Observations of Nebule and Clusters of Stars. 139 
G. C. | h. & H. | ——- 
1855, May 16. The n one is m EH, and 
seems to have a knot or * in p extremity, 
which makes it sometimes look double ; 
nova is visible f, p L, vv F. 
1878, Apr. 26. The p oneis pB, E pf, not 
as L as the f one, * 13:14 m 2’np; f one 
B, L, m E ns, centre v B and R, * 12m 
Pos: 90°-6, Dist. 94:7, * 13-14m Pos. 
253°-2, Dist. 89-9. [The 3" neb in the 
diagram does not seem to be the same as 
the one seen in 1850 & 1855.] (VI. 
obs.) 
3850 
has Nucl; 16’nf 1783 there is a L, F ray 
about 43’ by 1’, gvlbM. [Dist. is only 
about 10’, RA of 3855, therefore 1™ too 
great, as found by D’Arrest. | 
1850, May 12. 1782 is pB, L, gbM, 1783 
is v B, R, Nucl; Nova p B, D * close p, * 
in nf edge. 
1851, Apr. 7. Both bM, p one E pf, 2" v8, 
K, r? 
1878, Apr. 24. 3850 & 51 in Pos. 44°-4. Dist. 162'°7. 
3850 to * 14m Pos, 297°-1. Dist. 162"°7. 
3851 to * 12m 315°9. 71:4. 
3855 is vF, lenticular, vm E 53°-2+, 3'long, * 11m 54! sf, * 13-14m 2/np, all in 
one line. (V. obs.) 
ee 1849, Apr. 26. 1782 is B, E, 1783 vB, R, 
3851 t 
| 
J 
3855 
3854 1786— | 1865, Apr. 26. BNucl., forms a quadrilateral with 3 st sp, sf & f. (IL. 
II. 754 obs. ) 
3856 1790= | 1854, May 15. pI but vF, 1bM, fades off very gradually. 
I. 235 | 1864, May 4. vgvmbM, pL, edgeseF. (II. obs.) 
3858 1789 || 1855, Feb. 19. Saw only 2, both pB, R, bM. 
3859 1788= | 1855, Apr. 13. Isee but 2 neb nnp ssf, both 8, R, bM. [As remarked on p. 34 
of the G. C., it must have been h 1789, e F, which escaped the observer's 
3860 | 1791=— f attention. This group has not been observed by anybody else after h.] 
IIT. 417 } (IT. obs.) 
3864 | 1792— 
ITT. 121 
3866 1793— 
TIT. 122 
1852, Apr. 14. Both F. 
1858, May 12. 1792 isl1E npsf, vF,bM. I am nearly sure I saw st in it. 
1793 has a more condensed centre, but is also vF, and I suspect a * closely 
fits centre? (II. obs.) 
3867 ne 
III. 733 (| 1867, Mar. 27. One or perhaps 2 novae; 2°? one may be a *. [First 
3871 | 1800= nova = 5770.] (I. obs.) 
IIT. 734 
3869 | 1797—= !1856, Mar. 28. pB. The brightest part seems to lie nearest the f edge & to 
IOI, Were extend from that round to the n. S$ * p. 
1856, Apr. 29. A Cluster? Edges filamentous, centre vB. I suspect the 
brightest part to be curved. (II. obs.) 
