5038 
0039 
5040 
5042 
5043 
5046 
5048 
TRANS. ROY. DUB. SOC., N.S. VOL. II. 
2207 = 
If. 851 
MWB J 
TI. 231 
2279 — 
TIT. 232 
2280 
I= 
IIT. 233 | 
2282— 
IT. 468 
2284— 
VI. 30 
2288— 
IIT. 466 
2290— 
Il. 232 
2291— 
IT. 10 
2292 
2294— | 
IIT. 855 
2295 — 
ITT. 856 
2297 — 
TT. 240 
Observations of Nebula and Clusters of Stars. Wee 
1872, Oct. 13. v loose scattered Cl of st 10m. A 94m * of a full yellow colour 
about 1™ p. (IT. obs.) 
1873, Nov. 15. pB, pL, R, gmbM. 
* 12m) Pos. 33:8) Dist: 39/0 
* 10-5m 333-4 117:9 (I. obs.) 
1850, Noy. 4. 2 p ones have nuclei, 2280 is a 8S neb with Nucl and aS * np. 
4 neb 10! nf 2279. 
1874, Oct. 15. 5025 and 26 are 2S stellar knots, sbM, Pos. 78°:4, Dist. 112’'-3. 
5027 is 8, R, sf 5026 in Pos. 98°-8 (2 hurried measures, when the telescope 
was at the limit of its range), Dist. 278-4 (2). (IIT. obs.) 
1877, Oct. 1. pF, pS, 1E np sf, * 10m 2’n. No concentration, very diffused. 
Night bad. (1. obs.) 
1857, Oct. 24. bM, 1E npsf? 
1877, Dec. 8. Found something v F and r looking, no doubt a Cl, a * brighter 
than the rest looks like a Nucl. * 8m Pos. 280°-8 (2), Dist. 277’°8 (6). 
Wire Micrometer. (V. obs.) 
1851, Oct. 24. Very coarse Cl, st quite distinct and no neby visible, dark holes 
and jagged branches, but no regular arrangement. (V. obs.) 
1874, Noy. 5. vF, suspected irr, fades away gradually. 
ee Hétonl yen Pos. 203°:3, Dist. 51-8 
* 13m 218:4 153-2 
2nd * from first one 207-0 100-0 [Pos. 227° ?} 
1874, Nov. 6. * 14:°15m 208-2 54-5 
* 13m 220-0 144-6 (IL. obs.) 
1855, Oct. 31. pB, pL, has a F but pretty sharp Nucleus. 
1857, Sept. 19. 1K, I suspect stars through it ; edge ragged. 
1867 [date uncertain]. Perhaps details of form. * 10:1lm. Pos. 205°-5 (2). 
(VI. obs.) 
1854, Nov. 22. pB, pmE, F*p. 
1877, Oct. 10. E 39°-4, * 12°13m 3’f. (IIT. obs.) 
1866, Oct. 29. <A rich field with 9 or 10 B st, but no remarkable cluster. 
(I. obs.) 
1872, Oct. 26. 5043 to *10m Pos. 321°:6, Dist. 298-3 
5042 231-0 61:5 (I. obs.) 
1855, Oct. 12. pL and B, E, gmbM, a decided dark lane runs through it in 
the direction of its major axis. The neb is rather narrower in the middle of 
its length and spreads out laterally towards its extremities, fading away 
gradually. [P.T., 1861, Pl. XXX, Fig. 42.] 
1855, Nov. 3. Seen as before, dark streak through centre quite plain. 
1856, Sept. 9. _ Seen very well ; dark lane through centre quite plain, especia!ly 
with highest single lens. 
1856, Oct. 3. I think I see right hand side of centre [f side] to be composed of 
stars. It is brighter than the opposite side. [Pl. V.] 
| 1860, Sept. 17. The nf side seems sharpest. (XXIV. obs.) 
1854, Oct. 17. pB, R, bMN. (IL. obs.) 
nO) 
> 
