Observations of Nebule and Clusters of Stars. Ad 
1875, Dec. 3. About 20 st about 9:10 mag. The most conspicuous cluster 
in this neighbourhood. [Measured and drawn by Vogel, Positionsbestim- 
mungen von Nebelflecken und Sternhaufen zwischen + 9° 30! and -+ 16°30! 
Decl.]. (1. obs.) 
1875, Dec. 3. Cl. not conspicuous, a dozen stars about 12 mag. in a curved 
line. (I. obs.) 
1877, Jan. 13. vv F, pL, irr fig, probably E pf, diffused, has an are of stars sp 
and a * 10-11 mag. 4’ nnp. Sev. st 11 mag. f. (I. obs.) 
1850, Jan. ais pB, R, B pB, 8,y F, R, 6 F, E. Distance a 6 about %, Ox 
15’. 
1851, Oct. 30. h 334 is about 5’ n fa * 9 mag. y is v F, ZB and 6 are F. 
1851, Nov. 23. Sketch made, agreeing well with the one made last 
year. Dist. a 6 3'+, B y 5'+ nnf, a 6 13. 
1852, Jan. 17. The 2 south ones are bM, sf one ]Epf. gg 88 
1856, Dec. 26. 2neb. p &f. both F, R, 1bM, the p one is much the smaller; 
about 10'n of these I suspect a vE neb. just np a 8 *. 
[a—920—921—924, the 2 latter are put down in the Gen. Cat. as R. novae, 
but there is no doubt as to their identity with h 334; B—919, a—918, 
6=922. Adopting d’Arrest’s positions for 919 and 920, the places of the 
nebulae forming this group are for 1860-0 
919 An 45™ 215-0 93° 20' 45” vF, vS, * 9m. 32's 
918 4 45 24+ 93 16 45> wit 
920 4 45 32-2 93 20 40 1D, jolly 18, 
922 4 45 40+ 93 8 40+ Fj. (XX. obs.) 
O7 
1855, Dec. 8. S, slightly oblong, b MN. 
1856, Dec. 28. The Nucl. is an E disc, v F * sp, to which the neby. reaches. 
1858, Jan. 13. B center which I strongly suspect r, F neby. stretches out a long 
way, involving a minute * p. 
1860, Feb. 13. B, 8S, R, b M, could not be certain of stars in it. A smaller one 
nf, scarcely perceptible in finder and v F, above a F *. 
1864, Jan. 2. pB, broad Nucl. * 11 mag. sp. 
1875, Dec. 22. pB, 8, R, vg vm bM, Nucl.—*12 mag. * 11 mag. Pos. 224°-2 
(3). Dist 154"-4 (38). 
1875, Dec. 24. * 9 mag. Pos. 330°°3 (3). Dist. 3515 (3) or p 11°66, 3053 n, 
For 1860-0 the neb f 11°69 305":2 3 (corrected for refraction). [The * is 
Lalande-Baily 9310 and the place of the neb. for 1860 4° 50™ 1°47 95° 5' 
16'°8.] 
1876, Jan. 26. Looked for other neb. near it, saw none, many e F stars (one 
2' sf, another between 932 and the * 9 mag. n &c.) which may have been 
mistaken for neb. knots. * 9 mag. Pos. 330°-7 (2), Dist. 353'°4 (2) or p 
11°57, 308-2 n (for 1860 11°60, 308":1). (X. obs.) 
1854, Oct. 26. Only a group of 4 or 5 stars. (I. obs.) 
1872, Oct. 11. Cl, v L, st 11 & 12 mag. with some B ones. (1. obs.) 
1854, Dec. 18. Two neb. knots, the f one is a little larger and [93 AN 
brighter than the other, both R, lb M, * p. [The f one=h 339, p 
one—nova. 
1873, Dec. 22. 943 is the brighter and larger of the two, a F * or © 
a suspected neb. near, Both 943 & 944 are R and like distant 
globular clusters. 
Pos. Dist. 
943 to 944 282°°8 174-1 or 11%:3p, 38'°6 n. 
944 to *p 294-2 50-5 
1876, Jan. 21. A smaller and fainter neb. (944) p 943. Pos. 281°°8 (2), Dist. 
160-9 (2) or 10°7 p, 32-8 n. (AIL. obs.) 
