11.1374 J 
110 Observations of Nebule and Clusters of Stars. 
G.C h. & H. —— 
2755 1110— | 1850, Apr. 13. E np sf, 88” by 50’. (1. obs.) 
I, G8 
2756 | 1111—) | 1851, Apr. 26. h1111 has a B, R centre with 
Ey IMGs) ( Nucl, then two dark spaces concentric with 
ZOGO || WINGS | the Nucl and outside these F neby as in figure. 
Tl, 642 |} 1113 has a F Nucl or stellar point. 
aN Pos. 175% Dist: 145” 
a fa 181 58 
ay 202 181 
ao 63 227 
1851, Apr. 28. Previous observation rather con- 
firmed. ‘The dark spaces certainly exist, but 
I cannot be sure that appendages are not parts of spiral branches. 
1852, April 15. Last year’s observation confirmed as to dark curved spaces 
p and f centre and F neby outside them again. [P. T. 1861, Pl. XXVII., 
fig. 20.] 
1858, Apr. 15. Nucl and centre round it v B, but the neby outside it is vy F 
and diffused, and the details of the drawing barely traceable. h 1113 is 
F and bMN, brightest part E nearly p and f. 
1861, Apr. 13. Nucl vB. Hither like an S reversed or with a ring round 
Nucl'and joined to it on sp side. (V. obs.) 
2757 1112— | 1876, Mar. 18. pB, pL, ir R, vgymbM. Seems r. Probably sharper on np 
101, 88 side and more diffused, fading away on sf side, where it seems flattened. No 
stars near. (II. obs.) 
2765 1117= | 1854, Apr. 25. Did not appear E but R with Nucl and a * iny f Nucl, also a 
IT. 353 S * at a little distance np. 
1855, Mar. 15. B Nucl; HK nearly ns, * exactly f Nucl and nearly touching 
the neb. 
1878, Apr. 18. irr E pf, bi N, quite of a resolvable character, the nuclei being 
quite stellar. * 10m sp, Dist. 1563, * 11-5m nf, Dist. 65'-9, * 14m np, 
Dist. 61"-8. (LV. obs.) 
2768 | 1119= | 1855, Feb. 17. vB, R,bM,2stp. (1. obs) 
IT. 105 
2769 | 1120— ) 
II. 372 | 
BOO, |) LPs | 
5 » | 
2772 Feces | 1849, Jan. 28. Viewed in haze. (1. obs.) 
IT. 359 
2773 |1124— | 
ITI. 360 J 
2774 3383— | 1873, Apr. 25. Not found; slight haze [not observed by d@’A. Low set, 
IIT. 534 NPD=103°]. (Once looked for.) 
2779 1128— | 1856, April 6. F,bM,a B * in sf edge and a patch in np end which is the 
III. 697 brighter. Neb is fully 4' long. 
1862, Apr. 22. Dark space p the * in the sf edge? Not well seen. (II. obs.) 
BVM WIAD }) | 
IT. 373 | | 1851, Feb. 26. The larger is vIbM, perhaps not R; the S one r? 
2790 | 1136=— f 1856, Mar. 26. The p one is pL and pF, R,bM. h 1136 is about 18’ sf, v B, 
S, R, and I suspect it to be a Cl. (IT. obs.) 
