78 
1898 
1904 
1916 
1917 
1920 
1918 
1919 
1924 
1925) 
1926 | 
1928 
1930, 
1932 | 
1934 J 
1931 
626= 
G. C. | h. & H. | 
IL. 275 
630= 
I. 61 
III. 278 
638= 
TUL, GIL 
R. novee 
639= 
V. 26 
j 
] 
{eT 
| 1852, Feb. 18 
| Sev. e Sneb susp. s of 1924, but there are thin clouds now. 
Observations of Nebula and Clusters of Stars. 
1851, Mar. 5. 
1856, Jan. 30. 
R, vlbM. 
vF, pL, R, vgbM. Fades away very gradually. (II. obs.) 
1851, Mar. 5. 8, 1E, vg bM. 
1876, Mar. 18. B,vS, R, bM, * 9-10 m. in Pos. 234°:8 (4), Dist. 44-3 (4) 
[or 2°42 p, 255 s]. 
1877, Mar. 4. pB, pS, vmbM, * 10 m. Pos. 23678 (4), Dist. 42-2 (8) [or 
2°36 p, 23-1 s; the place of the * is given in Vol. VI. of the Bonn Obser- 
vations, and taking the mean of the above 2 nights’ results we find G. C. 
1904 for 1860-0 9» 35™ 29%-49, 93° 3' 43"-2]. (LIT. obs.) 
1873, Dec. 26. ¢B, v L, vgmbM, about 5’ long & 2'$ ¢ 
broad. *13 m. to * 11m. Pos. 149°-0 (2), Dist. 
150"-0 (2). The axis of the neb. is nearly parallel 
to the line joining these stars and is f that line. The 
neb. is more sharply defined on p than on f side. * 
13m: to * 8m. Pos) 165-45 Dist) 82556. The)* 
13 m. seems involved. 
1874, Feb. 21. a Pos. 149°:6 
ay 17-2 
ao 287-6 
313°2 
Dist. 148-7 (2) 
74-6 
196-6 
211:3 
(II. obs.) 
ae 
1854, Mar. 20. h. 634 & 636 e F, night bad. 
1855, Feb. 19. The p. one is double, its comp”. being close p; 1 E sp nf ? 
is | E npsf, has a F stellar Nucl. 
1857, Feb. 23. h. 634 is bMN ; vv F neby involving a * sp? 
IbM, oval nearly pf. 
1867, Mar. 27. R, lbM, with higher power I suspected a close ee F comp. unp. 
(V. obs.) 
h 636 
h 636 is F, 
Both ghM. 
1852, Mar. 9. The n one has mottled appearance. (II. obs.) 
1851, Jan. 25. E spnf, would be r on a good night, 
B, y, dare e F, < isee F, asusp., v F * in GB (and 
») 
n | 
1860, Mar. 24. pB, sometimes I see glittering 
points in it, 1 E sp nf, I think there is a v F neb. |G 
p and another e F f. E 
1878, April 1. pm E 51°°3, mbML oval Nucl. 
Dist. 
203'-1 
388°5 
552 
B, S, wr R, x 
y, VF, ps, Ennp ssf 
n, pF, 8, EH, * 13°14 l'p 
6, VF, S, stellar 
[= 1928] 
[= 1932 
[= 1934 
[= 1930] 
23°°6 
62:5 
88 
117-2 417-9 
[a = 1926 and 
¢ = 1925 were not noticed. The place for 1926 is evidently wrong, it must 
be about 9 40™ 15s, 45° 14'.] (III. obs.) 
1849, Mar. 14. *1in p part; brightest at s edge of centre. Seems stellar at 
moments, vy F neb. extends both ways in continuation of the brighter part. 
Badly seen. 
