irregular lace-work marked out by stars, but some parts are decidedly nebulous, wherein no stars can be seen. A figure (from which the drawing for the engraving was copied,) represents general character, but not the minute details of this object, which would be extremely difficult to give with any degree of fidelity. | 198 | | 2094 | VIII.82? | 20 50 28·0 | 45 10 50 | Coarse, poor, p L cluster; stars small | 8 | | 2095 | Nova. | 20 52 22·0 | 90 51 31 | Viewed. A mere clustering portion of the Milky Way | 189 | | 2096 | V. 37? | 20 53 12± | 46 20 ± | e F; S; E in the meridian | 81 | | 2097 | I. 52 | 20 53 36± | 74 28 49 | An immense nebulosity all around this place, but too ill defined to fix the limits. R A that of V. 37, from working list, not being settled by the obs. B; R; g b M; 60"; RA from working list, no transit being procured. | 203 | | 2098 | IV. 1 | 20 54 50·5 | 102 2 46 | Fine planetary nebula. The disc is exactly round, and nearly of an equal light throughout; blueish white; a little haze about it: has a * 15 m n p (about 80°) dist = 3 diameters. Round; v B; equal to a * 6.7 m; the light perfectly equable, only a little dim at the edges; diameter = 300". v B; diam 20 . . . 25"; a little oval, perfectly well defined | 12 | | | | 52·0 | 1 53 | Round; v B; equal to a * 6.7 m; the light perfectly equable, only a little dim at the edges; diameter = 300". v B; diam 20 . . . 25"; a little oval, perfectly well defined | 10 | | | | 54·3 | 2 4 | Exactly round; a very little hazy at the borders; the rest of the disc quite equable; light blue; diam 10 or 12". [See fig 44. M. STRUVE has given as measures of the diameters of this nebula 25" and 17". From the general tenor of the foregoing obs I am disposed to think this ellipticity greater than the real.] | 365 | | 2099 | I. 192 | 20 55 25·0 | 36 6 23 | L; E; r; has an appearance of two nuclei or points of greatest condensation; it touches a fine double star. | 34 | | | | 36·0:: | 6 55 | L; E; 60" l, 40" br; r; one star is very plainly seen; it is rather wedge-shaped, pos = 225° ±. A double * is close to it. RA very doubtful. | 211 | | 2100 | Nova. | 20 55 27·1 | 103 10 11 | e F; R; r; 60" | 48 | | 2101 | Nova. | 20 56 6·5 | 43 20 50 | A cluster. No further description. | 210 | | 2102 | II. 203 | 20 56 21·8 | 60 46 18 | p B; S; p s b M; 12"; has a * 10 m, pos 345° 0 by microm; field full of stars. | 177 | | | | 23·8 | 46 48 | p B; R; p s b M; 15" | 178 | | 2103 | VIII. 57| 20 59 38·5 | 49 11 7 | A loose straggling coarse cl. Stars 10 . . . 11 m, place that of 3 *s 10 m in a triangle in the closest part. Several st precede the cl, which seems to be an outlier of the second branch of the Milky Way. | 183 | | | | 101·0 | 8 31 | A poor and loose cluster; place that of a double star, h. 1613 of my fourth Catalogue. | 180 | | 2104 | Nova. | 21 2 11·7 | 75 14 19 | A scattered cluster of small stars | 12 | MDCCCXXXIII. | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep | |-----|----------|-----------|---------------|-------------------------|-------| | 2105 | VIII. 74 | 21h 2m 29s+ | 39° 50′ 24″ | A curious scattered cluster of triple stars; RA taken from working list. | 207 | | 2106 | Nova. | 21 3 49·3 | 56 58 6 | A cluster, not very rich; irreg figure, 8′ 1, 5′ br; stars 11...15 m | 199 | | 2107 | Nova. | 21 5 9·8 | 45 0 51 | A star 6·7 m situated just beyond the nf edge of a L, p rich cluster, 11...15 m, 20′ long, 7′ broad. Extended from nf to sp. | 210 | | 2108 | Nova. | 21 6 18·4 | 86 10 55 | e F; field feebly illuminated by ζ, but I remained satisfied of its reality. | 79 | | 2109 | III. 858 | 21 6 20·7 | 87 51 53 | e F; R; 1b M | 95 | | | | 22·9 | 51 25 | e F; R; barely visible; night exquisite | 94 | | 2110 | VI. 24 | 21 6 34·7 | 48 11 8 | v F; L; irreg fig; p rich; not m b M; 2 or 3 p L stars, the rest 16...18 m; 5′ diam. | 204 | | | | 40·9 | 13 3 | v F cl of e S st, 15...18 m; irr fig; p L; v g l b M; 4′ diam; a delicate object. | 183 | | 2111 | Nova. | 21 8 20·3 | 54 30 41 | No description. A cluster | 168 | | 2112 | III. 145 | 21 11 17·4 | 64 16 47 | F; R; 20″; the RA may be 2° or 3° out | 172 | | 2113 | Nova. | 21 12 43·6 | 99 30 3 | v F; R; g b M; near a double star | 86 | | 2114 | Nova. | 21 14 34·8 | 33 7 25 | A F, S, poor cluster, 8′ diam | 212 | | 2115 | Nova. | 21 15 16·0 | 39 54 40 | The chief * of a coarse, poor cl | 207 | | 2116 | VII. 51 | 21 17 5·4 | 44 21 8 | A neat, pretty compact cluster of 50 or 60 stars 4′ diam; irreg fig; a * 13 m taken, the chief in the preceding part. | 203 | | | | 7·2 | 20 32 | A * 10 m, the preceding of a cl, 4′ in diam, and pretty rich | 209 | | | | 7·6 | 20 28 | A fine cluster of a triangular figure; the preceding * taken | 210 | | 2117 | Nova. | 21 17 31·5 | 54 13 24 | A poor cluster, stars 10 m | 168 | | 2118 | VII. 50 | 21 18 33·0 | 42 42 27 | A double *. The chief of a poor cl | 209 | | 2119 | Nova. | 21 20 26·6 | 42 48 6 | A very poor and small cluster of an oblong figure. It is followed by a loosely scattered mass of stars. | 210 | | 2120 | M. 15 | 21 21 43·0 | 78 34 19 | v B; v L; irreg R; g b and v s m b M. A magnificent globular cluster; comes up to a perfect blaze in the centre, like a protuberance or nipple; not the condensation of a homogeneous globe; it has straggling streams of stars, as it were, drawing to a centre. It is not round. Has a * 8 m, 30° following in parallel. | 14 | | | | ... | 36 ± | Superb; very comp; irreg R; v S stars 15 m, all distinct but running together into a blaze in middle; 4′ or 5′ diam. One * 8 m nf dist 10′. | 13 | | 2121 | III. 859 | 21 22 47·0 | 88 15 13 | v F; S; R; has a * 14 m south. Dist from centre = 1 diam (by diagram). | 295 | | 2122 | VII. 52 | 21 23 16·9 | 43 38 57 | A * 10 m, the chief of a p rich, fine, L, 'coarse cluster. Stars 10...13 m. | — | | 2123 | Nova. | 21 23 46·7 | 73 19 19 | A coarse scattered cluster | 12 | | 2124 | VI. 32 | 21 24:35·7 | 39 10 30 | A ruddy * 11 m in midst of a beautiful cluster of stars 16...18 m; 8′ diam; not very comp; ζ troublesome. | 207 | | | | 47·4 | 9 4 | A rich fine cluster of st 11...16 m; it fills field; but the most comp part is about 6′ in extent. The middle of the cluster taken, but no particular star fixed upon. [N.B. This and the former obs disagree in the minute of RA, this giving 23, the other 24. The latter is probably right, agreeing better with my Father's determination.] | 384 | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks | Sweep. | |-----|----------|-----------|--------------|------------------------|-------| | 2125 | M. 2 | h m s | ° ′ ″ | A fine large globular cluster; it shines out between the clouds, and I see the stars of which it consists; and the determination of its place is good, though there is not a star now to be seen with the naked eye for clouds. (See fig 88.) | 81 | | | | 21 24 39·6 | 91 34 11 | A most superb cluster; round; stars e S; 12, 13, 14 m; they are evidently globularly arranged, and not internally condensed towards the centre more than the spherical form would make them appear to be; but in the middle they blend into a blaze of light. It is like a heap of fine sand! With 9 inches aperture I can just see the stars; with 6 it is resolvable. | 288 | | | | 40·0 | 91 34 18 | ... 35 ± | | | | | | | A most glorious cluster of stars 15 m compressed up to a blaze. Its most crowded part takes 6° to pass the wire, but there are straggling stars, although few, of the same size as the rest. There must be thousands of them. The total light of the cluster not exceeding a star 6 m, it follows that several thousand stars 15 m = 1 of 6 m. | 96 | | 2126 | M. 39 | 21 26 7·8 | 42 18 52 | A * 7 m, one of a large loose cluster of stars 7 ... 10 m; very coarsely scattered, and filling many fields. | 209 | | 2127 | Nova. | 21 27 57·8| 44 45 3 | The chief star (9 m) in a cluster of the 8th class. The double * No. 1660 of my fourth catalogue belongs to this cluster. | 210 | | 2128 | M. 30 | 21 30 41·5| 113 55 26 | Fine cluster; irreg R, with two projections A, B, at its northern side. (See fig 90.) A is directed from the central brightness and consists of 3 or 4 bright stars 12 m; its position taken with microm = 350°·4; B originates in the preceding side of the centre, and is directed in a position 331°·7 in a line not passing through the centre: diam = 6', stars = 12 m; fine object; has a * 9 m preceding it (2 or 3 diameters by diagram). | 299 | | 2129 | Nova. | 21 38 8·4 | 36 9 35 | A small, poor, but neatly defined cluster of stars 10 ... 12 m; with appendages n p at some distance. | 212 | | 2130 | VII. 40 | 21 38 20·3| 37 5 2 | A star 9.10 m of a ruby red colour in an oval annulus of small stars 4' diam. | 384 | | 2131 | IV. 75 | 21 39 2·2 | 24 40 41 | A very coarse triple star involved in a nebulous atmosphere; a curious object. The neb is e F and graduates away. | 221 | | | | 4·7 | 40 17 | Three stars in a nebula. Pos of A and B = 296°·3, Δ R A = 8°·0; pos of A and C = 46°·3, Δ R A = 8°·0; the place is that of A. | 224 | | 2132 | II. 261 | 21 40 20·6| 68 37 4 | F; R; v glb M; 30"; r ........................................... | 166 | | | | 21·5 | 37 44 | v F; irreg R; 40"; r ........................................... | 90 | | 2133 | Nova? | 21 41 21·7| 60 49 46 | Strongly suspected neb, or a v F double star with nebulosity. Has a * 11 m n p. | 177 | | 2134 | VII. 66 | 21 41 51·0| 24 58 57 | The chief star in the sf part of a large, pretty rich, loose cluster of st 12 ... 14 m; diam 10'; has more than one * 10.11 m in it. | 221 | | 2135 | III. 452 | 21 45 56·7| 87 51 33 | F; R; p L; 40", v glb M ........................................... | 295 | | | | 57·7 | 51 5 | p F; S; R; p s b M ........................................... | 95 | | | | 58·8 | 51 8 | e F; p L; b M; a glorious night ................................ | 94 | | 2136 | VIII. 67 | 21 48 56·7| 28 11 31 | One star 8 m (place taken), 4 = 10 m, 2 = 11 m, and a few smaller. | 217 | | 2137 | III. 930 | 21 50 10·6| 107 19 11 | Suspected, but the state of the air is most unfavourable ....... | 37 | | No. | Synonym. | RA 1830°.0 | N.P.D. 1830°.0 | Description and Remarks. | Sweep. | |-----|----------|------------|---------------|--------------------------|-------| | 2138 | III. 692 | h m s 21 51 52·1 | 104° 5' 16" | The faintest thing imaginable ........................................... | 10 | | | | | | v F; E; PD only a rude approximation .................................. | 34 | | | | | | v F; R; v g b M; r; 90" .................................................. | 9 | | 2139 | II. 247 | 21 52 25·5:: | 73 5 23 | R; g b M to a nucleus; has a * 89° s p, dist 90...100" .............. | 11 | | | | | | p B; R; g b M; 60...90". [N.B. The right ascensions in these early sweeps cannot be relied on.] | 12 | | | | | | B; R; p s b M; 20"; equals a * 10 m .................................... | 92 | | 2140 | III. 693 | 21 52 46·6 | 111 22 2 | v F; S; R; l b M; the first of 2 ....................................... | 299 | | 2141 | Nova. | 21 52 52·7 | 35 59 25 | The chief * 9 m of a v L, loose clustering group which fills two fields and is pretty rich of large stars. | 212 | | 2142 | II. 595 | 21 52 56·1: | 109 43 51 | e F; p L; R; the RA may err 10s ......................................... | 285 | | | | | | v F; p L; R; p g l b M; 50" .............................................. | 297 | | 2143 | II. 1 | 21 53 11·0 | 111 37 26 | p B; p L; v m E; position = 64°·3; p s v l b M; 2' long ............... | 299 | | 2144 | Nova. | 21 53 28·6 | 111 17 36 | v F; p L; irreg R; v g l b M; the second of two ....................... | 299 | | 2145 | Nova. | 21 55 14·3 | 80 0 0 | A coarse straggling cl. Stars 9.10 m .................................... | 14 | | 2146 | II. 599 | 21 55 52·8 | 49 46 8 | v F; l E; S; v g l b M; 15" .............................................. | 183 | | 2147 | VII. 53 | 21 58 30·4 | 44 20 18 | A * 10 m about the centre of a fine L rich cl; stars 9...12 m; fills field. | 210 | | | | | | Place of * 10 m near the middle of a fine L p rich cluster; 50 stars from 10 m to 13 m counted. It fills field. Moon full. | 209 | | 2148 | Nova. | 21 58 35·5:: | 62 43 0 :: | e F; R; b M; ill-defined; a v F double star 45° n p 4' dist points just to it. | 103 | | 2149 | II. 207 | 22 0 16·9 | 59 29 20 | B; R; 30"; g b M ............................................................. | 199 | | 2150 | II. 897 | 22 0 56·7 | 107 28 41 | No description ........................................................................ | 37 | | 2151 | III. 862 | 22 3 0·4 | 49 49 36 | e F; S; E; among 3 stars, with which however it seems not connected. | 183 | | 2152 | III. 931 | 22 4 59·5 | 107 54 31 | v F; R; b M; 20" ..................................................................... | 37 | | 2153 | II. 606 | 22 5 30·0 | 45 29 43 | A most e F nebulous appearance, which is probably only a few minute stars. No other near. | 204 | | 2154 | VIII. 63 | 22 6 30·8 | 33 34 23 | A * 10 m, the chief of a p compact cluster of 15 or 20 stars 10...17 m. One, 11 m, is of a ruby colour. | 211 | | | | | | A poor cl. South of the chief * is a ruby star 10 m. (N.B. These ruby stars often occur in clusters.) | 212 | | 2155 | VIII. 75 | 22 8 30·4 | 40 57 50 | A double * in a very loose straggling cl which more than fills the field. | 207 | | 2156 | III. 932 | 22 8 31·2 | 106 25 43 | v F; R; v g b M; has * 13 m south, at a dist from edge = 1 diam by diagram. | 274 | | 2157 | VI. 29 | 22 8 55·4 | 36 30 57 | A Milky Way cluster. Stars 14...15 m. It is more crowded than the Milky Way, so as to run up to a condensed but faint mass of light. | 384 | | 2158 | III. 933 | 22 11 11·3:: | 106 38 11 :: | e F, but certainly seen; p L; vision v bad ............................... | 37 | | | | | | p F; l E; g p m b M; 20" .................................................... | 274 | | | | | | v F; R; but hazy. In occasional glimpses p B ......................... | 273 | | 2159 | Nova. | 22 14 19·0 | 32 45 52 | The chief * of a coarse p rich cluster which fills the field. Stars 10...15 m. | 215 | | No. | Synonym | RA 1830°-0 | N.P.D. 1830°-0 | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 2160 | II. 284 | 22 18 8°5 | 74 43 3 | F; R; g b M, to a bright point | 11 | | | | | 12°7: | 42 59 | | | 2161 | Nova. | 22 18 33°5 | 33 1 32 | Large, coarse, not extremely poor, the stars scattered and 10...16 m. | 215 | | 2162 | Nova. | 22 19 29°1 | 61 45 56 | v F; R; 12"....15"; among stars | 177 | | 2163 | VII. 41? | 22 21 10°2 | 38 2 35 | A Milky Way straggler; a poorish cluster of stars 12....13 m | 384 | | 2164 | Nova. | 22 21 51°5 | 104 53 37 | F; p L; a strong suspicion; almost sure | 273 | | | | | 52°2 | 53 8 | | | 2165 | IV. 31 | 22 23 15°6 | 104 59 37 | v F; R; v g l b M; 20"; twilight commencing | 274 | | | | | | F; p L; R; v s b M to a S, F, R nucleus; diam 2'; has a * sf in pos 352°5 by micr; dist 3' | 273 | | | | | 15°7 | 60 23 | | | | | | 16°7: | 59 51 | | | | | | 18°5 | 58 57 | | | 2166 | Nova. | 22 23 31°3 | 59 54 58 | v F; R; v g b M; 12"; fog coming on | 178 | | | | | 40°3 | 54 16 | | | 2167 | II. 476 | 22 25 19°5 | 101 13 15 | v F; p L; b M; 2'. | 34 | | | | | 20°0 | 13 38 | | | | | | 20°1 | 15 16 | | | | | | 21°0 | 14 13 | | | | | | 22°1 | 14 12 | | | 2168 | II. 428 | 22 25 31°9 | 85 18 18 | Not v F; S; p s b M | 94 | | | | | 34°3 | 18 46 | | | 2169 | III. 180? | 22 26 14°3: | 70 33 ± | No P D obtained for clouds, but found by working list; e F | 90 | | 2170 | III. 237 | 22 28 19°9 | 69 15 7 | p F; irreg R; v g v l b M; 15...20" | 290 | | 2171 | Nova. | 22 29 2°1 | 80 20 30 | v F; R; v g l b M; 20" | 305 | | | | | 3°2 | 20 19 | | | | | | 3°8 | 20 20 | | | | | | ... | 20 19 | | | 2172 | I. 53 | 22 29 17°4 | 56 28 46 | v B; p L; s m b M; E 70° n p to s f; 90" l, 30" br. If I. 53, the working list is 9' out in P D. | 105 | | | | | | B; m E; p s b M; r; 30" l, 12" br; has another nebula 14°5 following; pos about 55° s f, n p. | 168 | | 2173 | II. 233 | 22 29 18°1 | 67 4 36 | B; S; m E in pos = 163°0 by microm; v s m b M to a * 11 m | 166 | | | | | 18°6 | 5 7 | | | 2174 | III. 166 | 22 29 31°9 | 56 27 9 | e F; it is n f from I. 53; pos by microm = 61°8; Δ R A = 14°5. | 168 | | 2175 | II. 284 | 22 29 38°3 | 67 5 6 | F; S; E nearly in parallel; v g l b M | 166 | | | | | 41°6 | 5 27 | | | | | | | v F; m E in parallel; 60" l; the following of two and a third suspected. | 290 | | No. | Synonym | RA 1830° | N.P.D. 1830° | Description and Remarks | Sweep | |-----|---------|----------|-------------|------------------------|-------| | 2176 | Nova. | 22 31 28·4 | 79 52 0" | e F; p L; 60" l, 30" br; a certain obs. | 304 | | | | | | Viewed; e F; about a radius of the field (= 7½') n p ξ Pegasi. | 305 | | 2177 | Nova. | 22 33 5·4 | 33 29 23 | A star 9.10 m, chief of a p rich, v L, very coarse cluster. | 211 | | 2178 | II. 705 | 22 34 0·1 | 29 36 27 | B enough to be noticed and caught in sweeping in full moonlight, with the C on merid; p g b M; R; no nucleus seen. | 218 | | 2179 | II. 442 | 22 35 41·0 | 91 3 18 | v F; S; R; p s b M; 15" | 288 | | | | 42·2: | 2 55 | p F; R; 25"; clouds interfered with the R A obs which may err 2s or 3s. | 371 | | 2180 | III. 477| 22 37 3·1 | 101 54 16 | e F; R. | 10 | | | | 5·5 | 54 21 | v F; p L; R; v g y l b M | 373 | | | | 6·1 | 53 57 | v F; p L; R; s b M, very dilute at borders | 34 | | | | 6·9 | 53 7 | e F; R; 20" | 372 | | | | | 53 53 | F; R; 1' diam; no other near | 9 | | 2181 | II. 598 | 22 38 34·0| 113 11 26 | p B; 1 E; g b M; 20" | 299 | | | | 35·2 | 11 34 | p B; R; b M; 15" | 293 | | | | 35·6 | 11 51 | p F; R; v g b M; 30...40"; several small stars near | 370 | | 2182 | VIII. 77| 22 39 28·1| 32 42 28 | A L, p rich, v coarse cl of stars 9.10 m and below. (No particular * taken.) | 211 | | | | 72·0 | 48 36 | A double *, the chief of a fine, p rich, L cluster, 10' diam; stars 9...13 m. | 214 | | 2183 | III. 216| 22 41 26·4| 79 16 59 | F; R; g b M; a star precedes | 15 | | | | 32± | 17 30 | p B; R; 20"; has a * 11 m near. The preceding of two neb. | 304 | | | | | | The * by diag is 1 radius of the neb n p its edge. | | | 2184 | III. 217| 22 41 32·9| 79 12 5 | p B; R; the following of two. | 305 | | | | 39·5: | 12 5 | p B; S; R; p g b M | 304 | | 2185 | II. 443 | 22 41 52·0| 92 26 43 | p F; R; p s b M; 50...70"; has a * n p; pos by microm = 350°·3. | 288 | | | | 52·8 | 26 5 | p B; R; s b M to a * 13 m; 25". It has a * 12.13 m, 1' north | 371 | | 2186 | II. 702 | 22 42 37·0| 111 30 26 | p B; R; g b M; 20...30" | 299 | | | | 38·7 | 30 22 | p B; irr R; p g b M; 30" | 293 | | | | 39·1 | 30 46 | Not v F; 1 E; g b M; 60" l, 40" br. | 370 | | 2187 | II. 453 | 22 42 46·7| 96 27 24 | e F; R; v g b M; sky dull. | 184 | | | | 48·6 | 27 48 | No description | 186 | | 2188 | Nova. | 22 43 20·2| 38 43 24 | A double star, the last of a poor cluster of about a dozen stars | 208 | | 2189 | Nova. | 22 43 39·9| 89 48 24 | p F; irreg R; b M; 60"; r | 93 | | | | 41·6 | 48 31 | p F; R; g b M; 30" | 295 | | 2190 | VII. 43 | 22 47 32·3| 30 4 16 | A S cluster of small stars 12 m, diverging in a fan shape; a * 10 m follows. | 214 | | | | 39·5 | 5 3 | A * 10 m in a cluster of v S stars 15...18 m; p rich; v g b M. A * 8 m is 2' south. | 213 | | 2191 | III. 745?| 22 48 4·9 | 33 47 48 | A large patch of the Milky Way, consisting of stars so small as to be quite nebulous. If this be not III. 745, I find no other. | 211 | | No. | Synonym | RA 1830°. | N.P.D. 1830°. | Description and Remarks | Sweep | |-----|---------|-----------|---------------|------------------------|-------| | 2192 | III. 576 | 22 48 5'0 | 54 32 13" | F; S; R; b M; 12". A double * s p points back somewhat n of the neb. | 168 | | | | | | e F; p L; R; a coarse double * 6 m precedes a little to south. Hurried obs. | 105 | | 2193 | Nova. | 22 49 6'3 | 30 54 58 | VIII class; pretty compact, poor cluster; stars 9...11 m.... | 213 | | 2194 | III. 465 | 22 49 29'7:: | 77 47 19 | e F; R; b M .................................................. | 15 | | | | 34'3 | 46 25 | v F; R; 15"; has a double * foll................................ | 305 | | | | | 46 45 | e F; S; R; precedes a neat D * 5s............................. | 304 | | 2195 | III. 243 | 22 49 45'7 | 64 45 20 | F; E in parallel; g b M; 60" l, 30" br ....................... | 167 | | | | | | Viewed in place; v F; L; irreg fig; r........................ | 172 | | 2196 | Nova. | 22 50 20'2 | 36 33 31 | A large oblong cluster which fills two fields. Place that of the double star h. 3157 of my fifth Catal. | 384 | | 2197 | II. 450 | 22 51 10'9 | 103 42 53 | irreg R; p F; s b M almost to nucleus, r. The northern of a double neb. (See fig 73.) | 9 | | | | 12'5 | 42 41 | F; R; p s b M, rather the brighter of 2 ...................... | 373 | | 2198 | II. 451 | 22 51 11'4 | 103 44 23 | p F; irreg R; s b M almost to nucleus, r; the southern of a double neb. | 9 | | | | 12'5 | 44 21 | F; R; p s b M .................................................. | 373 | | | | | 44 26 | The southern of a double nebula ................................ | 10 | | 2199 | II. 251 | 22 51 38'5 | 74 55 23 | p B; L; v g b M; E pos 85° n p to s f ......................... | 11 | | | | 39'4 | 56 11 | No description .................................................. | 175 | | 2200 | II. 590 | 22 52 48'4 | 89 9 8 | Hardly visible for C, but sure of object ...................... | 108 | | | | 48'6 | 9 18 | v F; v S; p s b M .............................................. | 295 | | 2201 | II. 212 | 22 52 51'8 | 60 46 10 | B; L; 1E; p g b M; 60"; has a stellar point in the centre .. | 178 | | 2202 | III. 210 | 22 53 27'2 | 74 56 1 | No description. The first of 2 .................................. | 175 | | 2203 | III. 211 | 22 53 36'2 | 74 56 38 | No description. The second of 2 ................................ | 175 | | 2204 | III. 230 | 22 54 41'6 | 82 1 59 | F; S; R; v s m b M; equals a * 12 m with a v F wisp about it. At first seems a star. | 281 | | 2205 | I. 55 | 22 56 24'0 | 78 35 19 | p B; irreg R; r; I see 2 or 3 stars in it; E between 2 stars. (See fig 63.) | 14 | | | | 26'0 | 35 30 | B; m E; pos by micr = 192°0; p g m b M; has a * 12 m n p; a large * s, and one or two 15.16 m in or near the middle. | 304 | | | | 26'9 | 35 35 | p B; m E, pos by micr = 11°8 (= 191°8); 2' l, 30" br; between 2 small stars. Has two v S stars in it. | 305 | | | | 28'8 | 35 50 | p F; b M; E in merid between 2 stars; 90" l, 40" br .......... | 13 | | 2206 | Nova. | 22 57 8'7 | 87 22 23 | v F; E; p s b M; 20" l, 8" br ................................ | 295 | | 2207 | Nova. | 22 57 58'3 | 56 48 46 | v F; S; R; b M; 12"; has a * 10 m, 5' p in same parallel .. | 168 | | 2208 | III. 558 | 22 59 27'3 | 106 32 16 | e F; v L; 2 or 3'; the faintest thing imaginable; half way between two coarse double stars in same parallel. | 307 | | 2209 | III. 203 | 23 0 36'0: | 72 45 23 | e F; E like the tail of a comet; 1 b M ....................... | 11 | | | | 36'8 | 44 13 | v F; m E; pos 45° n f to s p; 4' l, 1' br .................... | 92 | | 2210 | III. 184 | 23 2 55'2 | 93 5 3 | Not v F; v S; R; b M; well observed ......................... | 96 | | | | 58'8 | 3 55 | Not v F; R; g b and s m b M to a * 15 m ..................... | 371 | | 2211 | II. 2 | 23 2 56'3 | 119 28 9 | F; R; b M; 30"; has a * 10 m, 10° n p; 4' distant ........... | 292 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|---------------|--------------------------|-------| | 2212 | Nova. | 23h 3m 14s | 77° 59' 19" | e F; seems to have a * in centre | 15 | | | | | | e F | 14 | | 2213 | VII. 44 | 23h 4m 4s | 30° 21' 1" | A fan-shaped cluster composed of two principal lines of stars drawing to one about 2°1'; pos 248°8 by microm. | 214 | | | | | | A v pretty fan-shaped cluster of p B close stars in two lines with other smaller to N. A * 10 m taken. Another 11m dist 19°0; pos = 244°. | 213 | | 2214 | III. 220| 23h 4m 16s| 78° 14' 20" | p B; p L; R; g b M; 30" | 304 | | | | | | p B; p L | 305 | | | | | | F; R; v g l b M | 13 | | 2215 | II. 229 | 23h 5m 56s| 86° 25' 43" | F; S; R; b M; the s p of 2 | 95 | | | | | | v F; irreg R; b M; the s p of 2; pos by microm 48°0 | 302 | | 2216 | II. 230 | 23h 6m 5s | 86° 23' 25" | v B; L; E, 10° n p to s f; 80"; the n f of 2; a * 10 m s f | 95 | | | | | | B; m E; pos about 5° n p to s f; 80" long; the n f of 2, pos of the other 228°0. | 302 | | 2217 | Nova. | 23h 6m 7s | 67° 14' 6" | F; S; R; p s b M; 12" | 166 | | 2218 | Nova. | 23h 6m 35s| 71° 56' 43" | The n p of 2 | 92 | | 2219 | Nova. | 23h 6m 48s| 71° 57' 43" | p B; R; 20" ; the s f of 2 | 92 | | 2220 | II. 235 | 23h 6m 59s| 93° 18' 52" | p B; R; a bright double * f | 96 | | 2221 | Nova. | 23h 7m ± | 78° 21' ± | F; R; b M; place very loose; two or three more nebulae suspected in the neighbourhood. | 174 | | 2222 | III. 221| 23h 7m 14s| 77° 37' 31" | F; R; v g b M; 30" | 175 | | | | | | p B; p L; R. Has a * 16 m in the centre. The n p of 2 | 304 | | | | | | F; R; b M; 30"; the n p of 2, the place by reference to the other | 15 | | | | | | F; R; v g b M; place very uncertain by estimation from the other. | 13 | | 2223 | III. 222| 23h 7m 19s| 77° 44' 19" | p B; S; R; s m b M; a B * near; the s f of 2; the R A supposes a mistake in the wire. | 15 | | | | | | p B; R; p s b M; 20" | 175 | | | | | | p B; p L; R; has a * 16 m in centre. The s f of 2 | 304 | | | | | | e F; b M; the R A supposes a mistaken wire | 13 | | 2224 | II. 467 | 23h 7m 20s| 84° 14' 9" | B; S; R; p s b M; 15" | 302 | | 2225 | III. 182| 23h 8m 44s| 72° 14' 8" | F. | 92 | | 2226 | II. 236 | 23h 9m 22s| 95° 34' 7" | p B; S; R. R A from working list | 96 | | 2227 | II. 431 | 23h 10m 5s| 98° 28' 44" | F; R; l b M; 15"; sky not good | 184 | | | | | | p B; R; p s b M; 15"; R A doubtful 2 or 3 seconds | 186 | | 2228 | I. 104 | 23h 10m 18s| 99° 25' 17" | v F; L; m E; night unfavourable | 372 | | 2229 | Nova. | 23h 11m 19s| 82° 31' 9" | e F; e S; sky clear. | 281 | | 2230 | II. 439 | 23h 11m 37s| 82° 44' 28" | B; p L; R; p s b M | 280 | | | | | | p B; R; b M; 30". PD inaccurate | 89 | | 2231 | III. 435| 23h 11m 54s| 82° 31' 39" | p F; R; p s b M | 281 | | 2232 | II. 250 | 23h 11m 56s| 73° 42' 53" | B; R; s b M; 60" | 11 | | | | | | p B; R; b M; 25" | 92 | | No. | Synonym | RA 1830°.0 | NP.D. 1830°.0 | Description and Remarks | Sweep. | |-----|---------|------------|--------------|------------------------|-------| | 2233 | II. 440 | h m s | B; R; pL; psbM ........................................... | 280 | | | | 23 12 6·7 | 82 42 48 | pB; R; bM; 30"; PD inaccurate ................................ | 89 | | 2234 | II. 441 | | | A double star with some singular nebulous appendage. The stars are 14 m. | 281 | | 2235 | IV. 52 | 23 13 20·3 | 29 45 1 | A star 9 m with a vF nebulous atmosphere or a nebula rather excentric towards the sp side. | 214 | | 2236 | II. 600 | 23 13 56·7 | 50 3 35 | vF; E; vglbM; 40", 20" br .................................. | 180 | | | | 59·1 | 5 40 | F; L; mE from a bright to a faint star; vlbM; 2½l, 20" br. See fig. 60. | 183 | | 2237 | Nova. | 23 16 21·5 | 75 39 23 | F; R; gbm; 40...60" ....................................... | 11 | | | | | 38 45 | eF; R; gbm; 30"; appears as M. 71 does in the 7-feet reflector with the double eye-piece. | 1 | | 2238 | M. 52 | 23 16 43·9 | 29 20 12 | A ruddy star 9 m in the p part of a p rich irreg cl of stars 13 m, all separate, 6' diam; a v little more comp in the sf part. | 218 | | 2239 | III. 212| 23 17 22·4 | 76 43 26 | vF; S; R; psbM; 15" ....................................... | 175 | | 2240 | Nova. | 23 17 24·2 | 63 54 0 | F; vS; psmbM; 6"; almost stellar; a star 10 mp; dist 1' in parallel. | 172 | | 2241 | IV. 18 | 23 17 42·1 | 48 24 24 | A fine Planetary Nebula. Diameter 12"; with 240 beautifully defined, light, rather mottled, and the edges the least in the world unshaped. It is not nebulous, but looks as if it had a double outline, or like a star a little out of focus. A perfect circle. Has a star near; pos 68°1, well measured over the centre of the nebula. See fig 45. | 183 | | | | 43·2 | 23 33 | vB; R; blueish white; 8 or 10" diam. It has no haze at the edges, but if it be not enveloped in an eF nebulosity (perhaps arising from glare) and also the star 13 m whose pos is 61·9 and ΔRA = 4°0. The light is a very little mottled and not absolutely planetary. It is = a * 7 m. (N.B. These satellites of planetary nebulae ought to be especially attended to.) | 180 | | | | 44·0 | 23 53 | Diameter in RA = 2°0 of time. The attendant star is double A = 12 m; B = 13 m, pos of A = 58°5; ΔRA from centre = 4°0. The nebula is not perfectly round; light equal, but a very little hazy at the edges. | 204 | | | | 44·3 | 23 40 | Exactly R; 2°5 of time = diam in RA. Has a * 13 m pos 69°0; dist 30"; the light of the disc is perfectly equable, and equals a star 8 m. | 189 | | | | 46·2 | 23 40 | Exactly R; = a * 8 m; a * 13 m n.f; pos = 65°6 by microm; dist = 30". [N.B. The great discordance in the measured positions of the satellite-star seems to arise from the star being double, and taken for a single one. Whenever this occurs, it is a source of error, and should be most carefully guarded against in all future observations of this interesting object.] | 190 | | 2242 | III. 226| 23 18 41·3 | 78 28 39 | pB; R; vsbM, almost to a star ................................ | 15 | | | | 44·9 | 28 0 | pB; S; vlE; bM; has a * 8 mp ................................ | 305 | | | | 45·0 | 28 10 | pB; S; R; a star 10 m precedes in parallel near the neb .... | 304 | | | | 45·8 | 29 0 | pB; S; R; 20"; mbM, with a hazy border. Approaching to a stellar, or a planetary character. [A mistake in the wire presumed in the transit observation.] | 13 | | No. | Synonym | RA 1830-0 | N.P.D. 1830-0 | Description and Remarks | Sweep | |-----|---------|-----------|--------------|------------------------|-------| | 2243 | Nova. | 23 19 18·6 | 82° 9′ 4″ | F; R; g b M; 30″. The p of 2 ........................................... | 281 | | 2244 | Nova. | 23 19 28·6 | 82° 9 49 | v; F; R; g b M; 20″; the f of 2 ........................................... | 281 | | 2245 | II. 226 | 23 19 57·8 | 68° 30 37 | F; v R; p L; l b M; very symmetrically situated in the southern part of a lozenge of 4 stars, on the longer diagonal, forming an elegant object. See fig 85. | 91 | | | | | 59·1 | 30 28 | 166 | | | | | | v F; R; v g b M. Occupies the southern half of a lozenge of four stars, its centre being just upon the longer diagonal. | | | 2246 | III. 860 | 23 20 21± | 58° 35 ± | S; R; query if not stars; RA by working list. PD rough. | 100 | | 2247 | II. 242 | 23 20 21·2 | 73° 37 53 | e F; S; it is a v F neb of third class .................................. | 92 | | | | 22·5: | 38 3 | v F; R; g b M; 20 . . . 30″; near a double * .......................... | 11 | | 2248 | III. 426 | 23 21 50·1 | 87° 2 3 | e F; L; 60 . . . 90″ ......................................................... | 295 | | | | | ... | e F; L; 90 . . . 2′ ............................................................ | 302 | | 2249 | VIII. 69 | 23 22 3·7 | 41° 49 2 | A bright coarse cluster 7′ diam; seen in full C. Place of the chief *= 7 m; about a dozen 9 . . . 11 m, and many 12 . . . 14 m | 209 | | | | | 3·9 | 47 54 | 208 | | | | | | A poor scattered cluster. Place of a * 8.9 m in preceding part. Full C on merid; so that I could not see the small stars. | | | | | | | A * 6 m in the middle of a cluster of about 50 stars coarse and straggling. | 207 | | 2250 | III. 213 | 23 23 50·0 | 75° 5 31 | e F; p L; forms a triangle with 2 st 10 m, near it ..................... | 175 | | 2251 | Nova. | 23 26 13·5:: | 74° 52 23 | v F; v S; g b M; 10″; has a * 1′ dist n f .............................. | 11 | | 2252 | Nova. | 23 26 21·2 | 86° 2 18 | e F; hardly perceptible; a * 12 m precedes ............................. | 94 | | | | | 21·3 | 2 28 | 95 | | 2253 | Nova. | 23 26 30·3 | 85° 58 58 | v F, but brighter than the preceding .................................... | 95 | | 2254 | III. 579 | 23 26 34·6 | 46° 37 28 | e F; follows a * 9.10 m. (? if not an e F double *) .................. | 204 | | | | | 36·7 | 37 50 | 190 | | 2255 | VIII. 62 | 23 26 58·0 | 18° 1 12 | A * 8.9 m, the chief of a scattered cluster of 30 . . . 50 stars, 10 . . . 15 m. It more than fills the field. | 378 | | | | | 62·5 | 1 47 | 228 | | | | | | A poor and coarse cluster of large and small stars. The largest (= 9 m) taken. | | | | | | | A star 8 or 8.9 m, the chief of a poor and diffused cluster of small stars. | 229 | | 2256 | II. 244 | 23 27 4·4 | 75° 38 31 | p F; R; p s b M; 15″ ....................................................... | 175 | | | | | ... | 37 ± | 1 | | 2257 | Nova. | 23 27 30·6 | 88° 46 48 | p B; S; R; p s b M; in field with 16 Piscium; a star 12 m near, sp; (dist = 1 diameter of neb by diagram). | 295 | | 2258 | Nova. | 23 27 47·8 | 90° 38 40 | Not e F; p L; 1 E; g b M; has a * 10 m exactly south, dist 2′ | 371 | | 2259 | III. 146 | 23 29 58·4 | 63° 55 32 | p F; R; b M; 20″............................................................... | 172 | | 2260 | II. 432 | 23 30 0·6 | 97° 27 48 | v F; L; R; v g b M; 60″ .................................................. | 186 | | | | | 2·5 | 27 32 | 184 | | | | | 5·0 | 27 9 | 185 | | 2261 | I. 110 | 23 30 7·5 | 103° 53 56 | No description ............................................................... | 373 | | | | | 9·4 | 53 53 | 9 | | | | | | Irreg R; g b M; 2′ diam; r. I certainly see one star near the middle. | | | No. | Synonym. | RA 1830.0 | N.P.D. 1830.0 | Description and Remarks. | Sweep. | |-----|----------|-----------|--------------|-------------------------|--------| | 2262 | I. 111 | h m s | 23 31 5·1 | pB; R; pgmbM; 40" | 373 | | | | | 6·2 | pB; R; vsmbM | 9 | | 2263 | Nova. | | 23 33 47·1 | vF; a star 14m with a nebulous brush extended towards the star, and on its sp side; position from the star by diagram = 250° or 260°. This disagrees with my Father's description of II. 208, which is said to be sf a star, but this may be a mistake for sp; but then also the RA disagrees 2m and the PD 6'. It can hardly, therefore, be the same object. | 172 | | 2264 | II. 255 | | 23 35 36·8 | B; R; aB*f | 15 | | | | | 37·1 | B; R; psbM; 25"; a*f | 305 | | | | | 37·2 | F; R; sbM; 20"; has a*f | 89 | | | | | 45·3:: | B; R; gmbM; 60"; has a small * one diameter following. [N.B. The RA is good for nothing, as are all those in the early sweeps before the chronometer was used.] | 13 | | 2265 | II. 256 | | 23 35 41·9 | R; smbM almost to a nucleus; has a*1' dist, 20°n f | 14 | | | | | ... | pB; R; sbM; 20"; r | 280 | | | | | ... | pB; R; psbM; 15"; has a*15m, dist 1'; pos = 153°8 by microm. | 305 | | 2266 | Nova. | | 23 37 3·4 | F; S; R; bM | 89 | | | | | 21 11 30 | About a * 8m is a very extensive space which I am certain is affected with nebulosity. | 223 | | 2267 | III. 427 | | 23 37 58·2 | Not vF; L; R; 40 or 50" diam | 295 | | | | | 57·4 | Not eF; pL; R; 1bM | 94 | | | | | ... | pB; L; near 2B stars 10 and 11m | 95 | | 2268 | II. 213 | | 23 38 32·0 | pF; L; vgBM; 70"; r | 177 | | 2269 | III. 437 | | 23 39 18·2 | F; S; R; gBM; 12...15" | 300 | | | | | ... | pF; S; R; 15" | 302 | | 2270 | Nova. | | 23 40 3·4 | vF; pL; R; vg1bM; 40"; a*13m, l'n | 300 | | | | | ... | vF; L; R; has a*13m north | 302 | | 2271 | III. 854 | | 23 40 34·3 | pB; psbM; 12"; query if not a F double * with neb | 178 | | | | | 36·6 | vS; r; I am sure I see 2 stars; a suspicious object, possibly (not very probably) a nebulosus D *. | 177 | | | | | 37·1 | B; vS; query if not 3 small stars close together | 100 | | | | | 37·6 | B; S; R; perhaps a* or two in it. [N.B. The obs makes the PD 59° 52' 55", but there is an obvious mistake of 5' in the reading off of the Index.] | 102 | | | | | 40·2 | Query if not 3 or 4 stars and nebulosity | 104 | | 2272 | VII. 55 | | 23 41 39·3 | avL, v coarse, rather poor clust of *s 11...15m. The most comp part taken. | 223 | | 2273 | Nova. | | 23 42 21·4 | vF; S; irreg fig; appears by glimpses to contain a vF double *, but it is a nebula. | 172 | | 2274 | II. 230 | | 23 42 22·6 | pB; R; bM; 25" | 91 | | | | | 26·5 | pB; S; R; bM; the np of two | 92 | | 2275 | II. 231 | | 23 42 43·6 | pB; E; bM; has a vS almost stellar neb about 45°sp dist 40" | 91 | | | | | 48·0 | pB; E; bM; has a smaller neb, 60°sp, 35" dist. (See fig.) | 92 | 3 q 2 | No. | Synonym. | R 1880°. | N.P.D. 1830°. | Description and Remarks. | Sweep. | |-----|----------|----------|---------------|-------------------------|-------| | 2276 | Nova. | 23 43 6'5'' | 74 41 23 | A cluster of scattered stars 10 m | 11 | | 2277 | II. 851 | 23 43 32'6'' | 59 40 20 | The faintest conceivable | 102 | | | | 36'2 | 41 ± | e F; s p a * (by diagram * 70° n f, dist 1 diam of neb from edge). | 104 | | | | ... | 42 ± | e F; R; near a * | 178 | | 2278 | III. 231 | 23 44 39'3'' | 83 4 9 | F; R; b M | 281 | | | | 39'9 | 4 3 | p B; R; p s b M; 20'' | 280 | | 2279 | III. 232 | 23 44 46'9'' | 83 3 53 | p B; R; p s b M; 20'' | 280 | | | | 47'3 | 3 49 | p F; R; p s b M; the brightest of 3 | 281 | | 2280 | Nova. | 23 45 6'3'' | 83 4 19 | F; S; R; the faintest of 3 | 281 | | 2281 | III. 233 | 23 45 13'0'' | 82 58 4 | p B; p L; R | 281 | | | | 13'6 | 58 18 | p B; p L; g b M; 40'' | 280 | | 2282 | II. 468 | 23 46 37'5'' | 85 1 34 | B; S; R; p s m b M; among three stars | 300 | | | | 37'5 | 1 44 | p B; S; l E; p s b M; among three stars | 302 | | | | 38'0 | 2 18 | p B; R; b M; r; a * 7 m precedes 30° ± | 95 | | | | 39'5 | 2 18 | p B; R; b M | 94 | | 2283 | Nova. | 23 48 12'4'' | 29 33 44 | v S and close cluster. One * 10 m with a great many very minute stars close to it. | 216 | | | | 14'6 | 32 52 | A p rich, S, condensed cl. One * 10 m, the rest 13 m | 219 | | 2284 | VI. 30 | 23 48 28'7'' | 34 13 48 | A most superb cluster, which fills the field and is full of stars; g b M; but no condensation to a nucleus; st 11...18 m. The place is that of a double *. | 211 | | 2285 | VII. 56 | 23 48 31'3'' | 29 43 52 | A double * in the p part of a pretty rich cluster; diam 4'; st 12...13 m; the f part most comp. | 219 | | 2286 | Nova. | 23 49 15'5'' | 80 10 20 | v F; v S. Query if not a star | 305 | | 2287 | Nova. | 23 50 4'3'' | 30 55 43 | A star 7 m, the chief of a v L coarse scattered but poor cl which fills the field. Stars 10 m. | 213 | | 2288 | III. 466 | 23 50 15± | 80 12 55 | e F; irreg fig; p L; 40'' | 305 | | 2289 | III. 867 | 23 50 18'2'' | 87 18 43 | e F; not v S | 95 | | 2290 | II. 232 | 23 50 45'7'' | 70 10 15 | p B; S; R; b M; has a * 10 m 60° sp, dist 65'' | 91 | | 2291 | II. 10 | 23 50 56'2'' | 76 8 26 | F; S; E; irreg fig; 18'' | 175 | | 2292 | Nova. | 23 51 46'8'' | 40 13 40 | A double * in a tolerable cluster in which is one star 9 m | 207 | | 2293 | Nova. | 23 52 17'5'' | 84 42 9 | v F; S; R; p s b M | 302 | | 2294 | III. 855 | 23 52 42'7'' | 59 31 30 | e F; S; R; s b M; double; the s p of 2 | 178 | | | | 42'8 | 30 27 | e F; very little more than a suspicion, and could not find the object again. [N.B. A diagram made at the time represents the two nebulae in their right position; therefore no doubt but the wire of the transit was mistaken.] | 114 | | | | ... | 30 31 | e F; seen by glimpses in a fog | 104 | | 2295 | III. 856 | 23 52 44'3'' | 59 29 ± | e F; a companion to III. 855; v doubtful. | 114 | | | | 45'5 | 29 57 | e F; b M; like a blurred star | 106 | | | | 46'2 | 31 10 | e F; S; R; s b M | 178 | | No. | Synonym | R 1830°-0. | N.P.D. 1830°-0. | Description and Remarks | Sweep | |-----|---------|------------|----------------|------------------------|-------| | 2296 | H. MS. | h m s 23 53 37·4 | ° 77 58 36" | e F; follows 2 st which point a little s of it. It is called a suspected nebula by my Father in his Sweeps. | 174 | | | | | 39·3 58 31 | "Suspected nebula." Verified; a * 11 m p to n, and another v S, point a little south of it. | 175 | | | | | ... 57 ± | "Suspected nebula." Verified, being found in the middle of the field by setting the telescope on the place per working list; but it is so nearly a star as to be easily mistaken for the third * of a triangle. | 15 | | 2297 | II. 240 | 23 54 32·5 | 74 47 33 | B; L; irreg R; vg b M; 2' or 3' diam; no nucleus. | 11 | | 2298 | III. 436 | 23 55 ± | 83 35 18 | v F; R | 280 | | 2299 | Nova. | 23 55 7·8 | 83 27 45 | v F; p L; R; g b M | 281 | | 2300 | II. 227 | 23 55 16·7 | 70 10 5 | p B; m E; 1b M; 2' l, 20" br; pos 45° n f to s p by diagram. | 91 | | 2301 | Nova. | 23 55 47·5 | 85 44 40 | B; S; m E; vs m b M to a *; 12' l, has a * p | 300 | | | | | ... | Viewed; p F; E; follows a s *; the first and southern of 3 in a line. | 302 | | 2302 | Nova. | 23 56 1·1 | 22 16 20 | The central part of what I am positive is an enormously L, but e F neb of a round figure, though I cannot trace its limits. The night exquisite. I swept often across it to be sure, but always recurred to the same place. No doubt but can never be seen but in the best state of the air and sky. Diam 10' ±. | 223 | | 2303 | Nova. | 23 56 23·5 | 84 1 44 | Not v F; S; R; 12"; a * 9 m n p | 302 | | 2304 | Nova. | 23 56 24·0 | 85 44 14 | v F; S; g b M | 302 | | 2305 | VIII. 29 | 23 56 29·8 | 111 39 39 | A triangular group of about a dozen stars | 293 | | 2306 | Nova. | 23 56 45·5 | 85 43 49 | v F; S; R; s b M; has a * nf | 302 | | 1 | III. 868 | 0 0 2·0 | 86 19 35 | &c. &c. | &c. | **ERRATA AND ADDENDA.** Page 361, line 9, . . . for 2500 read 2300 —— 361 —— 10 . . . for 2000 read 1800 —— 388 Obs. 536 . . . for II. 880 read II. 280 —— 379 —— 344 . . . for PD 52 50 56 read 53 10 56. Omitted Nebula.—R.A. 13h 56m 23s·6; PD 33° 21' 50"; v F; Sweep 546. APPENDIX. The manner in which the observations, whose results are above stated, have been performed, that is to say, the method and order in which the business of a sweep is conducted, having been stated at large in my catalogues of double stars, it will not be necessary to recapitulate the particulars here; but it would not be right for me to lay before the Royal Society the present collection of reduced observations unaccompanied by some explanation of the manner in which the reductions have been executed, and how the numbers here set down as the mean right ascensions and north polar distances of objects for the epoch 1830, are concluded from the numbers registered at the moment of observation, especially since the method actually pursued for this purpose is materially different from that taken to reduce my earlier catalogues of double stars, being at once much more exact, and far less troublesome. This change has of course involved the necessity of a recalculation of all the sweeps which had been reduced on the original plan; and although this has proved a work of considerable labour, the advantage of the adoption of a uniform system throughout the reductions is more than an equivalent for the time and trouble it has cost—not to mention the detection of several errors in particular cases, and the satisfaction of a general verification of the great body of the former computations. Every complete observation registered in the sweeping books contains the following particulars: 1st. The time, shown by a chronometer (of unknown error and rate), when the object passed one or other of the vertical wires of the eye-piece, or finally left the field, after which, though it might be recovered, and viewed and described at leisure, by withdrawing the tube from its bearing against the ladder, yet no further determination of time was practicable, other than a very rude one, by taking the transit of some small star, on the same parallel, and then temporarily fixing the tube in a new position, remote from the ladder, and noting the difference of right ascension between that star and the object, by their transits afresh across the wires so displaced. 2ndly. The wire across which the transit was observed is noted in the next place, and the first step in the process of reduction consists in applying to the observed times of transit a reduction to the first wire, when not directly observed, founded on a knowledge of the interval between the wires and the extent of the range of the field of view, as also of the approximate polar distance of the object. 3rdly. The third datum given by observation is the reading off of the brass sector attached to the end of the tube, by the lateral microscope. The sector is graduated to degrees and minutes, and the seconds are estimated, which is easy, as each minute is nearly a tenth of an inch in length. Though I have no reason to apprehend any error in the graduations, or in the values of the degrees, minutes, &c., into which the arc of this sector is supposed to be divided, both are regarded as unknown elements, whose values, if necessary, might be investigated, but into which, by reason of the system adopted, there is no occasion to inquire, further than to be satisfied that their errors are of an order so small as not to bring into question the identity of an object. These are the data furnished by observation for every object in a complete sweep; and I shall now explain how from these data, compared with the mean places of all those known objects which are to be found in authentic catalogues brought up to a given epoch, and which occur in a sweep, the mean places of all the unknown ones for the same epoch may be obtained, with the greatest degree of accuracy of which the system of observing is susceptible,—without the necessity of taking into direct consideration any uranographical or instrumental correction whatever,—and that in a manner which, as will appear, carries with it a moral certainty of eliminating (so far as they can be eliminated by any process) whatever errors may have been committed in the observations of the zero stars. In fact, if we consider all the corrections which we can possibly have occasion to apply to observations of this kind, whether arising from the uranographical reductions, (viz. precession, aberration, nutation and refraction,) or from instrumental mis-adjustment, such as extrameridional situation of the plane of the sweep, or its deviation from a vertical; error and rate of the chronometer; error of evaluation of the divisions of the sector, &c.; or, lastly, even from instability of the instrument itself, due to hygrometrical or pyrometrical causes, whose operation, though very irregular, is still to a certain extent gradual; we shall find that they are all functions of two quantities,—the time elapsed since a given epoch, or, which comes to the same thing, the sidereal time at the moment of observation; and the inclination to the horizon of the line of collimation, or, which comes to the same, the polar distance of the object. Hence it follows that in all cases the mean R. A. of an object observed must necessarily be derived from the observed chronometer reading, (reduced to the first wire,) by adding to that reading a reduction (R) which is some certain function of these two quantities, and that the mean polar distances, also reduced to the same fixed epoch, will in like manner be had from the reading of the index arc or lateral sector, by adding thereto another reduction (r), which is also a function of the same quantities. We have therefore, if we call \( \alpha \) and \( \varpi \) the mean R. A. and polar distance of any object, \( t \) the time (by chronometer) of its transit over the first wire, and \( i \) the reading of index arc, two equations of this form: \[ \begin{align*} \alpha &= t + \text{funct.}(\alpha, \varpi) \\ \varpi &= i + \text{funct.