Observations of Nebula and Clusters of Stars. «Si 
G. C. | h. & H. | — 
701 from 700 Pos. 1°-0 (4), Dist. 98''5 (4) [in perfect accordance with 
d’ Arrest. | 
702 — 701 13:0 361-9 
703 — 702 1-0 (2), 358 (2) or O°4 f, 358"n. 
[N P D of 703 in G. C. is 3' too small, R A 2° too large.] (XIV. obs.) 
704 299— | 1854, Dec. 16. vF,c E, upsf, lbMN. 
TIT. 445 | 1861, Nov.6. Evnpsf, vg, sbM ; I suspected a darkness round the Nucl. (III. 
obs.) 
708 |TIT.959 | | 1877, Jan. 13. 708 is v F, vS, 709 is some minutes f, and B, pL, E114”, g, 
709 I. 60 } sbMLN. Both seen to great disadvantage owing to the low altitude. (1. 
obs.) 
710 1873, Oct 11. pB, cS, R, smbM to a vF Nucl. *9m. in Pos. 33-1 (2), 
Dist. 216-6 (2) [or 9*-2 f, 181'°5 n, Auwers has 7*+ f, 2'+ n]. There are 
2 st 12 m. nearer. 
1877, Dec. 1. Looks like a Cl., very badly seen. (II. obs.) 
711 1873, Nov. 16. cF,S8,R, gbM, 2 st 12 m.p on parallel, the nearer in Pos. 
287°-3, Dist. 60'-0. Many small stars in field. (1 obs.) 
717 301 1854, Noy. 24. Scattered Cl., L and § stars. (I. obs.) 
720 | VIII. 84] 1875, Oct. 9. Only 7 or 8 st. 9.10 mag. forming the letter 8. (1. obs.) 
726 9548— | 1866, Nov. 13. ¢B,p L, bM, either double or with a * very closely p (observations 
Il. 290 interrupted by the superb display of shooting stars). 
727 302— | 1850, Oct. 11. Suspected r by both observers. 
TIT. 446 | 1861, Nov.6. Epf,bM. 
1861, Dec. 27. a and fare B,S,gbM, dandevF, yisv F and 
perhaps a F* [A comparison with h’s and @’Arrest’s descrip- 
tion shows, that B=:727, a—Nova d’Arrest =5314, 6 and « 
Nove ?] 
1861, Dec. 28. F, pL, vg bM. 7 
1877, Nov. 6. pF,S, R, ££, 5314 (nova d’A) is a little brighter } h | 
and E nearly pf, Pos. 324°-1, Dist. 410’. Looked for other neb. sp 727 and | 
p 5314, found only v F st, Iam sure there are no nove here. (VI. obs.) 
738 303—= | 1854, Oct. 26. vF,pL, R. 
II. 288 | 1857, Dec. 7. F, L, mottled. 
1861, Nov. 6. R,bM. 
1861, Dec. 28. pB, * close tonedge. (V. obs.) 
T4A7 | 2567— ] 
IT. 593 (| 1866, Nov. 8. Neither of them v B, clouds interrupted the observation. 
752 ae || 1866, Dec. 12. p one B, pS, fone v B, p L,bM. (II. obs.) 
© J 
753 | 304— | 1855, Jan. 17. Double net ., both v 8, b M k het 
IIT. 263% , Jan. 17. ouble neb., n and s, both v8, b M. Cannot make out whether 
there is a connexion between them. (I. obs.) 
754 | R. nova j 
756 305— )| 1848, Dec. 19. 3neb. nearly inalinennp. Middle one the brightest, 2 others F. 
IIT. 569 From 1st to 2nd about 10’, from 2nd to 3rd about 6’. 
758 306— || 1850, Oct. 7. First appears divided and p part has a minute * or stellar point in 
IT. 455 it. 2nd about 11’ off is brightest of the 3 and:b M, 3rd about 7' from 2nd is 
760 307= equable in light and I suspect a 4th F one perhaps 20! off. [The estimated 
IT. 456 distances in these two observations as well as in the following one from 1851 
763 | R. nova } disagree in a very strange mamner with the real distances, at least as far as 
regards that between 305 and 306. According to H and @A Aa=2" 11°, A 
TED) ==)", 
1850, Dec. 8. Istisv Fand hasaS * np; 2nd has, I suspect, a F Nucl., itis b M 
and the brightest of the 3, nofa*. About 16' f the 3rdis a F Nova[=7 63}. 
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