G. C. | h. & H. | 
1680 IIT. 235 
1684 518— 
I. 204 
1686 519 
1688 521= 
IIT. 49 
1689 b= 
IDL, HBP 
1691 520— 
I. 288 
1697 3139 
1698 524 
1699 
1704. 526— 
IL. 80 
1705 |R. nova. 
Observations of Nebule and Clusters of Stars. 69 
1852, Mar. 9. B part a little n of middle; p this and a little s I suspect a 
darkish space. 
1856, Jan. 11. 
1860, Dec. 19. 
Perhaps 1 E sp nf. 
FB, pL, vgbM toa F * or Nucl. (X XVI. obs.) 
1867, Jan. 28. Not found. [Not observed by d’Arrest]. (Once looked for). 
1849, Mar. 22. 
1850, Mar. 12. 
1852, Jan. 27. 
seen. 
1856, Jan. 29. I see no appendage; m E npsf, v B centre. 
1863, Feb. 20. A F twist starting from sf end and turning p & np suspected 
several times. (XIII. obs.) 
1851, Jan. 24. 4st in scarcely perceptible neb. 
1856, Jan. 30. 4st in v F nebulosity. 
1877, Mar. 7. Neby very distinct, though v F. 
Lbreawaxalh f the 4st, involving some v F ai just n of the third B *. 
1857, Feb. 23. E upsf. malo, I think a is a VF ray though likely F 
to be taken at first:for a * 
1866, Dec. 29. cB, p8, VE “145° +, bM. 
Points to a * sf; vdull Nucl., suspect F neby in all directions. 
Has Nucl. ; F appendage sp, parallel to neb. ? ? 
Lenticular ray npsf, gmbM,vF. No appendage whatever 
3-st.7 or 8 m. s. 
I strongly suspect an eF 
(VII. obs.) 
v F,.irr R, stellar point or v F Nucl. in centre. 
F, p L, bM, light not equable. B*n, 2v Fst p. (III. obs.) 
(3 ft. telescope). v B, I think in the 6 ft. it would be r? 
(3 ft.) p B, Enpsf, vgbM. (II. obs.) 
(II. obs.) 
1852, Mar. 9. 
smaller p it. 
1855, Feb. 17. 
1858, Feb. 16. 
1861, Feb. 10. 
1862, March 21. 
Almost planetary, * in nedge, second * ‘iniuch 
1878, Jan. 28. Doubtful whether found, many Sst; definition very bad. 
(I. obs.) 
1867, Jan. 2. About 20 stars. (1. obs.) 
1873, Dec. 26. 
2! nf. 
1876, Feb. 21. 
1848, Dec. 19. 
cE, pS, 1E pf; was thought to have an e F companion about 
e F; I think it is only a 
Close D neb, S * p. 
1852, Jan. 17. S*p, neby of h 526 involves a companion neb. 
1855, Feb. 9. Very close, almost touching; h 526 is [ 
mbM, h 527 is smaller & lbM [the latter is not h 527, 
but the close comp". to h 526, viz. 1705]. 
1860, March 24. p B Nucl, companion v F, sometimes I 
thought them connected by v F neby. 
1866, March 7. Certainly double p & f with S * (mebu- 
lous ?) p; h526 is R, vs vmbM, comp". F, 8, R, bM. 
1866, Dec. 29. h. 526 to neb. f. Pos. 97°-8 (2), another 
p. Pos. 295°:3 (2) [the latter seen in 1848, 1852, 1855, 1873 & 1876 as a F *]. 
“NO tm, se mi, (ALL, Os) 
1873, Dec. 26. * 14 m invf Pos. 98°:8 Dist. 32"-1 [= 1705.] 
* 15 m inv p 294-0 31-4 
* 14m 123°8 704 
*13m 31:3 99-0 
1876, Feb. 21. Seen tolerably well for a minute or two, the sky then became 
extremely misty, p B, p L, irr, 2 st 15:16 m. inv. f & npp. 
Pos. Dist. 
*14m 32°°1 (2) 100"°6 (2) 
* 14:15 m 121-7 (i+. (eX. obs:) 
