of new Nebula and Clujters of Stars • 
249 
V. 
1786 j 
Stars. 
j] 
vr. s. 
29 
2 
61 Urfae 
f 
45 38 
3 ° 
18 
4 2 1 c Orioni 
45 J 
P 
0 0 
3 1 
3 1 
44(0 
P 
0 0 
3 2 
33 
Feb. X 
28 (.) 
P 
f 
17 26 
X 26 
34 
— 
46(5) Orionis 
P 
0 0 
35 
„ 
36 w — 
f 
3 39 
• 
5 & 
P 
2 l6 
3 6 
* 
Oft. 17 
35 (*) Alidro 
P 
9 8 
37 
24 
57 Cygni 
£ 
5 3 
38 
Dee. 20 
19 ( 0 ) Orion 
t 
f 
11 9 
11 35 
39 
21 
x 1 (0) Crater 
P 
8 15 
1 
1 
* 
jD.M.f 
1 
Oh 
Defcription. 
take up lefs than -§ degree, but 
X fuppofe it to be much more 
extenfive. 
f 
0 40 
I 
eF. vL. vlbM. r. io' 1 . 8 or 9' b. 
n 
0 0 
2 
The ill and 2d c Orionis, and the 
ftars about them, are involved in 
eF. unequally B. m. nebulofity. 
n 
0 0 
2 
t Orionis with its neighbouring ft. 
are involved in eF. m. nebulofity 
to a great extent. 
f 
3 4 
2 
cB. vL. m. diffufed and vanifhing, 
near and ff. Bft. 
f 
0 7 
I 
Diffufed eF. m. nebulofity. The 
means of verifying this pheno- 
menon are difficult. 
n 
0 0 
I 
I am pretty certain s Orionis is 
involved in unequally diffufed m. 
nebulofity. 
f 
0 40 
4 
Diffufed m. nebulofity, extending 
n 
0 28 
5 
over no lefs than 10 degrees of 
PD. and many degrees of RA. 
It is of very different brightnefs, 
and in general extremely F. and 
difficult to be perpeived. Moft 
’ probably the nebulofities of the 
28th, 30, 31, 33, 34, and 38th 
of this clafs are connected toge- 
ther, and form an immenfe ftra- 
tum of far diftant ftars, to which 
muft alfo belong the nebula in 
Orion. 
f 
0 20 
2 
vF vL. E. nearly mer. or a little 
from np ff. about 20' 1. 
f 
I I 
1 
vL. diffufed nebulofity. bM. 7 or 
8' 1. 6'b. and lofing itfelf vg. 
and imperceptibly. 
n 
f 
x 19 
O 52 
1 
Strongly fufpedted nebulofity of v. 
great extent. Not lefs than 2°i i x 
of PD. and 26" of RA. in time. 
f 
1" 
O X7 
2 
vF. mE. nearly par. or about 1O 0 
fp nf. vgbM, 8' 1. 3' b, 
_ 
40 