}(\alpha, \varpi). \end{align*} \] This form, however, is unsuitable to our purpose, the quantities \( \alpha \) and \( \varpi \) being themselves the object of inquiry; but it is easy to give the equations a more available form, if we consider, 1st, that \( \alpha \) and \( \varpi \) are never materially different, the former from \( t \), the latter from \( p + i \), where \( p \) is the polar distance corresponding to \( i = 0 \); and 2ndly, that we intend to have no concern at all with the analytical form of the functions involved, which, so far as our purpose goes, may be regarded as unknown or arbitrary. Denoting then by \( F \) and \( f \), other forms of functions equally unknown with the former, we are at liberty to suppose our equations transformed as follows: \[ \begin{align*} \alpha &= t + F(t, i) \\ \varpi &= i + f(t, i) \end{align*} \] Our attention must now be directed not to discover \textit{à priori}, by theory, the analytical forms of the functions \( F, f \); but, \textit{à posteriori}, from observation, to tabulate their values, or, in other words, to reduce their calculation to a simple process of interpolation between their observed values as concluded from the zero stars. To this end we must put the above equations under the form \[ \begin{align*} F(t, i) &= \alpha - t \\ f(t, i) &= \varpi - i \end{align*} \] and putting $F(t, i) = R$ and $f(t, i) = r$, we must first ascertain the values of $R, r$ from each of the zero stars observed, with the corresponding values of $t$ and $i$ given by observation, and then tabulate them by interpolation, for all the other values within the limits of the sweep. With respect to the first of these operations it is very easy. For in the case of a zero star, $\alpha$ and $\pi$ are given by the standard catalogue, brought up to the given epoch if required, and $t$ and $i$ are the actual readings off of the chronometer and index arc, the former being merely reduced to the first wire, by an appropriate table, when that wire is not observed. The problem then is reduced to this,—given the values $R, R', R''$, and $r, r', r''$, &c., of two functions of $t$ and $i$, of whose analytical form we are ignorant, to interpolate these functions, and tabulate their values for every value of $t$ and $i$ within certain limits. The principle on which this problem may be easiest and most generally resolved, as well as with the highest degree of probability which the case admits, is an extension of the method I have used for interpolating the angles of position of double stars. We may regard $R$ and $r$ as the third or vertical coordinates of two curved surfaces, of which $t$ and $i$ are respectively the first and second or horizontal coordinates. Having, therefore, obtained a number of corresponding values of the three coordinates, we have given so many points in each curve surface, or rather which should lie in such surface were all the observations free from error. Since that, however, is not the case, the surface, such as it theoretically ought to be, did we know its true form, will not pass through but among the points in question; and it must be our care so to describe it as to deviate as little as possible from them while yet preserving a seemly and moderate flexure in itself—at least if we have no reason to believe that jumps exist in the instrumental errors. A graphical process which should require us to describe a curve surface through or among given points in space, would be difficult, but fortunately in the case before us the difficulty may be evaded. For the limits of a sweep in polar distance being only three degrees, the amount of flexure of either of our curve surfaces in the direction of the coordinate $i$ will of necessity be trifling, and may be disregarded. The surface therefore will be one of a cylindroidal nature, in which the ordinate is of the form $\text{funct.}(t) + \text{funct.}(i)$, so that if we denote by $A$, $B$, and $a$, $b$, such functions of these respective variables, we shall have $$R = A + B$$ $$r = a + b$$ where $A$, $a$, are functions of $t$ alone, and $B$, $b$, of $i$ alone. Thus the interpolation of the functions $R$, $r$, is reduced to that of the functions $A$, $B$, $a$, $b$, each of which involving only one independent variable, the precepts given in my paper above alluded to, apply immediately to its interpolation, and enable us to tabulate its value with the greatest readiness. The process which I have used throughout the reduction of the sweeps has been grounded on these principles, and may be thus summarily described. 1st. From the registered chronometer and index reading, compared with the standard catalogue adopted, deduce the reductions, in R. A. and N. P. D. of all the known stars which occur in the sweep, or the zero stars, as I have called them. By the reductions, I mean the quantities in time or in space which must be applied to the observed chronometer or index reading to produce the catalogued R. A. or N. P. D. for the epochs. These are the quantities $R$, $R'$ and $r$, $r'$, &c. 2ndly. Take a piece of paper, divided into squares, either ruled or printed, of which every tenth line in both directions should be stronger than the rest. On this, choosing one direction (suppose the horizontal) for measuring off the values of the independent variable $t$, let the other (the vertical) be devoted to measuring off those of the function $A$ corresponding to those values of $t$: and in this way lay down a series of points on the paper, having $R$, $R'$, &c., for their ordinates and the values of $t$ corresponding, for their abscissas. Through, or among these points, so as to make the least deviations consistent with a gentle and moderate curvature, or, if possible, with a rectilinear form, describe a curve, which may be called the reducing curve in right ascension, for time, and then read off the values of its ordinate $R$, which correspond, not to the observed values of $t$, but to a regular arithmetical or tabular progression of this quantity; for instance, to every tenth, or twentieth, or thirtieth minute, according to the rapidity of its variation. Lastly, enter these readings off of the interpolating curve in a table, which will therefore express the values of the unknown function $A$, and may accordingly be used as a table of reductions in R. A. for that part of the reduction which depends on the time. 3rdly. Suppose $A, A', A'', \ldots$, &c., to be the values of $A$ taken from this table corresponding to the values $t, t', t'', \ldots$, &c., of the time, at the moments of observation of the zero stars; then, since $R = A + B$, we have $B = R - A$, and similarly $B' = R' - A'$, and so on. Thus, then, we get a set of values of $B, B', B'', \ldots$, &c.; and these being in like manner laid down on a paper of engraved squares, and an interpolating curve drawn, read off, and tabulated as in the case of $A$, we get a table of values of $B$ to be used for that part of the reduction in R. A. which depends on the index arc. These tables once constructed, we may apply them immediately to the reduction of all the observations of unknown objects in R. A. which were made on the first wire. But for those made on the second, or at leaving the field, a further correction will be required, viz. the interval between the wires, to be applied negatively to the observed chronometer reading. This correction is of the form $c \cdot \text{cosec } \varphi$, or $c \cdot \text{cosec } (p + i)$, where $p$ is the polar distance of the top or zero of the sweep. By numerous observations made for the purpose, I have determined the value of $c$ in my eye-piece as follows: - for the second wire, $c = 31^\circ 09$; - for the final exit from the field, $c = 58^\circ 69$. In order, however, to avoid the trouble of making this subtraction, as a separate operation, for all the unknown objects which happen to have been observed under these circumstances, it is preferable to construct three independent tables of $B$ (with which this correction, depending on $i$, unites itself,) to be used for observations made on the first or second wire, or at the exit from the field, which we shall denote by $B^1, B^2, B^3$. To reduce the index readings to polar distances, for the adopted epoch, a process exactly similar must be used for determining $a$ and $b$. A table of $a$ being first constructed, the equation $b = r - a$ gives us the means of interpolating and tabulating the values of $b$. In this case, however, there is no occasion to form tables for the other wires, the bisection of the object by the horizontal wire being alike in all parts of its passage through the field, except within a degree or two of the pole. To reduce a sweep, then, in the most general case, we require six tables, viz. two for the values of $A$, $a$, whose argument is the registered time, per chronometer, and four for $B^1$, $B^2$, $B^3$, and $b$, having the index reading for their argument. The construction of these tables in the manner described, and their application when constructed, is attended with very little difficulty, when once the computer is accustomed to the construction and reading off of the interpolating curves. In most cases, however, the value of $A$ is so nearly constant, that its variation (in such observations as these) may be neglected: whenever this is the case, the table for interpolating $A$ may be suppressed, and its constant value simply added to those of $B^1$, $B^2$, $B^3$, which are always required. It is therefore advisable universally to regard $B^1$, $B^2$, $B^3$, as containing the constant part of $A$, by which procedure all occasion of mistake arising from change of method is taken away. Most usually also the value of $B^1$, so increased by the constant part of $A$, is the same throughout the limits of the sweep. When this is not the case, it is ordinarily owing either to extrametrical situation of the telescope, or to rapid hygrometrical changes, or lastly, to wind. But with its causes we have no concern, further than to endeavour to reduce its amount when inconveniently great, by a motion of the instrument in azimuth. The values of $a$ are liable, as I have found by experience, to considerable fluctuations, and that in very variable degrees at different epochs of the observations. Hygrometrical changes have some influence: but by far the worst, and most intractable part of these fluctuations appears to have taken its rise from the shifting of the line of collimation, owing to the mirror taking a new bearing in its cell. I regret that I did not earlier perceive this cause of error. It has only recently occurred to me, and the remedy almost at the same instant suggested itself in a simple, and what I trust will hereafter prove an effectual application of the collimating principle of Rittenhouse and Kater. It consists in attaching to the inside of the wooden tube of the reflector a small achromatic telescope, having its object-glass turned towards the speculum, and its eyend projecting at right angles to the axis of the tube through an aperture in the side, the cone of rays being deflected outwards at a right angle by a small mirror $45^\circ$ inclined to its axis. In the focus of the object-glass, (thus rectangularly deflected,) is fixed a cross of fine spider-lines, strongly illuminated by a lamp (capable of being shut off when not wanted), which also serves to illumi- nate the field. The cross is so situated that its image, seen in the telescope as an object infinitely distant, (according to the principle of the collimator,) makes with all its arms, angles of $45^\circ$ with the horizontal and vertical wires of the sweeping eye-piece. In the beginning of a sweep, the intersections of both crosses are brought to exact coincidence (by a method presently to be explained); and it is evident that if in the progress of the sweep the slightest shifting of the mirror in its cell should produce a motion of the line of collimation, it cannot fail to be detected by the apparent recess of the two crosses from their original common intersection. A relative motion, to the amount of two seconds of space, either laterally or vertically, cannot possibly escape detection, as I have convinced myself by many trials; and so satisfactory has this mode of overcoming the difficulty in question proved, that I have no hesitation in saying that the only obstacle to the use of large reflectors for the nicer purposes of exact theoretical astronomy, (viz. the error caused by the shifting of the mirrors in their cells, by reason of their great weight, and the danger of securing them by strong pressure,) has