Observations of Nebule and Clusters of Stars. 
79 
89 
90 
| =III. 476) 1857, Oct. 23. p F, R, 1b M. 
1852, Aug. 24. eF neby. involving some stars, one of 12 or 13 m. Neb. is 
E nnp ssf, and perhaps about 8’ or 9’ long and 5’ or 6’ wide. Do not feel | 
satisfied that it is Herschel’s object. [Could it be 909] 
1852, Sept. 16. Sev. st. besides h.’s in middle. Spirality not detected, but 
night much disimproved. (V. obs.) 
30 1854, Dec. 9. R,pL,bM. (I. obs.) 
II. 478 
32 1857, Sept. 20. F,S, R, b M. See no comp™ [See note to 82.] 
1866, Oct. 16. The p. neb. is sbM. ff. neb. follows 14’. *7:8 Pos. 14°.+ 
Dist. 5’. [This “f. neb.” is evidently the same as was seen in 1874. 
1874, Nov. 5. Neb.witha sharp nucl. *8 m. Pos. 16°5 (4). Dist. 259-3. (4) 
N. f. the neb. is a v. F. * or neb* knot in Pos. 74°-0. Dist. 69'-9.(1) [Seen | 
by Schultz, and taken for G. C. 80.] | 
1874, Nov. 6. *8.9. Pos. 17°:2 (3). Dist. 2597-3 (23)*. An eS, F neb. point, | ° 
| or probably a F. * nf 79 in Pos. 78°-0. Dist. 718. 
| 1875, Oct. 9. v Fin moonlight. *7 m. Pos. 18°°3 (4). Dist. 257''-9 (4). 
| 1875, Oct. 23. *7 m. Pos. 18°-7 (3). Dist. 255-6 (3). These measures are 
bad, as the neb. was e F in the exceed. misty sky. (VII. obs.) | 
| 1857, Sept. 18. AvS, D neb., the n. one is Espnf,bM. [The observer mis- | 
| took this for h. 32, in consequence of which G. C. 80 was entered as a “‘ Nova | 
| R.” There is a small diagram exactly like the one made on Oct. 22, 1857, 
| and the position of the B. * shows clearly that 82 and not 79 was observed | 
on both nights. | 
1857, Oct. 22. D.neb., a is mEpf,bM. £6 is 1 E nearly oad 
ns., b M. : 
1866, Oct. 8. Close D. neb. 2 st., one nf 2’ and another sf 1’ / 
and a *7 mag. 216-8 dist. The nebule are 33-9 dist., both 
E. and inclined perhaps in the f. direction. * p. 99-0 distant. | @ “4 : 
1866, Oct. 15. Both E. at right angles, the line p and f bisecting ce 
the angle between them. ‘Three nebule in the field, perhaps 
more, which would be worth examining on a good night. The 2 st. 6 and 
7 mag. can be seen in finder together. 
1866, Oct. 16. Closely double or with two knots, the dist. being }’. 
1874, Noy. 6. D neb., or perhaps an E neb., with two nuclei n and s *6.7 
mag. in Pos, 63°-4 (2). Dist. 234/”3 (2) or 15°. 19 f., 104-9 n. of the centre 
of neb. [* = B. w. 0" 757 and the place of the neb. for 1860-0 is 0° 29™ 30*. 
26, 66° 47’ 77-9. ] | 
1875, Oct. 9. Close D. neb., seen v F. Moon setting. *7-8 m. in Pos. 63°:7 (3). 
Dist. 2387-0 (2). (VII. obs.) 
III. 870 | 1874, Nov. 7. pB,S. *9m. (Schjellerup 213), yellowish, in Pos. 305°-0 (4): 
Dist. 228/-4 (5), or 12°47 p., 131-0 n. The place of the neb. for 1860-0 
is accordingly 0 31™ 1* 56, 88° 2’ 34’”-0. 
1876, Oct. 22. *9.10 m. in Pos. 306°:0 (2). Dist. 220-0 (2), or 11° 83 p. 
WYO im. (IE @os,) 
35 1848, Mar. 28. Resolved by a power of 800, although the night was rather | 
—II. 707 hazy. | 
1849, Sept. Think it r., and that it has the appearance h. 2120 would present 
if removed to a great distance. It is L and rather F. 
1851, Oct. 25. Strongly suspect neb. extends to 6’ all round centre, which is r. 
| S. *nf centre. Dark band cutting off part of neb. np the centre? 
1852, Sept. 16. pL, R, gb M, *in M.; * 1’ nf, diameter about 2/ or 3/. 
| 1855, Oct. 7. WL. irreg. R. b. M. r. 3 st. in it thus—[see Pl. I], and many 
| others, round skirts of neb. [Could this be 72%] 
1866, Sept. 14. ¢ F, L, b M, clouds passing. (VI. obs.) 
* [Mean of the two nights 16°°8, 2593 or 5°44 f, 248-2 n. ‘The * is B. W. 0%, 727, whence the place of 79 for 1860-0. 
Qh 28™ 42°19, 66° 48’ 567-5. J 
