170 Observations of Nebule and Clusters of Stars. 
G. C. h. & H. — 
4879 2199= | 1854, Sept. 16. * in np edge unmistakeably seen. Sharp stellar point or * 
II. 251 seen in centre of Nucl ? 
1873, Oct. 20. Slightly concave towards p side. 166°-6. * 10-5m Pos. 100°:8, 
Dist. 1506 [B.D.+15°, 4742]. Two st 15 and 14m p, the f one in Pos. 
310°°6, Dist. 141'-1, 
USS Sey NOS fol, 1b, md) WAI, iin Ios, WOO, IDrise, U4"o7 (). 
(VI. obs.) 
4880 TI. 249 | 1875, Oct. 23. pF, pS, gbM, * 11m Pos. 296°-8 (2), Dist. 54-2 (2). A * 13m 
about 70 n. Clouds. (I. obs.) 
4883 2201= | 1851, Aug, 24. E np sf, S * p inv. 
IT. 212 | 1854, Oct. 16. E npp sff, * exactly p Nucl inv, neby extends probably a good 
way allround. B Nucl. 
1862, Sept. 20. I am almost sure the centre is r, I could see one * plainly at 
times, itis]E. [Pl. Y.] (V. obs.) 
4884 2200= | 1856, Sept. 6. F,urR,bM. (II. obs.) 
If 590 
4886 | 2202= ] | 1860, Sept. 17. Found 3nebfaB*a. fis Epf, y is 
III, 210 R and I suspected a * in it [=6112]; I thought 
4887 | 2203— once or twice that 3 and y were joined at the f end. 
TIT. 211 | 6 like a * in haze, while a and the 3 st at <« are quite 
6112 Aa sharp. 
1860, Sept. 22. 6 is F, Epf, y v F and at times I 
thought it jomed to 6. 6 is p B, R, bMN. 
1875, Sept. 10. Seen for a short time, 4887 seemed the 
faintest. 6112 F, 8, E in same direction as 4886 (sppnff). * 10m Pos. 
233°°9, Dist. 153-4 from 4886. 
1877, Oct. 29. 4886 to* 10m Pos. 230°:8 Dist. 153"-0 
6112 135°5 40 estim. 
4887 115:2 207-7 
4886 is EH, 6112 is e F, vS, vl E, 4887 F, vS, R. (IV. obs.) 
4892 2205= | 1849, Sept. 10. Spiral, but query whether this is not more properly an annular 
T. 55 than, a spiral neb. [P. T., 1850, Pl. XXXVI. fig. 4; ibid. p. 511: 
‘Observed frequently, and by many friends. ‘he drawing represents the 
object with considerable accuracy.” Several rough sketches have been made 
since 1850, but in none is the faint spiral appendage p shown as distinctly 
as in the published engraving. | 
1850, Nov. 26. In centre of f part there isa Nucl. The p branch seen indis- 
tinctly. * in n end from * p, Pos. 23°, Dist. 106”. 
1854, Aug. 31. * p is nearly central with regard to the spiral convolution. At 
times Dr. Robinson thought he could trace the latter round to f the *. Sky 
bad. 
1860, Oct. 19. Sev st through it, especially in Nucl. I saw occasionally the 
bend round the * p, but could not say positively whether it is eaveloped or 
not. 
1860, Nov. The * n is not inv, I think; the F * p may be nebulous. 
1873, Sept. 22. * llm n, Dist. 77'-4, there is also a B * n, about 3’ dist. 
1875, Sept. 28. Not well seen, sky hazy. * 10-11m Pos. 195°-7 (2), Dist. 
202''5 (2). The e F * n of Nucl seems nebulous. 
1876, Oct. 10. The F * np Nucl, which I last year thought nebulous, was 
barely visible, Pos. 329°-9, Dist. 49-6. * 10m, Pos. 195°-1, Dist. 201'1. 
No details seen. (About XX. obs.) 
4893 2206 1855, Oct. 7. Perhaps 1E pf, centre B, looks like a * seen in haze. (AI. obs.) 