ceased to exist*. It is not, however, sufficient to have the means of readily detecting error, without possessing that of correcting it with equal readiness, or at least measuring its amount. A very simple and effectual contrivance accomplishes this. The two adjusting screws by which the mirror case is supported against the bottom of the tube are terminated, outside of the latter, by large disks or wheels of wood about six inches in diameter, grooved at their edges. Round these, re-entering cords are conducted over pulleys, to a convenient point within reach at the mouth of the tube, forming a kind of reins, which hang loose when not in use, but by tightening or drawing one or other of them, any motion, however large or * My first collimator consisted of a small object-glass, by Fraunhofer, of about one inch and a half in diameter, and twelve inches focus. When applied to the twenty-feet reflector, as described in the text, it formed an admirable microscope with its full aperture,—an extraordinary proof of the perfection of its construction, this being doubtless the severest test to which an achromatic object-glass can be possibly subjected. The most beautiful object I can remember to have seen in telescopes was Jupiter entering, perfectly defined, and with all the appearance of a real globe, into the image of a small glass globule, placed in the focus of the collimating telescope. It seemed like the mutual penetration of two solids, or rather two essences of different natures, the one bright and ethereal, the other dark and adamantine. This most exquisite specimen of workmanship was destroyed by an accident. That with which I have been forced, temporarily, to replace it, bears no comparison with the original. minute, may be given to the line of collimation at pleasure. By the aid of this mechanism, the perfect adjustment of the line of collimation (to the full extent of the optical powers of the instrument,) is performed in an instant, and may, if we please, be repeated at every observation, being attended with no trouble. Nay, the line of collimation may be purposely deranged to any extent, and immediately corrected. So that by graduating the grooved disks, and adopting an index to each, a very complete distance and position micrometer for the measurement of double stars might be formed, in which, if necessary, two lucid points might imitate the two stars to be compared. To return, however, from this digression, and to illustrate by an example what is here said of the method of sweeping, we may take that of sweep 384, in which the zero stars run as follow: | No. | Name of Star | Observed Chronometer | Wire | Observed Index | |-----|-------------------|----------------------|------|----------------| | 9 | Piazzi, xxi. 383 | 21 57 5·0 | 1 | 1° 5′ 30″ | | 13 | 3 Lacertae | 22 18 23·5 | 1 | 0 25 0 | | 22 | P. xxii. 276 | 22 53 21·0 | 1 | 0 25 30 | | 29 | P. xxiii. 73 | 23 17 25·0 | 1 | 2 7 45 | | 31 | P. 0. 70 | 0 46 22·0 | 2 | 0 47 35 | | 41 | P. i. 130 | 1 30? 57·0 | 2 | 2 1 30 | | 49 | 4 Persei | 1 52 42·5 | 1 | 2 40 50 | | 60 | P. ii. 115 | 2 26 44·5 | 1 | 0 14 30 | | 65 | γ Persei | 2 54 9·5 | 1 | 1 51 15 | | 79 | P. iv. 7 | 4 5 8·5 | 1 | 2 12 0 | | 83 | 1 Camelop | 4 21 8·5:: | 2 | 2 32 40 | | 84 | 2 Camelop | 4 28 9·0 | 1 | 2 8 0 | By comparing the observations with Piazzi's catalogue brought up to 1830·0, and with that of the Astronomical Society for the same epoch, we get the following values of $R$, $r$. Constructing now an interpolating curve to pass among a series of points laid down from the chronometer readings taken as abscissæ, and the values of $R$ as ordinates, we get the following Table of $A$, by inspection of the course of the curve, as read off upon the squares of the interpolating chart. Taking out now from this Table the values of $A$ corresponding to the times of observation, and subtracting them from those of $R$, we find the following for the interpolated residues or values of $B^{(1)}$. Laying these down in like manner on a divided chart, we get the interpolated values of $B^{(1)}$ as in the following Table, beside which are also annexed those of $B^{(2)}$ and $B^{(3)}$, obtained by adding to $B^{(1)}$ the corresponding values of $-31^\circ 09'$ cosec $(39^\circ - i)$, and $-58^\circ 69'$. cosec $(39^\circ - i)$; $39^\circ - i$ being the approximate polar distance of any object in the sweep in lieu of $39^\circ + i$, because the telescope is directed between the zenith and pole, where $i$ is taken negatively. | $i =$ | $B^{(1)}$ for 1st Wire. | $B^{(2)}$ for 2nd Wire. | $B^{(3)}$ for leaving Field. | |-------|------------------------|------------------------|-----------------------------| | 0° | +0 3·1 | -0 46·3 | -1 30·2 | | 20° | +0 2·5 | 47·3 | 31·6 | | 40° | +0 1·8 | 48·3 | 32·9 | | 1° | +0 1·2 | -0 49·3 | -1 34·2 | | 20° | +0 0·5 | 50·3 | 35·6 | | 40° | -0 0·2 | 51·4 | 37·0 | | 2° | -0 0·8 | -0 52·5 | -1 38·3 | | 20° | -0 1·4 | 53·5 | 39·7 | | 40° | -0 2·1 | 54·5 | 41·1 | | 3° | -0 2·7 | -0 55·6 | -1 42·6 | A process exactly similar being gone through for $a$ and $b$, we find $b = 0$, and for $a$, the following Table. | $t =$ | $a =$ | $t =$ | $a =$ | |-------|-------|-------|-------| | h m s | h m s | h m s | h m s | | 21 0 | 39 2 | 8 | 1 0 | | 22 0 | 1 59 | 2 0 | 1 24 | | 23 0 | 1 51 | 3 0 | 1 10 | | 0 0 | 1 43 | 4 0 | 0 55 | | 1 0 | 39 1 | 34 | 5 0 | | | 39 0 | 36 | | These Tables constructed, all we have to do to reduce the whole series of objects comprised in the sweep (89 in number), is to take out from them, by proportional parts, the quantities corresponding to the registered time and index, and apply them with their proper signs. Thus, for example, the star $\Sigma$. 446 in the cluster VIII. 80, which is No. 308 of the general series in this paper, was observed in this sweep as follows: | No. | Chronometer. | Wire. | Index. | |-----|--------------|-------|--------| | 73 | h m s | 1 | 9 0 | | | 3 38 14·0 | | | And the process of reduction stands as follows: | Chronom. | h m s | |----------|-------| | A | -0 1 38·7 | | B(1) | +0 0 0·8 | | R. A. 1830·0 | =3 36 36·1 | | Index | h m s | |-------|-------| | | -1 9 6 | | a | +39 1 0 | | N. P. D. 1830·0 | =37 52 0 | With regard to the limits of probable error in the determination of places of such objects as have been only once observed, and which therefore admit of no check by the context, it may be right to say a few words. I consider the probable error of a single good observation, free from mistakes in the readings and reductions, and occurring in a tolerably regular sweep, in which the zero stars are in sufficient number, not to exceed a second and a half of time in R. A. and 30" in P. D. Mistakes, however, will unavoidably occur in the wire observed, in the minute of time (owing to misadjustment of the chronometer hand), and in the numerical process of reduction. All these are sure to be detected, and are easily corrected, when two or more observations of an object exist; but when one only has been obtained, it remains liable to them all. I can only hope that such cases are not numerous. There is, however, one mode in which a mistake in the R. A. may arise, not so easily detected, and which though of rare occurrence, has certainly been committed occasionally, and has no doubt been the cause of some, if not all, the very bad discordances between right ascensions determined in different sweeps. This is when the position wire of the micrometer, having been left in a direction nearly parallel to the meridian, has been mistaken for one of the fixed wires of the eye-piece, and the transit of the object over this, registered, in lieu of its passage across the true first or second wire. The error thus produced may be of any amount less than the interval of the wires, and though habitually guarded against by setting the position wire obliquely after reading off, has evidently crept in, in some few cases, by the neglect of this precaution. With respect to the discrepancies, and apparent contradictions, which will be found in the descriptions of one and the same nebula in different sweeps, they are to be accounted for by differences in the states of the atmosphere, the mirror, and the eye, and will not appear at all surprising to any one accustomed to observation of this nature. At the same time they will serve to show what caution we ought to use in admitting such discordances between descriptions of different observers furnished with different telescopes, as evidences of real changes in any nebula. MDCCCXXXIII. Explanation of the Plates, with a List of the Nebulae figured in this Paper. | Plate | Figure | |-------|--------| | IX. | 1...6 | | | Figures illustrative of degrees of brightness. Fig. 1. eF; Fig. 2. vF; Fig. 3. F; Fig. 4. pB; Fig. 5. B; Fig. 6. vB. | | | 7...12 | | | Figures illustrative of degrees of central brightness. Fig. 7. vl bM; Fig. 8. l b M; Fig. 9. b M; Fig. 10. p m b M; Fig. 11. m b M; Fig. 12. v m b M. | | | 13...18| | | Figures illustrative of gradations of brightness from without inwards. Fig. 13. vg b M; Fig. 14. g b M; Fig. 15. b M; Fig. 16. p m b M; Fig. 17. m b M; Fig. 18. v m b M. | | | 19...24| | | Figures illustrative of degrees of elongation of form. Fig. 19. vl E; Fig. 20. l E; Fig. 21. E; Fig. 22. p m E; Fig. 23. m E; Fig. 24. v m E. | List of figured Nebulae. | Plate | Figure | Number in Observations | Synonyms | R. A. | N. P. D. | |-------|--------|------------------------|----------|-------|---------| | X. | 25 | 1622 | M. 51 | 13 22 39 | 41 56 | | | 26 | 2060 | M. 27 | 19 52 12 | 67 44 | | | 27 | 1486 | M. 64 | 12 48 23 | 67 23 | | | 28 | 218 | V. 19 | 2 11 58 | 48 25 | | | 29 | 2023 | M. 57 | 18 47 13 | 57 11 | | | 30 | 2002 | Nova | 18 7 1 | 109 56 | | | 31 | 311 | IV. 69 | 3 58 36 | 59 40 | | | 32 | 838 | M. 97 | 11 4 49 | 34 4 | | XI. | 33 | 2088 | V. 15 | 20 38 39 | 59 54 | | | 34 | 2092 | V. 14 | 20 49 20 | 58 57 | | XII. | 35 | 2008 | M. 17 | 18 10 45 | 106 15 | | | 36 | 368 | M. 78 | 5 38 2 | 90 1 | | | 37 | 1357 | V. 24 | 12 27 53 | 63 5 | | XIII. | 38 | 112 | II. 252 | 1 15 0 | 77 59 | | | 39 | 1649 | II. 297 | 13 28 53 | 107 1 | | | 40 | 731 | IV. 60 | 10 28 7 | 35 37 | | | 41 | 1456 | M. 94 | 12 42 52 | 47 57 | | | 42 | 1989 | Nova | 17 44 43 | 66 53 | | | 43 | 2051 | IV. 73 | 19 40 19 | 39 54 | | | 44 | 2098 | IV. 1 | 20 54 53 | 102 2 | ## List of figured Nebulæ.—Continued. | Plate | Figure | Number in Observations | Synonyms | R. A. | N. P. D. | |-------|--------|------------------------|----------|-------|---------| | XIII. | 45 | 2241 | IV. 18 | 23 17 44 | 48 24 | | | 46 | 2047 | IV. 51 | 19 34 21 | 104 33 | | | 47 | 2075 | IV. 16 | 20 14 48 | 70 26 | | | 48 | 2072 | IV. 13 | 20 9 33 | 59 57 | | | 49 | 355 | I. 261 | 5 20 11 | 55 54 | | XIV. | 50 | 1376 | I. 43 | 12 31 11 | 100 40 | | | 51 | 859 | V. 8 | 11 11 22 | 75 28 | | | 52 | 61 | V. 1 | 0 39 12 | 116 13 | | | 53 | 854 | M. 65 | 11 10 2 | 75 59 | | | 54 | 875 | Nova | 11 14 12 | 76 5 | | | 55 | 1175 | V. 43 | 12 10 33 | 41 46 | | | 56 | 242 | I. 156 | 2 29 46 | 51 41 | | | 57 | 1235 | I. 210 | 12 15 6 | 42 4 | | | 58 | 151 | IV. 42 | 1 40 4 | 84 56 | | | 59 | 1148 | I. 109 | 12 7 15 | 75 54 | | | 60 | 2236 | II. 600 | 23 13 58 | 50 4 | | | 61 | 536 | II. 280 | 8 45 50 | 92 25 | | | 62 | 1499 | IV. 30 | 12 50 57 | 54 13 | | | 63 | 2205 | I. 55 | 22 56 26 | 78 36 | | | 64 | 399 | IV. 2 | 6 29 53 | 81 7 | | | 65 | 537 | IV. 66 | 8 46 33 | 35 35 | | | 66 | 1362 | III. 602 | 12 28 28 | 74 48 | | | 67 | 1509 | I. 143 | 12 52 2 | 86 35 | | XV. | 68 | 1252 | V. 29 | 12 17 22 | 55 31 | | | 69 | 1202 | {M. 61} | 12 13 13 | 84 35 | | | | | {I. 139} | | | | | 70 | 604 | I. 56 & 57 | 9 22 32 | 67 45 | | | 71 | 1146 | I. 95 | 12 7 5 | 52 44 | | | 72 | 444 | II. 316 & 317 | 7 14 50 | 60 11 | | | 73 | 2197 | II. 450. 451 | 22 51 12 | 103 43 | | | 74 | 1408 | M. 60. III. 44.. | 12 35 4 | 77 31 | | | 75 | 1414 | I. 176. 177 .. | 12 35 39 | 56 54 | | | 76 | 1397 | V. 42. II. 659 .. | 12 33 54 | 56 30 | | | 77 | 1905 | II. 751. 