40 Observations of Nebule and Clusters of Stars. 
G. C. | h. & H. | 
1873, Nov. 15. Exquisite planetary nebula. * 14m. in the centre, surrounded 
by F neby and that again bya Bring. Many S st in field [diam. 8'] powers 
414 and 650 showed the Nucleus quite stellar 
Pos. Dist. 
* 12-5 m. IPG 134"°8 
F116) Tan, 192:9 89:9 
* 12 m. 311-6 166°3 
*16 m. 354-0 92-7 
Diam. ns 54-1 by dark bars, 56'"3 by bright wires 
” pf 63°6 ” ” 54:0 ” ” Ge obs.) 
802 | VII. 47 | 1873, Nov. 15. Coarse but brilliant cluster, in the centre is a double star, Pos. 
124°-2, Dist. 17-0, both stars 8-5 mg. (I. obs.) 
895 TI. 279 | 1876, Jan. 21. pF, vm E 13°, about 2’ long, vlbM (or rather s of the middle ); 
* 13-14 m. p, Dist. 73”, 2 st 14:15 m. nff, 2' and 3! from neb., in a line with 
the p star. * 9-10, Pos. 163°°3 (2), Dist. 217-3 (2). 
1877, Jan. 13. pF, p L,mE9°°6, vvlbM, * 15m. p, Dist. 81"-4(2). *10m., 
Pos. 161°-8, Dist. 225'-1 (Dist. difficult to measure on account of the Elong.) 
(II. obs.) 
809 VII. 60 | 1875, Dec. 4. Cl, not Ri, most st 11:12 mag., fills exactly field of finder eyepiece 
[Diam.=13']. (1. obs.) 
810 311— | 1852. Jan. 13. New spiral of an-annular form round the *, which is central. 
IV. 69 Brightest part is sf the *, spirality is v F, but I have no doubt ot its existence. 
1855, Oct. 7. Annular, but with a break in the south side of the annulus, or 
perhaps it is spiral. 
1856, Oct. 31. I feel certain of a dark space nearly p the central *, but the shape 
of the whole is only conjectural ; there is a * plain np the neb. 
1857, Dec. 7. Not v F, and the break in the south side of the ving of neb is quite 
easily seen ; between this ring and the central * is not black, but filled with 
more F neby. 
1858, Jan. 9. Observed for a sketch; last observation correct as to shape, the 
brightest part is sf, and the next brightest is on the opposite side, and with 
J-inch single lens the whole annulus has a mottled look. 
1858, Jan. 13. The whole edge was ragged and irregular and the whole neb. much 
mottled. [See P. T. 1861, Pl. XXV., fig. 7]. 
1862, Nov. 20. Very difficult to determine its true shape.. I think 
there is a * at a in a little knot almost detached from the neb. 
The opening at 6 is easily seen. Sometimes at ( the little knot 
seemed attached, and occasionally as if it extended south for 
some distance. At y I was doubtful whether the ring is closed or not. 
1862, Noy. 24. I think observaticn of Noy. 20 is correct. 
1864, Febr. 3. In nf end I thought two or three times I saw a dark lane. Is 
the brightest part (s of this doubtful lane) resolvable ? 
1873, Nov. 16. *8m. ina neb. atmosphere which is irregular in brightness, 
being somewhat denser sf and somewhat fainter np. * 16 m. about 10" n of 
the n edge. Diameter ns 114-0. (XX. obs.) 
813 2611 | 1867, Jan. 25. I have little doubt that there are interesting details in the form 
of this object but the altitude is low (15°) and the night was bad. The 
middle part is B but apparently excentric if (as was suspected) there is a 
branch proceeding s and somewhat curved towards the p side. F; L; E; bM. 
Has a star pos. 239°-6, dist. 139'-0 from the B part. (1. obs.) 
820 | VII. 61 | 1872, Oct. 13. Ck Ri, 1C, the stars have rather a tendency towards a spiral 
arrangement. 30! sf is a very red * 93 mag. 
1875, Dec. 4. Cl, pRi, st 10-11 mag. About 2°f and 12'+ south isa very red 
* 9-10 mag. [Not in Schjellerup’s Catalogue, it is probably B. D. + 50°, 
965.] (II. obs.) 
