Observations of Nebule and Clusters of Stars. 15 
GaG; | h. & H — 
212 87 1854, Oct. 26. B,S, R, b M. _h. describes it as bet. 2st. I think the northern- 
=11.218 | most one is a neb. of same character but smaller. 
213 “CR. nova || 1856, Oct. 23. Notv F, R,b MN. 2 objects one n. and the other f. h. 87, but 
= I cannot be sure that they are really nebule. I suspect them both to be | E, 
215 VA. and to have nuclei. 
1857, Sept. 18. South one is p F, R, b M, north one fainter and also R, b M. 
1866, Dec. 6. 212 is c B, 8, R, a* in Pos, 221°, Dist. 77", clearly this is one of 
the two stars mentioned by h., and 215 was mistaken for the other. Once I 
suspected some neby. connecting it with 215. The latter [—213] is p F, 
S, R, Pos. 41°, Dist. 52”, from 212. e F nova in Pos. 143°, Dist. 143” 
from 215 ; this nova is a suspected neb. preceded by a v F *. Besides these 
I suspected other nebul in the field. (IV. obs.) 
217 . 1866, Dec. 30. ‘Found certainly two, perhaps 3 neb.; a is E p f, B is F and vS, 
y is e F, possibly a* but more probably a neb. exam, B&y =5153 & 
5154]. Stars numbered according to brightness. 
| Pos. Dist. 
| a to G 242°°5 151 
| atoy 291°3 110 by estimation. 
| 1874, Oct. 7. m E 263°:2, hasa Nucl.; n fend a little longer than |” 
spend. Lord Rosse suspected dark cuts on both sides of 
Nucl., which D. was unable to see. s of it are 5 st. and 
south of them a S neb. [5152] in Pos. 205°-4 Dist. 464-3 
from 217. * 1 isin Pos. 177°-2 Dist 87''-3 (1) from 217. F neb. knot in Pos. 
352°°9, Dist. 281"-7 from *1. [—5155]. 
1874, Oct. 15. I was again unable to see the dark bands bet. nucl. and ends of 
neb, which Lord R, susp. the other night. 
1874, Oct. 19. Certainly c E, although d’A. once (1862) calls it “rotunda”, 
| a second time (1865) “longula”. Pos. of EH 84°-0 (4). neb. could be traced 
about 96", though sky not good. 
1874, Nov. 2. Order of brightness of st. 2,1, 4, 3, 5. 
| Pos. Dist. 
| * 2 from Nucl. 147°-8 156":2 
al % 169°5 84:9 
| neb. sp. from * ] 209-4 407-8 [5152] 
1875, Oct. 23. Neb. [5152], e F,S, R, Pos. 205°-3 (2), Dist. 475” (32) from 
217. Sky very misty, distance Retnaps not exact. Mean of this and last 
years results is 205°°3, 470" or 25*-2 p., 425s. Adopting d’Arrest’s place 
for 217 we find as the position of 5152 for 1860-0 1> 1™ 4*-5, 58° 6' 51” (D.) 
(VI. obs.) 
218 89 1850, Nov. 7. R,BM,r. I think, a cluster. 6'n p *4.m. 
| =I. 224 | 1854, Dec. 9. Suspect the centre resolvable. 
| 1855. Oct. 16. pl, B. I have no doubt it is a cluster. The F borders of the 
neb. extend a long way out, involving sev. st. 
1856, Oct. 28. Esp nf, one * in nf edge, suspect others, Nucl. resolvable. 4 
Light patchy. 
1862, Nov. 12. pL,vgbMN., nf it is a close * , both about 14m. (IX obs.) 
221 | Il. 219) | 1866, Sept. 9. Night bad. Distance about 260". 
299, | TUL, 590 f 1873, Sept. 24. 221 isSc Ens, 1 or 2 eeF st. inv, 1 b M. 
Pos. Dist. 
“IL sate 243°°7 122"-6 
*12°5 m. 282-1 120-7 
2221s p B, pL, R, gb M to asoft nucl. Pos. from 221 71°-9. Dist. 290':7. *10 m. 
Pos. 302° (3).. Dist. 198-6 (3). (IT obs.) 
229 90 1850, Nov. 30. 1bM. (I obs.) 
=T1T. 154 
