521 
of goo new Nebulce, and Clusters of Stars. 
IV. 
1790, 
Stars. 
M. S. 
D. M. 
66 
Mar. 18 
17 Ursas - 
P 
1 6 29 
1 
3 6 
67 
— — 
66 Ursge 
P 
0 39 
n 
1 55 
68 
*9 
45 Lyncis - 
P 
4 15 
n 
1 44 
69 
Nov. 30 
f 26 Auriga 
| or 31 Hevelii 
p 
s 
88 24 
24 59 
/ 
/ 
0 11' 
1 2 6 J 
c 
o~ 
Description. 
1 
1 
1 
around. A power of 300 
shewed the same, but gave 
a little more extent to the 
nebulosity. The 23d Mon- 
cerotis was quite free from 
nebulosity. 
A small star with a^B. fan- 
shaped nebula. The star 
is on the p side of the di- 
verging chevelure, and 
seems to be connected 
with it. 
pB. ph. R. The greatest 
part of it equally B, then 
fading away p suddenly ; 
between 2 and 3' diam. 
vB. S. exactly R. BNM.and 
z;F. chev. vg. joining to 
the N. In a lower situa- 
tion the chev. might not 
be visible, and this neb. 
would then appear like an 
ill defined planetary one. 
A most singular phenome- 
non; A ft 8m. with a faint 
luminous atmosphere of a 
circular form, about 3' in 
diam. The star is perfect- 
ly in the centre, and the 
atmosphere is so diluted, 
faint, and equal through- 
out, that there can be no 
surmise of its consisting of 
stars, nor can there be a 
doubt of the evident con- 
nection between the at- 
mosphere and the star. 
*■ 
