Observations of Nebule and Clusters of Stars. 109 
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G@@ || W&Ub == 
1861, Apr. 13. [See Diagram.] 1088 ism E, Nucl also E, susp r. The p edge 
is sharper and I think v F neby parallel to the neb just beyond the edge. 
Ata there seems a twist and neb is there a little brighter than nearer the 
Nucl. 8 F,8 [5618], y 1 E, B Nucl [h 1091], ov F, v8 [5619]. D * yellow 
and blue. (LV. obs.) 
2728 |R. non | 1851, Mar. 6. h1092hasaNucl. Another also E and v F, about 18' sp. 
9733 | 1092— “| 1855, Apr. 18. 2 neb about 14’ dist, 45° nf. Is the sp one of this shape 
V.4 ) with a wedgeshaped division runing downwards? The nf neb is (\) 
oval np sf, has Nucl and is the larger and brighter of the two. "3 99) 73 
the Nucl. 
1856, Mar. 29. 2 neb. 14’ dist. Last year’s observation confirmed as to the 
shape of the s one. The n one is however a spiral hike an S, the arms being 
F, (IIL. obs.) 
2734 1094— | 1851, Feb. 26. A long ray very much resembling h 242. 
LT. 33 1856, Mar. 26. mE, B Nucl. extremities F. 
1872, Mar. 6. vg bM,m E118°-2. * 11m. Pos. 312°-0 (8). Dist. 124"-8. 
1878, Apr. 4. m E 110°-2, * 10m. Pos. 312°°5, Dist. 1790. [The discrepancy 
between the measures probably arises from the circumstance that the neb is 
E towards the *. There may, however, be an error of 1 rev. = 65'-1 in one 
of the distances.| (IV. obs.) 
2744 1108— | 1850, Apr. 13. * sf Nucl, light perhaps unequal ; night bad. 
TI. 321 | 1855, Apr. 17. Has a B, R Nuel surrounded by much F neby, which is patchy 
and involves a B *. 
1856, Mar. 7. Not B, but pL and bM. The neby reaches toa S * sf. xr? 
(III. obs.) 
1.196 | 1868, Mar. 27. Patchy appearance, E nearly n ands (in the direction of a * n). 
No distinct details, v F connection bet neb and B * n suspected. 
1872, Mar. 12. psmbM toa Nucl which is slightly EH 151° 5. Nucl. seemed 
a little mottled. * in Pos. 338°°5 (4), Dist. 56-9. 
1874, Mar. 9. pF, pL, R, glbM. 
bo 
“I 
nS 
Cr 
* Om. Pos. 42°-4 Dist. 389''-8 
* Om. 327-6 DATE 9 en (ulilegobs)) 
2748 1104— | 1874, Mar. 9. pF, S, R, psbM to asoft Nucl, * 13m about 22'p nearly in 
JAY5 OLS parallel. (1. obs.) 
2749 1107= | 1849, Mar. 15. Pos. of E about 100°+, S * about 3's of middle. 
Il. 747 | 1850, Mar. 9. Long ray with unequal light, and probably a tendency to an 
annular arrangement about Nucl. (II obs.) 
2750 1105— | 1852, Feb. 24. vF, * 14m sp. 
[. 169 | 1855, Apr. 10. Badly seen through clouds. It appeared L but F and of irr 
shape. 
1855, Apr. 13. pB, R, bM but no Nucl. (IV. obs.) 
2751 R. nova | 1848, Apr. 1. AS neb, R A 3™ less than that of h 1106, same N PD. 
1877, Apr. 4. 3™ 3°5 p and 35”'s of 2752. F,S, * 3'p and a little n, another 
3’n, D * in Pos. 189°-5, Dist. 329'-5 (centre of D * from the neb). [Place 
for 1860-0 11" 59™ 52s, 70° 40’ 52'.] (AI. obs.) 
2752 1106= | 1848, Apr. 1. A very close Cl of faintish stars. 
J. 19 1872, Mar. 8. Glob. Cl, completely resolved, B * 40's and slightly p. 
1877, Apr. 4. Glob. Cl, more scattered than most such, 4 or 9 st outlying very 
conspicuous, especially one s and one p, sev f. 
1878, Mar. 25. Badly seen, B part like double, outlying parts v F. (V. obs.) 
