80 Observations of Nebule and Clusters of Stars. 
G. C. | h. & H. | —— 
1950 IV. 79 | 1871, May 21. <A most extraordinary object, at least 10’ in length, and crossed 
=M. 82 by sev. dark bands. A L, F neb. not far from M. 81 and M. 82. [Only 
noticed this evening, unless it is 1982 ; d’Arrest did not see G. C. 1953, which 
can scarcely exist.| (II. obs.) 
1951 650 1849, Feb. 26. Bet 2 Bst. 
1849, Mar. 14. * 9 m. with neb. 2’ diam., psb M. (II. obs.) 
1956 3196= | 1876, Feb. 21. Nota glob. Cl. pL, ir R,mbMN. Sky very bad. (1. obs.) 
10L, 98 
1957 651— WisKos}, Witenes, UG, OY warm, a double branch suspected, starting from p end in 
Il. 835 sp and np direction, and another branch from f end towards n side, connecting 
the principal neb. with another e F parallel streak north. (I. obs.) 
5509 Bes 1877, Mar. 7. pB,8,1Epf, forms a trapezium with 4 st 13 m. p, the nearest 
one in: Pos. 232°:3, Dist. 687-7. (I. obs.) 
1958 652— | 1852, Mar. 10. LL, F, thin ray. (II. obs.) 
TIT. 254 
1959 3198 1866, Feb. 17. Suspected 2 neb. ; sky bad. 
1962 3202— {| 1867, Feb. 10. F, pL, not uniformly B, not b M; S object (* or neb. %) sf. 
III. 272 Clouds interrupted. Is the object sf=1962% [No, the p L neb. must be 
—1962; both 1959 & 1962 were observed by d’Arrest in the places given in 
the G. C.] (II. obs.) 
1964 656= | 1855, Mar. 15. Espnf, has a B nucl. anda knot in sp end, or rather a twist 
VI. 4 towards then. [PI. III, fig. 2.] 
1856, Jan. 30. I see it as last year with appendage or curved branch at s p end. 
The opposite end is much the brighter and has a Nucl. 
11857, Mar. 19. Espnf, p L, Nucl and I think it has a F knot in s p end. 
1861, April 3. Esspnnf, st sparkling through it at intervals. (V. obs.) 
1973 657= | 1850, Mar. 13. Longitudinal split visible occasionally, at least in f 3. A B 
II. 492 streak seemed to run transversely. across neb. 
1851, Jan. 8. A B streak transversely, np sf. [Not seen since this date. ] 
1855, Feb. 9. Thought I saw f end split in two ; also that the neb. was narrower 
in p end, tapering off more in that direction. 
1855, Feb. 18. p half the narrower and brighter. I barely suspect I see the 
dark line in f end. 
1856, Mar. 7. Well seen with high powers, I strongly susp. itis r, also I believe 
the details suspected before will turn out to be real. 
1861, Jan. 15. fend broader and perhaps forked. 
1878, Mar. 28. pB, pL, oval, scarcely bM. E 105°°8, * 9m. Pos. 73°°7, 
Dist. 244-4, (XV. obs.) 
1975 659 = 1851, Feb. 28. Nucl. or * in centre. : 
TI. 59 |1877, Mar. 15. pB, pS, R,mbM, among 3st. 5’ nnp is an object which I 
have little doubt is a v F, vS neb, perhaps] E[=9513]. Clouds. (III. obs.) 
1978 660— |1855, Jan. 21. Hither Nucl. or * in centre, v F, R, light mottled, S * nf. 
T1I. 542 | 1867, Feb. 2. F, L, amid a L quadrilateral of 4st witha S*fand ones. (II. 
obs.) 
1982 |! 658=— | 1873, Dec. 26. vB, L, R, comet like with 2 streams of neby toward thes. * 
I. 286 8 m. Pos. 327°:2, Dist. 227-2. 
1874, Feb. 21. cB,c L,gbM, v1 E 48°-2, boundary sharper on np side. * 
8:5 m. Pos. 326°:5, Dist. 219'-7 [or, taking the mean of the two measures, 
p 23°15, 187-1 ni]. 
Ge 
