30 Observations of Nebulae and Clusters of Stars. 
G. C | h.& H | — 
560 232— | 1851, Oct. 23. Somewhat fan-shaped, light suspected mottled. 
II. 211 | 1855, Oct. 7. Has a knot in p edge; neb. spreads out and fades away gradually 
sf. 
1855, Oct. 12. Last week’s obs™ confirmed ; sketched [See Phil. Trans. 1861, 
Pl. XXV, fig. 3.] 
1855, Oct. 16. Sketch should have been fainter and the knot in p end less well 
defined. 
1855, Dec. 8. Lord Rosse thought it resolvable. 
1857, Dec. 9. The drawing makes its edges rather too sharp. 
1861, Dec. 28. Sharper on nf edge and curved on that side. 
1862, Nov. 18. Pos. of E 145°-4 i) a 
af Pos. 18°3 Dist. 94” <«% 
ay 285°9 45 CO 
aé 95°6 41 
y 46:0 99 
1866, Oct. 8. It was suspected that branches proceed from neb. towards the 
stars a and § (in the above diagr.), but of this I was not sure. Neb. ends 
more abruptly on the other side. (XV. obs.) 
565 | 235= ) 
NOL, Bh) t 1866, Oct. 29. South neb [565] pB, Ens, bM, n one [566] vF,S, Epf. AS 
566 | 236— neb suspected p the south one about 1’ dist.? (II. obs.) 
TIL. 573 | 
569 238— |1848, Dec. 18. bM nearly to a Nuel. 
IIL. 557 | 1875, Nov. 26. F, not v8, irr (perhaps vl E pf or spnf), sbM. * 10m in Pos. 
180°-9 (2), Dist. 236'-5 (2); * 10m in Pos. 81°-7 (2), Dist. 349-7 (2). 
(IV. obs.) 
572 241— | 1854, Oct. 26. Thought there was a dark space cutting off the south end of neb, 
IIT. 152 which is E ns, and has a B * f. 
1854, Dec. 11. Again I believe I see a dark space of some kind s of main nucl. ; 
sometimes I thought it cut off the s end entirely, sometimes I thought it a 
dark eavity enclosed on all sides ; once it struck me it might be open on the 
f side but having a F branch p, connecting the south end with main part of 
neb. A second fainter Nucl. or * close south of cavity. 
1857, Nov. 23. Sketched. [See Phil. Trans., 1861, pl. xxv., fig. 4.] 
1862, Nov. 20. Nucleus (or rather the brightest part) is clearly r, I saw 2 st 
in it sev. times distinctly. One * in ssp end clearly seen. The * close f is 
about 14 mag. (X. obs.) 
574 944— | 1856, Nov. 28. pl, mbMN, patchy. Suspect the p end is separated from the 
I. 102 rest of the neb. by a darkish line. § * or knot close np. 
1872, Nov. 1. * 11min Pos. 48°°5. Dist. 125-2. (II. obs.) 
575 242—- |1850, Sept. 14. LL; 6 st seen distinctly in it, one suspected close south of 0 
L. 156 |See diagram to 1850, Dec. 27] and at moments others near 6. 
Pos. Dist. 
1850, Dec. 27. aN UDP 54” 
ay, 79-6 199 
af 328°8 29 
ao 279-0 99 
About 20' p h242 is a * of 8th or 9th mag. which appears 
to me to have an Atmosphere. {This * must be B. D. + 38° | LY, 
No. 527=Lalande-Baily 4845 ; 7-8 mag. | EVES, 
1856, Oct. 2. With one-inch single lens Lord Rosse thought the Nucl. was 
composed of stars. 
1860, Dec. 11. Centre v B & R with v F arms extending pf of same or even 
greater breadth. 