752 .. | 15 0 0 | 69 48 | 382 ### List of figured Nebulæ.—Continued. | Plate | Figure | Number in Observations | Synonyms | R. A. | N. P. D. | |-------|--------|------------------------|----------|-------|---------| | XV. | 78 | 1358 | Nova ..... | 12 27 55 | 77 49 | | | 79 | 936 | II. 103 ....... | 11 31 24 | 73 43 | | XVI. | 80 | 1991 | IV. 41 ....... | 17 52 0 | 113 1 | | | 81 | 357 | M. 1 ......... | 5 24 16 | 68 7 | | | 82 | 2093 | Nova ....... | 20 50 4 | 60 26 | | | 83 | 1352 | I. 92 ......... | 12 27 31 | 61 6 | | | 84 | 1466 | II. 75 & 74 .... | 12 44 21 | 77 50 | | | 85 | 2245 | II. 226 ....... | 23 19 58 | 68 31 | | | 86 | 1968 | M. 13 ......... | 16 35 37 | 53 13 | | | 87 | 1916 | M. 5 ......... | 15 9 56 | 87 16 | | | 88 | 2125 | M. 2 ......... | 21 24 40 | 91 34 | | | 89 | 1929 | Nova ....... | 15 29 9 | 83 27 | | | 90 | 2128 | M. 30 ......... | 21 30 42 | 113 55 | | | 91 | 415 | VI. 2 ......... | 6 45 18 | 71 49 | **Notes on the foregoing List.** Fig. 25. M. 51.—This very singular object is thus described by Messier:—"Nébuleuse sans étoiles." "On ne peut la voir que difficilement avec une lunette ordinaire de 3½ pieds." "Elle est double, ayant chacune un centre brillant éloigné l'un de l'autre de 4' 35''. Les deux atmosphères se touchent." By this description it is evident that the peculiar phenomena of the nebulous ring which encircles the central nucleus had escaped his observation, as might have been expected from the inferior light of his telescopes. My Father describes it in his observations of Messier's nebulae (which are not included in his catalogues,) as a bright round nebula, surrounded by a halo or glory at a distance from it, and accompanied with a companion; but I do not find that the partial subdivision of the ring into two branches throughout its south following limb was noticed by him. This is, however, one of its most remarkable and interesting features. Supposing it to consist of stars, the appearance it would present to a spectator placed on a planet attendant on one of them eccentrically situated towards the north preceding quarter of the central mass, would be exactly similar to that of our Milky Way, traversing in a manner precisely analogous the firmament of large stars, into which the central cluster would be seen projected, and (owing to its greater distance) appearing, like it, to consist of stars much smaller than those in other parts of the heavens. Can it, then, be that we have here a brother-system bearing a real physical resemblance and strong analogy of structure to our own? Were it not for the subdivision of the ring, the most obvious analogy would be that of the system of Saturn, and the ideas of Laplace respecting the formation of that system would be powerfully recalled by this object. But it is evident that all idea of symmetry caused by rotation on an axis must be relinquished, when we consider that the elliptic form of the inner subdivided portion indicates with extreme probability an elevation of that portion above the plane of the rest, so that the real form must be that of a ring split through half its circumference, and having the split portions set asunder at an angle of about $45^\circ$ each to the plane of the other. Fig. 26. Mess. 27.—Described by Messier thus: "Nébuleuse sans étoile." "On la voit bien avec une lunette ordinaire de $3\frac{1}{2}$ pieds: elle parait sous une forme ovale et ne contient aucune étoile." In my Father's observations the true form (like that of a double-headed shot or dumb-bell,) was of course distinctly perceived, and the small stars it contains are noticed, and taken as an indication of its resolvability. I incline, however, to the opinion of their being accidental stars (of which multitudes exist in the surrounding region). But here, as in the former object, the feature which gives a peculiar interest to the whole nebula, and alters entirely the light in which its physical constitution must be considered, has been hitherto overlooked,—I mean the faint nebulosity which fills in the lateral concavities of the body, and converts them in fact into protuberances, so as to render the general outline of the whole nebula, a regular ellipse, having for its shorter axis the common axis of the two bright masses of which the body consists, that is to say, the longer axis of the oval form, under which it was imperfectly seen by Messier. To this axis the complete figure is symmetrical, and if we are disposed to regard it as a mass in rotation, it is about this axis that we must suppose it to revolve. In that case its real form must be that of an oblate spheroid; and as it does not follow that the brightest portions must of necessity be the densest, this supposition would not be incompatible with dynamical laws, at least, supposing its parts to be capable of exerting pressure on one another. But if it consist of discrete stars, this cannot be admitted, and we must have recourse then to other suppositions to account for the maintenance of its form. Fig. 27. Mess. 64.—The dark semi-elliptic vacancy (indicated by an unshaded or bright portion in the figure,) which partially surrounds the condensed and bright nucleus of this nebula, is of course unnoticed by Messier. It was however seen by my Father, and shown by him to the late Sir Charles Blagden, who likened it to the appearance of a black eye, an odd, but not inapt comparison. The nucleus is somewhat elongated, and I have a strong suspicion that it may be a close double star, or extremely condensed double nebula. Fig. 28. V. 19.—An extraordinary object. Perhaps the representation in the figure is too nicely symmetrical, as it certainly is too sharply defined and distinct. It is of the last degree of faintness, and may very well be unperceived, though full in the field of view. There can hardly be a doubt of its being a thin flat ring, of enormous dimensions, seen very obliquely. Fig. 29. Mess. 57.—The annular nebula in Lyra. It is ill represented. The edges exhibit a curdled and confused appearance, like stars out of focus. The interior is far from absolutely dark. It is filled with a feeble but very evident nebulous light, which I do not remember to have seen noticed by former observers. Comparing figures 25, 27, 28, 29 and 48, it will appear that the annular form, or an approach to it, is one of those which nebulæ affect, and taken in connexion with the ring of Saturn and the Milky Way, may lead us to conceive that some kind of analogy, however obscure, may subsist in all those cases. Fig. 33.—The engraving represents this very strange nebula much too intense. It is an extremely faint object. The large double star is k Cygni. Fig. 35. Mess. 17.—The figure of this nebula is nearly that of a Greek capital omega Ω, somewhat distorted and very unequally bright. It is remarkable that this is the form usually attributed to the great nebula in Orion, though in that nebula I confess I can discern no resemblance whatever to the Greek letter. Messier perceived only the bright preceding branch of the nebula now in question, without any of the attached convolutions which were first noticed by my Father. The chief peculiarities which I have observed in it are, 1st, the resolvable knot in the following portion of the bright branch, which is in a considerable degree insulated from the surrounding nebula; strongly suggesting the idea of an absorption of the nebulous matter; and 2ndly, the much feebler and smaller knot at the north preceding end of the same branch, where the nebula makes a sudden bend at an acute angle. With a view to a more exact representation of this curious nebula, I have at different times taken micrometrical measures of the relative places of the stars in and near it, by which, when laid down as in a chart, its limits may be traced and identified, as I hope soon to have better opportunity to do than its low situation in this latitude will permit. Fig. 37. V. 24, and Fig. 50. I. 43.—The strong suspicion of a parallel appendage to the latter of these, is almost converted into certainty by its undoubted existence in V. 24, in which it was seen by two other observers as well as by myself. But what are we to make of such an appendage? Must we consider it as an extreme exaggeration of the case of M. 64 (fig. 27), in which the vacancy is extended up to almost the very extremities of the elliptic outline,—in which case the nebula would come to be regarded as a flat annulus seen at a great obliquity, and having very unequal breadths and densities in its two opposite semicircles? Or must we admit the appendage to be a separate and distinct nebula, dependent, by some unknown physical relation, on its brighter neighbour? Fig. 43.—This remarkable object, as my Father rightly observes, appears to constitute a connecting link between the planetary nebulæ and nebulous stars. It differs from the latter class of objects in respect of the intensity and comparatively sharp termination of the surrounding light; and no less from the former, in that of its stellar centre. With regard to nebulous stars generally, I ought to mention that it has frequently occurred to me to notice a peculiar state of the atmosphere in which all large stars (above the 7th magnitude) have appeared surrounded with photospheres of 2' or 3' or more in diameter, precisely resembling that about some of the finer specimens of nebulous stars. The state of the air alluded to, is not that in which fog, or any degree of haziness, or thin strata of cloud are perceptible to the sight. These produce no such appearance. Stars are seen through fog, cloud, or ordinary haze, pre- cisely as if there were no such intervening medium; only less bright. The photospheres in question are often seen when the sky seems quite pure and clear. They do not arise from dew on the glasses, as is proved by wiping them; nor in the eye itself, for they do not vanish when the star is made to blink behind one of the thick wires of the eye-piece; nor in scabrous polish of the mirror, for they are not permanent. They come on suddenly; seldom last very long, and disappear as unexpectedly as they come. When first this phenomenon presented itself, a considerable star which appeared so surrounded was at once set down as a superb nebulous star, and it was not until another and another entered the field similarly affected, that any doubt arose. As regards the true cause of this phenomenon, that it is atmospheric I have no doubt, and perhaps it must be looked for in some highly rarified material, disseminated in cloud-like, though invisible, masses, in the very highest regions of our atmosphere,—the same possibly which, when ignited by the passage of electric currents, gives rise to many if not all the phenomena of the aurora borealis. Be that as it may, the fact that an appearance, exactly resembling that of a nebulous star, may originate in a non-luminous medium, interposed between the eye and the star, serves to render it not improbable that such matter may exist, disseminated through the ether itself in determinate localities, and may render some stars which shine through it nebulous, which have no real nebulous atmospheres about them. The frequency of nebulous stars in the constellation of Orion seems to afford some support to this idea, though I am far from contending that there are no stars really nebulous. Of such the object immediately under consideration, indeed, must be regarded as an undoubted instance. Figs. 44 . . . 47.—Planetary nebulæ. The point to which I should here draw attention is the frequent and close proximity to these objects, of minute stars, which suggest the idea of accompanying satellites. Such they may possibly be. The enormous magnitude of these bodies, and consequent probable mass (if they be not hollow shells), may give them a gravitating energy, which, however rare we may conceive them to be, may yet be capable of retaining in orbits, three or four times their own diameter, and in periods of great length, small bodies of a stellar character. In this point of view a continued series of the angles of position of their companions, micrometrically measured with due care, would be interesting; and I regret not having sufficiently attended to this in my observations, the few measures given, being hurried, imperfect and discordant. Plate XIV. Figs. 50...67.