Observations of Nebule and Clusters of Stars. 83 
sa nan | a 
1856, Mar. 8. Seen as in last obs., but with only the same suspicion of a F branch f. 
1858, Feb. 16. I think I see as before a v F branch f and a S * in it. (LX. obs.) 
2056 690—= | 1874, April 5. vF,clL, R, gbM, * 15 m. near the middle and sev S st near 
IIT. 910 (within 2' or 3'f) but does not semr. * 14 m.p2’. * 14 m. Pos. 327°-4, 
Dist. 36'°3. 
1878, Mar. 31. A pL nebulous looking object with sev st 13:14 m. in it. 
(II. obs.) 
209 | 1850, Jan. a and y probably con- 
2055 ‘|R.nove. nectedand F nebyprobablyextend-| 7) ff J 
2057 ing to the right of a. In y sev f G 
2058 | 692— minute st seen by Lord R. f- 
IT. 44 1850, Mar. 15. 
2061 693— Pos. Dist. 
II. 45 a B Bil (2) Sy” (2) 
ay 301 310 
aé 216°5 647 
[a = h 692, 6 = h 693, y = 2055 6 = 2054, « = 2057.| 
1856, Mar. 1. Is the Nuel of 6 excentric? 
1857, Mar. 22. Sketched. 693 has its edge ragged and ill defined, I am 
nearly certain I can see its centre to be composed of st. In y I also saw B 
points at intervals, it is E and vF, 6 is ill defined, nucl near f edge; 3 
stellar points in it? [See P. T. 1861, pl. XX VII, fig. 14.] 
1873, Dec. 27. h 692 isv B, L, vm E,svmbMN. In the direction of Elong. 
is a F neb np = 2055, also c E in the same direction, so that one appears to 
be a continuation of the other, although there is no visible connection. The 
F neb makes a A with 2 F *. 
h 692 to 2055 Pos. 302°:7 Dist 296"-0 [or p17 -96, 159”-9 n 
h. 693 50-2 (2) 352-7 (2) [orf 19°54, 225-8 n 
2) am (atl 349-0 (2 500:3 (2) for p 6-88, 491-1 n 
( p 
* 15m 250-1 (2) 71:7 
h. 693 is v B, p L, 1 E, vm bM, * 9:5 m. Pos. 353°:9 (2), Dist. 80-6 (2). Sky 
hazy. [* 9 m. is B. W. 10" 202-203, not in Birmingham’s Cat. of red stars. 
Pos. for 1860-0 is 10" 10™ 14°56, 67° 19’57’"75.] (XI. obs.) 
2066 695— | 1850, Mar. 3. Probably F spiral. 
1851, Mar. 5. * in fend, light very unequal. 
1855, Mar. 12. m EH, sb MRN, perhaps a dark vacuity ssp Nucl? 
1857, Mar. 24. F, light very uneven, * in fend, dark spaces throughout its 
length. (V. obs.) 
| 
| 1855, Feb. 16. These 3 form an obtuse-angled A, the p one has 2 st closely n 
100, Oil. (7 and nf and is B, R, bM. The next is much like the p one and has one * nff. 
2074 700 = | The 3rd neb is much less bright and1E pf. (1. obs.) 
It. 722 ) 
2071 698 1855, Feb. 14. Too F to make anything out of it, almost invisible in finder-eye- 
piece. (I. obs.) 
2073 697—= | 1874, Mar. 9. pF, 1 eH 45°+, rr. * 11m 2/nf, * 13 m Pos. 350°+, Dist. 2". 
I. 266 (I. obs.) H 
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