Observations of Nebule and Clusters of Stars. 111 
G. C. h&H. | — 
2783 1131= | 1855, Feb. 19. Light uneven. Is the Nucl nearer the ssp edge of neb? * in 
IT. 106 nf edge, a triple * a short distance s. 
1855, Mar. 17. L,R, has Nucl. Is there a dark ring round the Nucl? * in 
nf edge. 
1857, Mar. 18. Has & Nucl which is excentric. Not R, an arm reaches toa 
pB* nf. Isuspect bands init. Night bad. (IIT. obs.) 
2786 11382— | 1850, Mar. 9. Ray, diminution of light in neighbourhood of Nucl; edges 
M. 98 parallel, night bad, remarkable object. 
1861, Feb. 10. I think a darkness exists on both sides of Nucl. About 4 field 
of finder [13']n of this isa F, R neb with a * or Nucl in centre, [ Not 
noticed on the other occasions, would be a Nova. | 
1861, Mar. 12. Around Nucl the neb is fainter than half way towards the 
extremities. Split f Nucl? 
1867, Mar. 29. EH 148°-4. A remarkable ray ; the p portion is not so long as 
the f one, in the latter there is about midways a spot much brighter than the 
neighbourhood. Split not seen. (IV. obs.) 
2794 1138=— | 1873, Apr. 20. cF, ir Ror v1E pf, rr, at least 2 centers of condensation. 
TI. 164 (1. obs.) 
2795 IT. 165 | 1860, April 23. Ray, gvlbM, pB* sf. Much fainter than h 1148. (LI. obs.) 
2796 1140= | 1855, Apr. 6. Very like a distant Cl, v B Nucl with neby gradually fading off. 
I, 17/6) * inv p Nucl and other stellar points susp in the outlying F neby. 
1855, Apr. 17. Like a distant Cl, a * plain p the Nucl, another fainter sp. 
1856, Mar. 28. B, R, sbM toa v B Nucl, edges fade away, very much filamen- 
tous,aS*pinv. Cl? (IIL. obs.) 
2798 weoxs 1874, Apr. 9. mE 38°:6. (1. obs.) 
2802 1144— | 1852, Apr. 14. The brightest part is in advance of the centre ; v S * n. 
II. 108 | 1867, Feb. 1. B,1EH 107°, bM. Clouds. [It is remarkable, that neither the 
observers here nor d’A have seen 2799=h 1142—TII. 107 p IT. 108 10°in 
parallel, which he observed in sweep 243, while 1144 was observed in sweeps 
419 and 338. H seems to have seen them both on Apr. 8, 1784.] (II. obs.) 
2804 1146== | 1856, Mar. 8. Ivreg. shaped neb with Nucl excentric and some sort of knot or 
I. 95 appendage f. Possibly another F knot in pend. The former one is likely 
connected with the neb forming a spiral arm. Perhaps a * nf centre. 
1856, Mar. 27. Much better seen. There are 4 knots or st in the neb besides 
the B patch sf. [Plate IIT., Fig. 10. ] 
1857, Mar. 19. I see the knot atsf end. This end of neb is much the brighter. 
I see the knots and by glimpses a * in p end. 
1857, Mar. 24. At times the knot sf seemed quite detached from the neb. I 
cannot see anything more in the p end than that it has a mottled look and 
a v F projection at sp corner. (VII. obs.) 
2805 1147— | 1851, Mar. 6. S lenticular ray. B Nucl. 
IT. 135 
2806 1148— | 1860, Apr. 23. A fine Eneb, v B M like a glob C] (1 think too itis r?), 8S *f 
I. 35 Nucl, where I also think there is very dilute neby, parallel to neb. The 
neb is either twisted at n end in p direction or it has F comp". there? Dark 
space round centre? perhaps only the contrast of the B centre. ,15' long. 
1867, Mar. 26. A remarkable ray, H 17°. (III. obs.) 
1849, Mar. 15. 1149 is lenticular with a split in direction of major axis, f 
centre. 1155 seen. (I. obs.) 
