5A Observations of Nebule and Clusters of Stars. 
G. C. | h. & H. | secu 
1442 403— | 1856, Dec. 28. Rather R with rays. (I. obs.) 
VI. 21 
1444 404— |1856, Jan. 10. Cl of S st, oblong nearly pf, contains about 30 to 35 st. 
VI.3 | 1857, Jan. 20. v irr, not remarkable. (II. obs.) 
1448 406— ) 
II. 615 || 1849, Jan. 27. Southern neb. has Nucl., 6 S st between them. 
1449 407= {| 1849, Feb. 20. sneb. brightest, S * close p, another sf the n one 
II. 614 J and 3 or 4 others bet the neb. 
1850, Feb. 3. Dist. about 3’, n one the brighter. 
1850, Dec. 11. The s one has a stellar point. 
1851, Feb. 26. South one has a dull Nucl. 
1855, Jan. 18. The s one issb M, F* inv p centre? 
1856, Jan. 29. Thes one the brighter, I susp. stellar Nucl. and a * closely p it? 
Both neb. I think r. (XIV. obs.) 
1453 408— | 1858, Jan. 13. A few larger st in its borders, not at all striking. (I. obs.) 
VIII. 31 
1454 411— | 1851, Nov. 25. Coarse, B Cl, most of the st from 10th to 12 mag., a few of 9th. 
M. 41 A spiral arrangement of some of the st is conceivable, (1. obs.) 
5369 Recs 1849, Feb. 22. 5 neb. in one field. 
1455 Mt | 1850, Feb. 3. a, B, y are p B, vvS, « ee F, 6 eee F. 
1457 410== || 1850, Dec. 8. a and y are the brightest and have Nuclei. 
ITT. 898 Pes. Dist. 
1458 409= ay 344°+ 152” 
IIT. 897 a B 324-0 106 
1460 ete a Od 4:5 308 
ae 31:8 371 [Es 
1856, Jan. 29. Group seen, some dist. p I found F, vS neb. [either 5366 or 5368]. 
1857, Feb. 14. ais1E sp nf, B is the smallest of the group and y next in size. 
These 3 seem to have nuclei. 6 and « are larger, the latter being ] Ens; it 
has a F nucl. ? 
1874, March 7. ais pB, 8S, R, smbM toa starry nucl., B isc F, 8, R, y isc F, 
SR ouseb: 
Pos. Dist. 
a 324°°7 107'-6 
a 341-8 (2) 162-2 (2) 
a to * p (nebulous ?) 300-1 149-1 
ato*s 156°6 65:5 
ao} 1-4 325-7 
1874, March 10. 
aispB,pS,R,shbMSN. BvF,S, BR, ypF, pS, R, bM, 
has * 12m.n; deF, L, R, IbM, ee F, L, c KE 0°, amongst st. 
Pos. Dist. 
a B 326°°9 104"°3 
ay 342:5 155-3 
ao 4-6 315-6 
ae 26-7 368°8 
a to *9m. 356:2 481-0 
ato* 9:2 m. 171°5 181-4 
The last * is the f * of 3 forming a rectangular A, the others are about 11 m. 
Searched for other nebul as far as 11'n of group, but could see none ; there 
are 2 § and insignificant clusters of ySst. Many st through the group. 
[The identification of this group in the G. C. is wrong. y=h 410 as already 
pointed out by d’Arrest, a is nova=5369, 6=h 409, a and y may be=III. 
897 & 898, as H. says these are np and sf. Adopting d’Arrest’s place for 
h 410 we find from the measures made in 1874 the following positions for 
1860-0. 
