Observations of Nebule and Clusters of Stars. 
G. C. | h, & H. —— 
| 
1850, Mar, 3. B, pS, * nf which perhaps is what caused h’s clubbed appearance 
11944). 
ee Jan. he r by both observers, s * near the middle and another nf ; 
lenticular. 
1851, Mar. 20. *n of middle, m E, knot in p end. 
1858, Mar. 8. Of unequal brightness throughout its length, p part is F but 
contains a B patch with a * in it ; the f part’ is comparatively much brighter 
and is mottled. 
1861, Mar. 29. Seems r in centre and to have dark spaces ; extremities v F. 
1867, April 2. B spots np and sf, the latter much the fainter, possibly a *; neb. 
is curved (2), the bend pointing to a * in Pos. 40° (2) which is not involved. 
Perhaps * near Nucl., neb. not by any means vm KE. [? 1944 taken for 1931. ] 
(XIII. obs.) 
1933 640 )| 1854, Mar. 1. One pB, 6'f and a little n are two others v F, about 3' apart pf; 
1935 641 | several others round about. 
1936 | Ree ( 1878, April 1. 1933 and 1935 seen for a few minutes [after 1931], the f one is 
IOS ff ||} J smaller and in a rectangular A of 3 st. (II. obs.) ; 
5507 one 1854, Mar. 21. 4neb. Two p andf, about 4’ apart; the 3rd is n about 3! 
1940 | R. nova forming the vertex of an obtuse A, the 4th is about 4’ further n and lenticular. 
1942 646— | 1932—h 642 was never seen by d’Arrest, and is = h 646 with an error of 
TOG, Bil 4 1™ in R A; the two first nebule mentioned above are 5507=d’ Arrest nova 
1945 | 648= | and 1940. The latter was not noticed by d’A.]| (1. obs.) 
IW. 52 ; 
1941 644 1851, Feb. 26. p onee F. 
1943 647 § | 1857, Mar. 21. Seen for a moment through clouds. (II. obs.) 
1944 645 = 1863, Feb. 11. * nf does not seem inv., two st near the middle 
I, 15) seen by glimpses. 
1863, Mar. 18. * a just on edge of neb., branch sf very doubtful, 
as also the dark streak p. One * in centre certain, 2 or 3 others 
strongly suspected. 
1863, Mar. 20. I strongly susp. the branch in f end comes round past 
Nucl., streak p not seen. About 3" p and 10'sis another neb. 
c E pf, bM, central * and * in pend. [=h 639; the above 3 
obs. of h 645 are recorded as. being of 639, but the neb. 3™ p 
shows the mistake. | 
1874, Mar. 18. Nucleus, stellar, mottled. * 14m to * 10m Pos. 144°-2. Dist. 
61"-5. Neb. to * 8m Pos. 282°-0. Dist. 756"-4 [or 59°68 p, 156"-5 n, *= 
B. W. 9°, 874 and the place of the neb. for 1860 is 9* 42" 40°-7, 55° 47’ 30"-5. | 
Nova p F, pS, R, gbM, 2vSstnr, * 15m Pos. 48°°6, Dist. 43-9. Nova 
in Pos. 137°-2. Dist. 164°-8 from * 8m [or 9° -04 f, 120"-8n, place of 5505 
for 1860: 9° 41™ 50°1, 55° 46’ 54'-8}. 
1876, Mar. 22. Seen for a short time between clouds in very bad sky. An e F, 
vS object in Pos. 138°-4+. Dist. 174+ [or 8°2 + f, 130" + s] from * 8m 
p 1944, but I was not quite sure it was a neb. 
1877, Mar. 17. * 14m to *11m Pos. 147°4. Dist. 63:6. The * 14m. is near 
the nff end of the neb., which is of unequal brightness, reminding me of M. 1, 
mottled. Novasf the * 8m seen, v F, stellar. (VI. obs.) 
1949 649= |1871, May 21. Very like Neb. in Andromeda. (3 ft.) 
M. 81 | 1874, Feb. 21. eB, vsvmbMN, extends about 8’ from Nucl. to the n, and does 
not extend beyond the 2 first stars, if so far ; E in the fainter part np sf. 
Pos. Dist. 
*10m 152-°Q 144-4 
*10m 166°8 202°3 
*12m 67:6 114:3 
*14-5m 256°9 38-4 
*13m 65:8 110°3 (IIT. obs.) 
Ne EE 
