104 Observations of Nebule and Clusters of Stars. 
G. C. h. & H. = 
2606 1011= |1851, Mar. 3. Lenticular, mottled. S neb, v F, 6’npp [not noticed since, would } 
V. 45 be a nova, if a real neb. | 
1856, Mar. 30. m Esp nf, B Nucl, very much mottled. The larger half of neb } 
lies to south of Nucl. A B streak obliquely through the Nucl and another 
B patch inthe send. Av F*n of the * nf Nucl? 
1856, Apr. 6. There appear to be two patches ins end, also a * ssf Nucl. 
Perhaps F neby reaches through the * p Nucl. 
1857, Apr. 19. Sketched [P.T. 1861 pl. XXVII., fig. 17]. (IV. obs.) 
-11852, Apr. 14. South one is E and hasa *n; the n nebhas 2 st inv. (I. obs.) 
2616 3370— | 1873, Apr. 25. pB, pL, R, gmbM. 
It, O0 Pos. Dist. 
* 15m Dil Bos) 88'-0 
3 Qebyran 200-1 (135-7 
* 10m 157-0 192:6 
* 12m 135°3 170°1 
* 12m 91-2 164-1 (1. obs.) 
2617 1016 1874, Apr. 14. pF, pS, R, psbM to a stellar Nucl.=*14m. 
Pos. Dist. 
* 10-5m Doweilh 54-3 
* 10m 242-1 176°3 
1876, Mar. 22. vF,vS, R. 
Pos. Dist. 
* 11m 25°-1 (2) 60°4 (2) 
* 10-llm 239-6 173°4 
The first * is not attached. (II. obs.) 
1868, Feb. 29. At 33° 59’+ PD and 6'+ p 2620 found a ray, H 130° (by 
estimation), * sp, two st (nands of one another) f and nff. 
1878, Mar. 31. sp one E120°-5 and p B, nf one F, R, Pos. Simp DIStaO Olds 
[This agrees well with H.’s description : “Two neb, the first p B, H, the 
second F,8.” d’A. and the observers in 1866 and 1868 have only seen 
TI. 789.] (III. obs.) 
2618 | IL. ie 1866, Apr. 8. L, E, bM. 
2619 | II. 790 
2620 1017= | 1854, Mar. 27. Filamentous, r, * near centre. 
TV. 62 | 1868, Feb. 29. Irr outline, patchy, * ssp, * susp. on Nucl. 
1873, Apr. 1. B, cL, R, mbM, rr. Definition not good, but feel sure that it 
is a glob. Cl. 
*10-5m Pos. 204°-2 Dist. 214-5 
* 12m 188-7 208-1 
* 15m 222°6 183°8 (IIT. obs.) 
2621 | LOLS= 1855, Mar. 15. pF,R,sbM. Nova nf. 
Il. 162 1856, Jan. 10. pB Nucl. ina L mottled disc of F neby, ir R. 
1876, Apr. 16. p B, pL, R,gbM. * 10m, Pos. 66°-0 (2), Dist. 170’8 (2); np the 
2622 |R. nova * in Pos. 318°:6, Dist. 56” is an ee F object, most probably an eS neb [2622]. 
