126 Observations of Nebule and Clusters of Stars. 
G. C | h. & H | —- 
3459 1564— | 1851, Mar. 1. vB centre, neb extends to a * sf? An appendage p. 
1.57 | 1858, May 3. Has Nucl and is E np sf, I see an appendage p. I also think I 
see a neb knot sf, in the direction of major axis of neb, but was interrupted 
by clouds. 
1862, Apr. 19. The patch p is v F, yet distinctly seen as far as in sketch [PIl. 
IIT., fig. 12], but I suspect it joins n end of neb. Nucl is nearer the p than 
the f side, the p side is also sharper than the f side. (III. obs.) 
3462 IT. 816 | 1867, Mar. 1. vS, stellar, b M. (1. obs.) 
D472 1569= | 1851, Mar. 1. Brighter st well separated, perhaps some unresolved neby. No 
Wik a spiral arrangement. 
1855, Feb. 19. Much unresolved milkiness about it. 
1855, Apr. 19. Cl, no neby remarked. (III. obs.) 
3474 1570= | 1850, Mar. 9. Another fine and B spiral. | 
M. 63 | 1855, Apr. 13. I can detect no spirality, but see indistinctly a darkness sf 
Nucl. Neb is E pf. 
1857, Mar. 24. No trace of spirality ; L, E nearly pf, sharp Nucl, s edge the 
best defined, on all other sides it fades away very gradually. I suspected a 
diminution of light just sf Nucl and perhaps reaching past s side of Nucl. 
1861, Apr. 13. Suspect a lane s of Nucl or rather F neby beyond edge. Ir 
shape. (VY. obs.) 
5730 .. + | |1855, Apr. 18. The s of these is p B, perhaps 1 E ns [h 1576], the middle neb 
3485 | 1576— [h 1578] is v F and flickering, the n one [h 1577] p B, 8,1 Ens. About 
DOC, Nes 12’ nf (Pos. 25°+) from the n one is another [3489] H nearly ns and pgm bM 
3486 | 1577 | but not well seen ; Mr. Stoney suspected a curved branch going p from n 
INL, UGS | end ; neb about 24’ 1. About 7’ np the B neb is a 8 neb [5730] with aS * 
3488 | 1578=— | | 20" sp [should be nf, see obs. in 1878 which agrees with d’A. ]. 
TIT. 118 | 1857, Apr. 24. n one is pS, 1E, mbM, * in s edge, middle one is F, E, no 
3489 | R. nova J Nucl, s one vS and F. About 12’ nf the n one is a fourth neb, E nearly ns, 
| has Nucl. I suspect others in the neighbourhood. 
| 1873, Apr. 20. 3486 is B, cL, E * 13m Pos. 139°:3, Dist. 59':9. 
3486 to 3488 Pos. 148°:3 Dist. 171'°7 
3488 to 3485 216°8 189-4 
1878, Apr. 21. Measures from 3486 : 
*8m Pos. 274°°4 (2), Dist. 486-2 (2) 
3485 185°6 320°1 
3488. 147-7 182-9 
3486 is p B, irr, bi N ns, s Nucl the fainter, 3488 is ¢ E ns, diffused, 3485 is p F, 
S, brighter than 3488. 3489 is 10’ f and 10'n of 3486, F, E ns, cometic. 
5730 is p B, vS, stellar, * 14m nf, sey vy F st near, * 8m (same as above) 
Pos. 207°°5, Dist. 430-1. (V. obs.) 
3495 1580— | 1854, Apr. 25. R,bM. (II. obs.) 
Il. 327 
3500 1582 1878, Apr. 4. pF, pS, R, very soft and vglbM, * 11m Pos. 
216°-3 (3), Dist. 102"-4. (I. obs.) 
3507 1586= | 1858, Apr. 15. AS, B sharp ray, E np sf, mottled, brightest part in np end 
IIT, 619 unless there is a continuation np the latter, as I suspect. (1. obs.) 
ddI] 1589— | 1856, Mar. 30. Sketched, sf branch very doubtful. 
II. 646 | 1856, Apr. 29. The B centre is E, but not quite in the direction of the neb. 
The F neby f does exist ; I suspect the centre is r, the whole neb is much 
mottled. 
