Observations of Nebule and Clusters of Stars. 
1529 
1532 
3081 
3083 
446 
Mii 
III. 703 
Mpa {t 
III. 900 
449— | 
Til. 901 | 
J 
II. 820 
450— 
IV. 45 
1876, Jan. 21. Both 8S, R, mbMN, 1520 probably a little larger than 1519. 
Pos. 53°:9 (4), Dist. 27'-7 (4). No change has taken place here since 1862. 
(XVIII. obs.) 
1877, March 3. Rich fields, no remarkable clusters. (I. obs.) 
1849, Feb. 20. 6 neb. of which ¢ is perhaps a D *. 
1851, Feb. 26. a B Pos. 222°°7 Dist. 221” 
By 283-0 337 
O€ 292-4 229 
ef 268'8 407 
[The diagram has by a mistake been badly reproduced in the 
P. T. for 1861, and h in the G. C. p. 21 has supposed it to be 
two separate diagrams of the same 3 nebul, instead of its 
being one diag. of 6 neb. 6 is most probably =h 446, the 
position of which thus becomes 7" 18™ 44°+ 55° 53'3, while 
¢ and « have been entered as 5380 and 5383 in the Suppl. to 
the Gen. Cat. a=h 449, 6=h 448, y=h 447]. 
1852, Jan. 24. 3 neb. seen. 
1852, Feb. 9. 7 neb. knots seen. 
1856, Jan. 29. Could only find 5 neb. About half a field of 
finder [13']nf there is a v F oblong neb., major axis ns 
with 2 st close f (nnp ssf of one another), its light is nearly 9 
equable, but p end perhaps brighter. [This appears to be a p 15279 I 
Nova, it can hardly be 5386]. 
1866, Dec. 10. a and # are much brighter than the others. I should call them 
pF, pS, 7 [=5385] is F and perhaps 1 E, 6 [=5386] is e F and S and only 
seen by glimpses. I feel certain there are other neb. in the field and many 
st, L and S scattered about. 
a B Pos. 220°:7 (2) Dist. 198'-0 (2) 
an 181-0 (2) 82-1 (2) 
a0 163°5 (2) 147-0 (2) 
1866, Dec. 12. An additional neb. (y=h 447) seen, e F. 
a Pp Pos. 21.9°:5 (2) Dist. 199""°5 (2) 
an 182:2 (2) 91-5 (2) 
256°5 (2) ATT + 
ay aS 
1876, Jan. 1. 1530 and 1531 (@ and a) are both e F, pS, R, p one vlbM. Pos. 
41°-4 (2), Dist. 214-6 (3). Nova [=5384], more stellar, mottled, in Pos. 
931°-0, Dist. 262''3 from 1530 or 16%4 p, 165"s. Sky very misty. 
1876, Jan. 25. Found sevy.e Fneb. The sky was very hazy and thin clouds 
were passing. Two neb. Pos. 103°-0, Dist. 342" [8 and y], two others Pos. 
107°°5 (2). Dist. 230" (2) [6 and e]. (LX. obs.) 
1876, Feb. 23. Irr R, probably 1E pf, stellar, looks like a hazy * (I thought 
once it might only be an eS group of ee F st?). Forms a rectangular A 
with a * 16m sf anda * 17m nff about 2' dist. 3st 14:15m pina curved 
line, the nearest one in Pos. 279°°5 (2), Dist. 161-2 (2). (1. obs.) 
1849, Feb. 20. Most astonishing. * perhaps a little nearer the p edge, breath of 
ring less on f side. Drawing taken. [See P. T. 1850 Pl. XXXVIIL, fig. 15.] 
1849, Feb. 22. Dark space to the right of *. . 
1850, Jan. 16. Both the dark and the B rings seemed unequal in breath. The 
light appeared unsteady and flickering, night rather foggy but sky black. 
(Small mirror found to be out of adjustment.) 
1850, Dec. 5. The p part of the dark ring is the most distinct. I had a vague 
impression that the f part of the outer luminous ring was encroached upon 
by the dark ring, and sometimes I fancied the p part of the inner luminous 
ring was detached from the * by a darkish space or else that the part of it 
next dark ring was brighter than that part next the star. 
