Observations of Nebule and Clusters of Stars. 99 
G.C. | h. & H. | ar aa 
Novee ... | 1874, Feb. 9. Set for 2464. Found a neb [e], 
PES wr lop Mile eine oss) Suc Oumm Distal Quo, 
another [7] p F, same * Pos. 5°-5, Dist. 71''-7. 
Third neb p [y], pB, cL, glbM, E 90°+, 
same * in Pos. 100°-4, Dist. 148-4. The 
* has a very red * 8:9m in Pos. 153°-3, Dist. 
526''8 [or 17-08 f, 470-6 s. * 8-9m—B. D. 
-+ 22°, 2380]. None of the 3 neb have 
Nucl. 
1874, Mar. 18. Found a neb [«], pB, S, R, smbM, 
Nucl. not stellar. 
9 fore, Jets, BN ID rete, GI) 
* 12m 207-4 63:0 
* 9m from * 8m 303°9 671-0 [or 40%-20 p 
3874/5 n| 
Neb[a], F,S, R,from*9m322°5 78-1 
[* 9m is—=B.D.-+-22°, 2377]. 
1874, April 5. Group of neb measured from a 
? NO ien, 
Novae near 246 
| Pos. Dist. 
v F, R [6] Wana) Gul9 
p B, pL [n] 187°8 80:7 
p B, R, cbM [«] 201°5 114-2 
F, L, H45°+ [2] 182-9 237-3 
pB, pS, R [6] 314:8 116-2 
p B, pL, R [6] 294-5 160-7 
p B, pL, BR [y] 278:0 153°5 
1874, April 14. pB,S, R, cbM [c], no stellar Nucl. 
Pos. Dist. 
* 13m IE Pse 62!-7 
- -* 85 (reddish) 80-6 162°6 
1876, Apr. 13. Group of 6 neb sketched [6, 7, ¢, y, 2, 6], ¢ to *, Dist. 118”. 
[The annexed diagram has been constructed from all the measures. Adopting 
the place for the red * as given in the Bonn Observations, vol. 6, we find the 
following positions for 1860-0 :— 
a ee BRS eos: Gi Omlai9 
B 28 53:54 28 21-2 
y 28 54:01 29 3-7 
5 28 58:14 — GB HY) 
é 29 ~=0-98 al 110 
C 29 3:35 33 24:8 
n 29 3:55 30 43°6 
0 29 4:28 30 29-6 
t 2 OOO 37 46-2 
d’ Arrest’s nova=2464, 115 29™ 168, 67° 24' 12”, which he only saw once and 
a second time searched for in vain, has therefore not been seen. None of the 
above nove are included in the Suppl. to the G. C., as the * 89m has only 
a short time ago been identified by means of the * 9m 11’ np]. (V. obs.) 
2466 ayers } 
2469 923— _ | 1857, Mar. 22. 923 isvS, R and very like an ill-defined *, npp is another of 
ITI. 29 j same character, but fainter [—2466, nova d’Arrest]. (I. obs.) 
