Observations of Nebule and Clusters of Stars. 11 
G.C h. & H. 
9] Le 
98 40 
IT. 856 
108 | coe 
94 37 | 
TIT. 595 
101 49 
5113 st uat) 
95 38 
II. 479 
97 | IL. 857 
104 | IL. 858 } 
105 A4 
—V. 18 
106 AB 
EG 
Or | Aes 
II. 452 
108 io 
111 AT 
=IT. 209 | 1854, Oct. 26. 
| 1850, Dec. 6. a is h. 40,itissb M. Itis 6’sfa *10 m. 
| 8 is much smaller than a, and-iss b M.,and J think 
nova. [The * is B. W. 0° 530 and B=G. C. 91 = 99.] 
1851, Oct. 23. h. 40 is B. M., suspect Nucl. 
1873, Dec. 11. *8m. to neb.s f[98] Pos. 150°-3. Dist. 357/-6 ky 
neb. is B,p L,R,svmbM. Same * toacF, Lneb. [= 103]. Pos. 80°°8. 
Dist. 402/72. (IIL. obs.) 
1854, Nov. 24. h. 37 is not L, R, b M., B.* closes p; r.? h. 42 is R,bM., r.? 
I suspect a v F, 8S neb. a little n nf h. 42, but cannot feel satisfied that it is 
not a * ill defined. 
| 1873, Dec. 11. 94 is p B,S, R,vsb MSN. 
[3 
*12 m. Pos. 244°-6. Dist. 31/7-4. 
NO) can, (18% ID) ba), Jets, IIL dO), Dist. 152/-3. 
94 to 101. Pos. 106°°3. Dist. 395-6. *10 m. (B. D. + 2°-85) to neb. F, 
R. Pos, 24°:2. Dist. 479’-7 or 13° 1 f., 437’-5n. A coarse D. * points to 
this new neb., both comp* 114 mag., the p. comp* f. 26°°8, 128’°3 n. 
1873, Dec. 19. 101 to*9m. Pos. 280°°7. Dist. 262-5, * — B. D. + 2°-85. 
NOMtomsIma Rosw3 539s eDisty N32 28 94s torso ms Poss 2492-63 
Dist. 32”-0. The 9 m. * to the last * Pos. 283°°6. Dist. 170-2. F. * or 
neb. from 101 Pos. 246°-6. Dist. 110’:8. 
Nova, E. 70°-8 (3). Pos. from B. D. + 2°°85, 20°-7. Dist. 498”-0. [| Pos. for 
1860-0 0> 32™ 28:0" 87° 19’ 317-0, = 5113.] (ILI. obs.) 
| 1866, Dec. 14. Oneneb. with either 2 st. or B, 8, neb. knots very closely f.—c B, 
p L, R,b M,twopBst. p. (1. obs.) 
1873, Sept. 17. Preced. neb. isc B, L, cEns, gbM, * 103. Y 
Pos. 348°-9. Dist. 247/71, sX 0 
This * to * 102 n. Pos. 1°-0. Dist. 57/6. | my 
2nd * toneb. f.(F, ¢ L,R,g b M.) Pos. 120°:4. Dist. 204”°6. 
First measure uncertain on account of clouds. G. C. 97 and 104? 
1876, Oct. 22. 18/+f and 4’ and 9’ n of 89 are 2 neb., p F, p L. Pos. 23°-7. 
Dist. 380". [A a = 10°-2. Schultz has 11*:2, H 18") 97 has a *11 m. in| 
Pos. 260°:2. Dist. 329”. (II. obs.) 
1850, Nov. 2. Spirality suspected. 
1855, Oct. 16. vL,mEnp,sf, sharp nucleus, for some distance round which the 
neb. is B. and then suddenly decreases ; there is a B. * n p nucl. ; and another 
inv. in s f end; another in p border. 
1876, Nov. 19. Far too B. and sharply defined in Bond’s drawing. 
1854, Oct. 16. Saw what I believe to be Herschel’s diffused neby. It extends 
farther n. s. than in the other direction. Many st. involved. (I. obs.) 
1857, Dec. 7, B. centre, m E,ns,armsv F. About one field of finder [26’| s, and a 
few seconds p. is another neb., F, E nearly ns, no nucl. [=108.| 
1877, Oct. 29. pB,pS,1E,mbMN,* 11:12 mag. Pos. 249°-3. Dist. 137”. 
About 35% p. and 25't south is 108, v F,S,1 E pf, mbM N, stellar, 5’ nnf. 
a coarse ¥ 10-1l and 12m. A very insignificant object. (II. obs.) 
1854, Oct. 17. B, R, b M. 
R, p L, b M. 
1855, Nov. 3. I found here 3 neb., perhaps 4, as in annexed sketch. 
A is oval, and I think r.. *atnp edge. BisS, R,bM. Cis 
so Fas to be rather doubtful, and D is either a % or, (as I] yy aS 
believe) a * close to a S neb. knot. A 
1877, Oct. 10. Looked attentively for the 2 or 3 novae suspected in 
1855. Could see none, and feel convinced that there are only F st near 111 (one 
for instance 6’tnff.) Neb. is p L, irr. R, soft looking. (IV. obs.) 
