Observations of Nebula and Clusters of Stars. 
Seen with difficulty, indeed I am not sure it is not a vS group 
(1 obs.) 
[II. 48 must have been = II. 80 (1704), compare the Suppl. to the Gen. Cat. p. 390. 
h 527 seen as an eS Cl by d’Arrest & Schultz. | 
Exceedingly close D neb.. 
e close D neb, light blended together. 
v close D neb, which I suspect to be enveloped in F neby, the 
p neb is the larger. Is there av F * npp? 
sp nf, equal in size and enveloped in F haze of neby. 
D neb. in Pos. 85°:5, p one ¢ B, R, mbM, f one F, R, perhaps 
with a * in the middle. A * in Pos. 20°, Dist. 109", another in Pos. 111°, 
Dist. 83" from p neb. 
pF, pL, close D neb. p &f (or neb with a D Nucl.) Badly 
seen among clouds. 
*12m. Pos. 195°] (2). 
== T@pilil inn, 9-9 
The last * has a comp®. 12:13.m I'nff. 
Dist. 131''-2 (2) 
298:5 
(1X. obs.) 
4' diam. gbM to a strong Nucl. 
v B Nucl. fades off all round but not quite symmetrically, 
Nucl. perhaps irr. shaped. 
p L, sbM S Nucl., perhaps filamentous. 
vy B, S Nucl., but not a *. F outlying neby very extensive. 
Seems an unresolved Cl, B centre, fades off very gradually. 
Very coarse Cl. (I obs.) 
v Llenticular ray, slightly concave np, gyvmbM, perhaps 10’ long. 
70 
G. C. | h. & H, | 
1707 527 1876, Feb. 21. 
of F st. 
1709 529— )| 1851, Feb. 26. 
TIT. 294 }| 1852, Mar. 9. 
1710 |R. nova ) | 1855, Feb. 16. 
1857, Jan. 20. 
1867, Jan. 12. 
1876, March 15. 
1711 530= | 1849, March 22. 
I. 242 |1850, March 9. 
1855, Feb. 18. 
1855, March 7. 
1863, Feb. 20. 
(XI. obs.) 
1712 531 1848, Dec. 19. 
1713. 532— 1851, Dec. 29. 
I, 200 
1854, March 1. Nucl, stellar? Are there parallel dark lines exterior to it as 
in Andromeda ? 
1858, March 8. Slightly concave towards p side. 
is double. 
1860, Feb. 12.. Centre has the peculiar sparkling appearance of the brightest 
parts of Neb. in Orion ; I feel certain it is r. 
1861, Jan. 15. The nf end of the neb. is the fainter and suddenly fades from 
the middle. 
1867, Jan. 10. Slightly concave p, Pos. of E 39°-5 (2). 
40" broad. 
1868, Jan. 2. On f side it fades off more gradually than on the p side, where it 
is more abrupt. Susp. v F streaks and lanes on each side parallel to the ray. 
1873, Dec. 27. v B, vm E 39°:6 (3), gbM to an ill defined centre, slightly con- 
cave on p side. 
Has a Nucl. * on np edge 
About 6’ long and 
* 11m (a) 
Pos. 27°:2 (2) 
Dist. 125-3 (2) 
ato* llmnp 303°6 (2) 84:3 (2) 
ato * 15m np 334°9 (2) 57°3 (2) 
a to * 10:5 sf 151-1 (2) 174-4 (2) 
ato*12ms(6) 195-4 (2) 275°5 (2) 
2 to* l6ms 201:7 32°8 
a to * 16m nf 49-1 115:4 
sf the last * 16m is another * 16m. 
1876, Feb. 27. Ray, gbM alm to a Nucl., abt 53’ Jong. A little concave and 
rather sharper on p side. Pos. of E 38°. 
* 10m Pos. 104°1 (2) Dist. 164"-1 (2) 
* 12m 29°8 139-4 (XVI. obs.) 
