distances and positions of 380 double and triple stars, &c. 151 
No. CXXIII. R. A. n b 17'; Dec!. 82° a'N. 
(201 Bode Camelopardali) ; Struve 386; 
Double ; 8th and 10th magnitudes. 
Position. 
90—47.15 
46.15 
46.50 
! 
H 
Mean rr — 46.47 
April 11, 1823. 
Five -feet Equatorial. 
np 
Position == 43 0 1 3' np 
Distance = 21 ".876. 
Distance. 
Parts. 
75- H 
65. 0} H 
Mean — 70. o 
7 j — 0.73 
69.27 
According to M. Struve, who has determined the place of 
this star in 1814 in his second Catalogue, the difference of 
declination between the two stars is equal to that of their 
right ascensions ; the magnitudes agree with ours (8 and 10), 
and the small star precedes. He makes the difference of 
R. A. by a mean of two observrtions on the wires of a transit, 
6 s . 6 of time, whence he concludes the difference of declina- 
tion i3".7, and the distance i9 r/ .4. Thus we have, according 
to these data. 
Position 45 0 np or sp, “ utra polo vicinior non notatum.” 
Distance i9"-4 vide Dorpat Obs. Catalogus I. No. 92. 
No. CXXIV. R. A. n h i8 m ; Decl. 4 0 o' N. 
83 Leonis ; Struve 387 ; IV. 
! 3 ; 
Position. 
March 14, 1821. 
Distance 
o 1 
61.48 ) 
Parts. 
s f 
95. 8' 
61.21 v H 
9 6 - 5 
61. 1 1 j 
99- 3 : 
6 °-35 ) 
96. 1 | 
60. 0 v s 
61.50) 
Position = 61° 7' sf 
Distance = 29 ,, .£42. 
96. 0 
96. 5 J 
- 61. 7 
Mean 1=96.70 
Z — — 3.16 
93-54 
