Observations of Nebulae and Clusters of Stars. 167 
G. C. | h. & H. | ——= 
1874, Oct. 7. 4815 has a B Nucl and is c E 163°: S neb [B=III. 166] 
Pos. 59°°8, Dist. 219'-8, another [C] in Pos. 43°-0, Di 327-6. Sev other 
knots f and one p in Pos. 277°°5, Dist. 153'°2 [= 6068]. 
1875, Sept. 8. v F,S neb [B=III. 166] Pos. 61°'0 Dist. 227':9 (2) 
eFB,eS 6068 | 278°7 165: 0 (2) 
eF 6067 | 226-0 265°1 
er C 43+ 3154 
The great number of stars in the field makes it difficult to distinguish the 8 and 
v F neb. 
1875, Sept. 9. e F,S, stellar neb [E] Pos. 119°-4 Dist. 328-2 (2) 
vE,vs [D| 92:0 (2) 506-9 (2 
[6070=Schultz IX. does not appear to have been noticed here.| (XX XIII. obs.) 
4821 MPs )\ || IO, Seon les, oF i qn OO OF D> O29) 
IT. 233 157°. 
4824 | 2175= (| 1850, Oct. 7. Upper neb [f one] is equable 
IT. 234 in light and is much the fainter. Pos. 
96°-0, Dist. 323”. 
EK of p one 155°°5 
aot 895 
1854, Sept. 14. The p one is lenticular, 
Nucl vB, f one much fainter. 
1854, Oct. 17. The f one has no Nucl but 
is pretty uniform in brightness and 
does not taper off towards the ends so 
fast as p one. 
1872, Oct. 9: 
E of p one 156°°4 (2) 
scmeleans 89-0 (2) 
The 2 neb 99°5 Dist. 314'°8 
B from p Nucl 160-0 138-7 
Mop - 118-4 152°9 
By 55-6 ; 112-6 
y 6 101-2 90-1 
y from f neb 261-3 188°8 
ye 51-4 154:0 
a from p neb 325°2 112°9 : 
a 14m, 6 9°5m, y 11:0, 6 12:0, « 13:0, & 14m. 
1873, Sept. 28. 4821 B 156°- 4 (2) 
to* 6 160°8 Dist. 132”-9 
to y 118-2 143-4 
4824 to y 260-1 159°9 
By 103-6 94:4 
Be 43°5 150°8 (XVII. obs.) 
6073 st 1877, Sept. 4. vE, pS, R, vvlbM, in a A of 3 st, 13m n, 12 sp, 11 f. Seen 
through haze. * 11m Pos. 102°-1, Dist. 217”°8. (1. obs.) 
4825 2176 | 1857, Sept. 20. Narrow ray, np sf, vvF, no Nucl. 
1875, Sept. 28. eF, vm E 130° (2), vIbM, perhaps a little curved so ). 
(IIT. obs.) 
4826 2177 +~| 1867, Sept. 3. Many loose st about, vIC. In milky way. (1. obs.) 
4827 2178= | 1851, Sept. 20. r? 3stsp. Query, planetary. 
II. 705 | 1866, Oct. 29. Perhaps E pf, edges not sharp but light does not seem brighter 
in the middle than over Aine greater part of the surface. About 1 sift 
is a vS neb or more probably” 2 Ie) 1D) 