—Long nebulæ. The general form of elongated nebulæ is elliptic, and their condensation towards the centre is almost invariably such as would arise from the superposition of luminous elliptic strata, increasing in density towards the centre. In many cases (as in fig. 53,) this increase of density is obviously attended with a diminution of ellipticity, or a nearer approach to the globular form in the central than in the exterior strata. It is probably owing to this, that extended nebulæ seen in dull or hazy states of the sky are often described as round, the fainter and more elliptic envelopes being obliterated, and only the more globular nuclei perceived. The great extension of some nebulæ into long lenticular rays, and the existence of every intermediate degree of ellipticity up to the exact circular form, with the various degrees of rapidity of central condensation, from a barely perceptible increase of density to a seemingly solid nucleus, are all accounted for by supposing the general constitution of these nebulæ to be that of oblate spheroidal masses of every degree of flatness from the sphere to the disc, and of every variety in respect of the law of their density and ellipticity towards the centre. It would be incorrect, however, to draw from this any inference as to the identity of the forces which maintain them in this form with those which determine the oblate spheroidal form of a revolving fluid mass under the dominion of the law of gravitation, and subject to compression by the superincumbent matter. If a nebula be nothing more than a cluster of discrete stars, (as we have every reason to believe, at least in the generality of cases,) no pressure can be propagated through it; and its equilibrium, or, to speak more correctly, the permanence of its form, must be maintained in a way totally different. In a system so constituted, no general rotation of the whole, as a mass, can be supposed. It must rather be conceived as a quiescent form, comprising within its limits an indefinite multitude of individual constituents, which, for aught we can tell, may be moving one among the other, each animated by its own inherent projectile force, and deflected into an orbit more or less complicated, by the influence of that law of internal gravitation which may result from the compounded attractions of all its parts. I have MDCCCXXXIII. shown elsewhere* how a quiescent spherical form may subsist as the bounding outline of an immense number of equal stars uniformly distributed through its extent, each of which individually attracts all the others with a force inversely as the square of the distance, and whose united attractions compose an internal force on each, directly proportional to the distance from the centre of the sphere. In such a state of things, each star might describe an ellipse in any plane, and in any direction in that plane about the common centre, without the possibility of collision; but the sphere, regarded as a whole, would have no rotation about any axis. If the form be not spherical, and the distribution of the stars not homogeneous, the dynamical relations become too complicated to be distinctly apprehended, yet we may still conceive that something of an analogous result may subsist, and that both the external form and the internal density may be maintained (at least under certain conditions,) for the mass as a quiescent whole, while all its elements are in a state of unceasing transfer and interchange. Plate XV. Figs. 68 . . . 79.—Double nebulæ. All the varieties of double stars, as to distance, position and relative brightness, have their counterparts in double nebulæ; besides which, the varieties of form and gradation of light in the latter afford room for combinations peculiar to this class of objects. The series of figures expressed in this Plate exhibits a considerable number of these combinations; and it will, I think, be found impossible, on casting our eye over its contents, and referring mentally to the great number of similar objects scattered through the heavens, to refuse our assent to the idea of a more intimate physical relation between the individuals of a double nebula than that of mere casual juxtaposition. The argument drawn from the comparative rarity of the objects in proportion to the whole extent of the heavens, so cogent in the case of the double stars, is infinitely more so in that of the double nebulæ. Nebulæ, for example, so large and faint, and so little condensed towards the centre as those of V. 29, (fig. 68,) are extremely rare, even single, so that the improbability of two such, casually occurring, so near together as to mix their nebulosities, is extreme. It will therefore become a very interesting subject of future inquiry, whether any traces of orbital motion (indicated by a progressive change in their angles of position with respect to the meri- * Cabinet Cyclopædia, Astronomy, last page. dian,) can be detected in these combinations. The micrometrical measures of many of them which occur in the foregoing observations, though neither so numerous nor so accurate as might be wished, will at least serve as terms of rough comparison, sufficient at least for the detection of rapid rotations. Plate XVI. Figs. 80, 82, 83, 84, 85 represent nebulæ which offer some remarkable peculiarity of situation with respect to stars. Of these the most singular are IV. 41, (fig. 80,) and that of fig. 82. The latter, however, is very imperfectly expressed in the drawing. Indeed it would be excessively difficult to execute a drawing of such an object with any pretensions to correctness. In this, general resemblance and character only has been aimed at, enough to express the peculiar feature of the object, which is a network or tracery of nebulæ following the lines of a similar network of stars. It is an extremely faint and difficult object, and only once observed; but I do not think it possible I could have been deceived as to the reality of the phenomenon, especially since the brighter parts of the nebula are stated in the observation to have been distinctly seen. Figs. 81, 86, 87, 88, 89, 90, 91 are clusters of stars, beginning with a barely resolvable one, (M. 1. fig. 81,) and ascending by successive degrees,—figs. 89, 88, 87,—to M. 13, fig. 86, which is one of the most magnificent assemblages of stars the heavens contain. They are instructive, exhibiting, as they do, an analysis of the intimate structure of nebulæ, on which depend many of the peculiarities of their appearance when no stars can be actually discerned in them, such as, for example, that peculiar character to which, when it has occurred, the epithet "hairy" or "filamentous" has been attached in the descriptions, and which is well illustrated by the figure (fig. 86) of Messier's 13th, and by the description of the 53rd of the Connaissance des Tems (No. 1558 in the above observations,) as set down in sweep 63; the border, instead of melting away insensibly, having a ragged or fibrous appearance. Again, fig. 90, if removed far enough to lose the stars, would be described, doubtless, as irregularly round or unsymmetrical, if not as having a bifid or forked tail: and fig. 91 (VI. 2,) would, under similar circumstances of removal, appear as a fan-shaped nebula with a bright point like a star at the vertex, such as is represented in figs. 65, 66, 67, 68. Before terminating this Appendix, it should be explained what is meant by the references, so frequent in the observations, to a "working list." It has been my invariable practice to prepare before each night's sweep a list, in order of R.A. with approximate polar distances, of the principal objects occurring within the zone intended to be embraced in the sweep, and about 5' or 10' above and below it. It is needless to mention that the nebulæ of these lists were mostly those of my Father's sweeps,—not, however, as taken merely from his printed catalogue, in which only references of their places to the nearest large stars are stated, but as reduced and digested (with great patience and care) into a regular catalogue in zones, by my aunt, Miss Caroline Herschel. This valuable MS., which performs the same office with regard to my Father's sweeps, as far as concerns the places of the nebulæ, as the present digested and reduced series of observations does to my own, has therefore been, in point of fact, the groundwork of my whole proceedings, and I should be not only ungrateful, but in a high degree unjust, were I to omit in this place acknowledging the advantage I have derived from its use. At the commencement of my sweeps, I contented myself, however, with a bare notice of the chief expected nebulæ, but finding that owing to the interest excited by these objects, the zero stars were too much neglected, and smaller nebulæ missed, these came to be inserted at convenient intervals. Subsequently, too, the double stars of Struve's catalogue began to be entered on the lists; and at length, experience having shown me that no trouble bestowed on the construction of an ample and exact "working list" could be considered ill bestowed, I threw aside all the earlier lists of this sort, and dividing the heavens into zones of polar distance, of $3^\circ$ in breadth from $0^\circ$ to $120^\circ$, proceeded to construct a series of lists or approximate catalogues in order of R.A. for 1830, in which should be comprised the following objects: 1st. All my Father's nebulæ and clusters. 2nd. Messier's ditto. 3rd. All other nebulæ and clusters of which any hints could anywhere be found, including new ones from my own sweeps, inserted from time to time. 4th. All the double stars of Struve's greater catalogue. 5th. All other remarkable double stars of which any record could be found, either in my own sweeps or elsewhere. 6th. A series of zero stars, chosen so as to interfere as little as possible with the other objects, and selected from the catalogue of the Astronomical Society; or where none fit for the purpose could be found there, from Piazzi's; or failing that, from other authorities. The construction of the "working lists" on this extended scale, has formed a very large part of the regular work of my sweeps; but so far from regretting the trouble they have cost, or regarding it as waste labour, I can only lament having deferred their full execution till impressed by the experience of much more, and far more valuable observing time lost, with a sense of their importance. One consequence of the construction of the working lists has been the gradual accumulation of a pretty extensive catalogue of missing nebulæ;—perhaps it would be more correct to say, nebulæ not found when looked for. The fainter nebulæ are so easily overlooked, even when in the field of view, and are altogether such very delicate objects, that it is the most difficult thing in the world to prove the negative proposition as to their existence. Many such cases, too, must have originated in mistaken entries on the list, some doubtless in mistakes in the observations from which those lists were constructed, and some from actually looking in the wrong places by mistaken settings of the telescope. Aware of all these possibilities, I have thought it best to suppress this list for the present, having had no time to go into an examination of the subject. Indeed I doubt whether it would be worth while to do so. There seems very little probability that a real nebula should have disappeared from the heavens; and though some few telescopic comets may have been noticed in my Father's sweeps, and set down as nebulæ, the chances are almost infinite against any such observation, if ascertained, proving of use as a datum for improving the elements of any recorded comet.