82 Observations of Nebule and Clusters of Stars. 
G.C h. & H. | Sata, 
2024 674—= | 1861, Sept.9. v B,v L, E, stv F. Hithera v F* or knotat a. 
i, 7 I susp. a lateral extension at 6. (3 ft. telescope.) (I. obs.) 
2025: 675  |1849, Mar. 14. S * at sp edge of neby. (IV. obs.) 
2026 677 — | 1854, Mar. 30. vF. (1. obs.) 
IIT. 53 
2028 | 680 = | 1877, Mar.7. pB, pL, irr Rorvl1E. *10-11 m Pos. 115°°6, Dist. 130"-2 [or 
If. 255 78 f, 56-38; d’A. has 7-7 f, 45"+s]. (I. obs.) 
2030 678— )| 1854, Mar. 27. 3 neb, p one v S, about 4'f is a S lenticular ray, Esp onuf, and 
IT. 639 | about 5’ south of the latter is another neb, R, both have a resolvable 
appearance. 
2031) |p | 1876, Feb. 27, vB,v§S, stellar, vsmbM. Av F, v8 neb, | E npsf in Pos. 
HOBD|f | PN 10°-2, Dist. 290" [or f 4°4, 285’ n]. There is a *13 m bet the 2 neb, nearer 
the nova ; p the latter is an e F, v 8, i R neb (with ane F* close sp), looks r, 
in Pos. 331°-9 (2), Dist 347'-2 (2) from 2030 [or 14°8 p, 306’ nj]. These 
2S neb must be 2031 and 2032. (AI. obs.) 
2034 682— | 1850, Jan. 16. S nucl, light unequal. 
II. 43 | 1852, Jan. 27. A F spiral. 
1854, Mar. 20. F* immediately f, spiral left-handed, spirality very faintly seen, 
night bad. 
1855, Feb. 19. I fancy I can trace spirality as previously suspected ; certainly 
a slight condensation from n round f edge. 
1856, Jan. 9. Centre B and neb certainly patchy. 
1857, Mar. 22. Mottled. Nuclalp centre? Suspect a * or knot in np edge. 
| 1860, Dec. 16. e F * v1p centre seen by glimpses, another * sf seen steadily, 
ee F neby round towards the latter. 
1864, Mar. 9. Clearly r, centre composed of sev st. 
1877, Mar.17. * 10m. Pos. 264°-3 (2). Dist. 200"-9 (2). * 13 m. I’ sff, to 
which the neb possibly extends. (XIV. obs.) 
2037 | R. nova. \} 1852, Mar. 18. 684 is probably r, both are B. 685 has sf edge the best defined 
2038 684—= and fades off gradually at np side of centre. 
1.3 »| 1855, Mar. 15. p neb is p B, R, smb M. S * sf to which it nearly reaches, f neb 
2041 685 | is sharper at sf edge and fades off np, spreading out in that direction. 
I. 4 J] 1856, Jan. 30. About 5' sp 684 is avv Fray extendingns. Previous obs. correct 
as to shape of 685, but is there perhaps v F neby beyond the well defined sf 
edge? 684 has B central Nucl. with a sensible disk. 
1857, Mar. 19. 684 is oval, * sf. nova is vv F. E. vib M. [PI. II, fig. 4.] 
1868, Mar. 13. Both certainly mottled. (VI. obs.) 
2051 I. 265 |1874, April5. c Borp B, pL, R, psmbM N=* 14 m. 
* 13m Pos. 217°°8 Dist. 85"-1 
* 10m 568 1445 
*11m 2! further off nf in same direction. (I. obs.) 
Nova 1851, Jan. 25. 25's and a little p h 688 I found a 8, R neb, r, near 2 st almost 
2049 
20505 Re neem 
2052 
in a line with it. 
1852, Mar 13. 8S, Nucl. sp 688 about 20'. (II. obs.) 
1851, Jan. 25. Is triple, neby perhaps extends round them all as far as the * n. 
| h 689 not seen [is—688, see the Suppl. to the G.C. p. 391]. 
688— {| 1851, Feb. 26. p part probably portion of a ring. 
I 168 j| 1856, Feb. 1. The neby connecting the 3 principal knots is vv F but I have no 
doubt of its existence. The F branch f the B nebis more doubtful. [See P. 
T. 1861, pl. XX VII. fig 13. where for h 689 should be read 688. | 
