Observations of Nebule and Clusters of Siars. 
Sa 
Ot 
G. C. | h. & H. | — 
[In the Gen. Cat. y is supposed to be h 582 and d—581. About the latter 
there can be no doubt, while it is doubtful whether perhaps not a is=h 582, 
but even if this was the case, the positions in the catalogue would be nearly 
right except those of 1811, 1812, and 1815 (y, 8,a). The N PD of 1813 is 
wrong ; it should, according to h’s identification, be 55° 38' 56”, while 
1809 = 1807 and the place of 1804 should be about 9° 11™ 9°, 55° 45', being 
the e F neb. nf 1807. ] 
1823 584— | 1849, Feb. 20. In general appearance very like Neb. in 
I. 205 Andromeda, f edge is perhaps sharp, extensive to 8. 
1850, Dec. 5. Nucl. a little nearer f edge than centre. 
1852, Jan. 20. gvmbM, 2st in np end of which the 
brighter seems to be on edge of neb. 
1860, Mar. 25. pB, Nucl., a little to the s. I think there 
is a 8 part of detached neby which seems to have a con- 
nexion with the other. (VI. obs.) 
1825 III. 64 | 1877, Feb. 15. vF,vS neb. 50+ nfa * 12m, 53'n of a*8 mag. (LI obs.) 
Q 
1826 | IIT. 628 | See 1831. 
1829 587= | 1855, Mar. 15. More R than H, but v F and outline indistinct ; F knot np 
IIT. 488 and a triple * nf, B * a little more distant nf. [PI. IIT., fig. 1.] 
1878, Mar. 25. vv F so that its shape remains doubtful, v dif, * 13-14m inv. in 
n end, * 11:12m 3’ nf. (II. obs.) 
Nova sted 1874, April 4. 9° 13-4, 104°-4, * 11m invS, p B, Rneby. 
Usimn, o JOS, IOS" Dist. 6-9 
Orin, 152-0 266°5 
Sa eOTIN 152:9 429-3 
1878, Mar. 25. 9"14™+ 104°-2+. I think it is onlyavSCl. I do not see 
any * as Bas Ilminit. * 11:12m Pos. 155°-6, Dist. 266':5, * 9m nearly 
same Pos., Dist. nearly double ; * 13:14m 2'nf. (II obs.) 
1831 588= | 1851,Feb. 26. Nucl., nothing particular, 2nd not seen[viz. 1852—h590—ITI. 630; 
Til. 629 most probably, therefore, 1826=IIT. 628 was mistaken for h 588]. (I. obs.) 
1833 589 = ) | 1856, Jan. 9. Both oval, their larger axes -— 
IIL. 714 | at right angles to one another, p one 
1834 | R. nova > susp. patchy. About 7’nf the n one 
1836 Hil | is another, p L, slightly oval, f 4S st, 
IIT. 713 } mottled, * susp. in its centre. Is there 
about 5'f this latter another v 8 knot 
with 2st p&n? qyiD 
1858, Mar. 11. Both E & IbM, in the = 
n one I susp. a * on p edge and another near its centre. 
1867, Mar. 5. Between clouds, Pos. 38°-5, Dist. 202". (IV. obs.) 
1835 592—= | 1858, Mar. 9. vv F disc, much and suddenly bM, but no sharp Nucl. ; has 
I. 132 F st on its edges. 
| 1866, Feb. 17. R, B Nucl., st in edge not seen, sky bad. (III. obs.) 
1837 993= | 1855, Feb. 14. Like h 476, sbM, stellar points in outlying F neby, especially 2 
Ih, Lasts which I can plainly see at moments with $ inch single lens. 
1857, Feb. 23. Looks very like a Cl., but I cannot resolve it. 2 F st on 
its edge. 
1861, Jan. 15. R,v B Nucl., fades off rapidly. 
1861, Mar. 28. Dull Nucl., I susp. a dark ring round it. Av F neb. nf. I 
strongly susp. st in h 593. 
1876, Mar. 17. p B, pS, vsmbM. * 8m in Pos. 289°-75 (3), Dist. 376'-7 or 
p 28°88, 127-0 n. [Adopting the place of the *, given in Vol. VI. of the 
Bonn Obs., we find the place of 1837 for 1860 9° 15™ 44°75, 54°53’ 18"°5.] 
(XI. obs.) 
