100 Observations of Nebule and Clusters of Stars. 
G.C | h. & H. | ——= 
2471 925— |1852, Apr. 9. gbM, a F appendage or 2nd neb. 
If. 731 | 1855, Apr. 17. The appendage looks like an 
independent neb. Lord Rosse thought the B 
ray Y. 
1861, Apr. 12. Two, probably connected. (III. 
obs.) 
2474 928— | 1872, Mar. 6. F,S, R, mbM. (I. obs.) 
IDOE, Sil 
2477 930— |1852, Apr. 14. Within a trapezium of 4 st. 
II. 732 | 1861, Apr. 12. One * on s edge, st p and n are not involved. 
(LV. obs.) 
2479 931) | 1852, Feb. 24. 2 rays, forming an angle of about 100°, the 
2480 xr s one has Nucl. and there is a knot at the n extremity of 
the n one. 
1860, Apr. 20. I am not sure whether they are joined at f 
end or not ; s one has a * in centre, both vgbM. : 
1877, Apr. 5. Both vgbM ; 2480 es 
is E 177°:2 (2); 2479 is less 
E 56°-8, it has a * 12°13m in 
Pos. 120°-6, Dist. 1281-0. 
(III. obs.) 
2481 933— 1| 1851, Apr. 3, Another 
ROD v F neb. about 6' nf 
2490 939 940 [=2496]. 
TI. 161 || 1855, Apr. 6. h 933 is 
ZO a eee vv, lbM, 939 F, 
2492 : IbM, 940 is pB, E 
2493 940 = sp nf, bM, neb nf 
III. 30 | the latter, vvF, R, 
2496 IbM [2496]. 
1856, Mar. 27. 6 neb. 
933 is Enp sf, bMN, 
939 more oval, bM, 
940 is E pf, hasa B 
* sf A isavv EF 
knot, B is pL, but 
v F and flickering, 
so that I could 
not well make out 
its shape. C is a 
vv F knot or possibly a*. [As B= 2496, 5069 = R. nova is to be struck out. | 
(ILI. obs.) 
2484 | IIT. 844 | 1860, Feb. 12. F, Ens, vgbM, ends pointed. (L. obs.) 
2486 934 } 1848, Apr. 1. A pBneb with a smaller one f. 
2488 936= \| 1849, Feb. 26. Suspect appendage to p one, f one susp. r. 
II. 103} | 1861, April 27. The f one is E towards the p one. Are they connected ? [2489 
—R. nova to be struck out, only h 934 and 936 seen.] (IIL. obs.) 
2487 938— | 1855, Jan. 21. vmEsp nf, B centre and 2 knots in sp end, these however may 
IT. 340 turn out to be st when seen more favourably. 
1857, Feb. 22. v F, E spnf, lbM. 
ha a Se 
