Is, s. 1 
Bemerkungen. 
Merz'sches Mikrometer. 
iter schwer 
ten. 
Ungewóhnlich schlechte . 
Bilder. : 
Fadenbeleuchtung. 
F. RENZ, BEOBACHT. VON 51 DOPPELSTERNEN MIT GROSSER DISTANZ 
Dunst. Begle 
h 
zu beobac 
| 
| 
c.918— .23 Herculis. (6.0 u. 
Refraction. 
Distanz. 
a-—16^18"7 ò= + 32036’ 
+ 07015 
+ 0.012 
+ 0.021 
+ 0.016 
c.5929. (7.2 u. 8.5) 
ي‎ = 16*26 "2. 8$ — + 8?32' 
| 58.400] -+ 0.034 | 71 27.0| — 0.4 | 
+ 0.030 
-i- 0.038 
e.527. (7.2 u. 88) 
a—16^38"9 8 = +4 6049 
2 5 T 
-tjs 
Ce e |a 
8.5) 
17°59’ | 4- 0/4 | 8—4 
18 50 4 
18 37 |+10|4 
18 28.7| ېه‎ 0.4 
71 97. [— 04134 
71 27 |—04|4 
292 0 ۱+ 09۱-4 
299 7 |+192|3-4 
| 
| 53.085| -i- 0.015 |292 al +10 | 
=+ 0.015 
+ 0.015 
34744 
34.35 
34.44 
34.410 
58.41 
58.39 
53.00 
53.07 
0.2.8911. (A = 7.9: B —11.8; 0 = 8.0) 
3—4 
a = 16^49"7 3 — + 57 
A u. C. 
+ 0.8 
+ 0.8 
+ 0.3 
+ 0.3 
318 
318 
318 
318 1.7 
+ 0.032 
+ 0.032 
—+ 0.032 
+ 0.032 
114.38 
115.09 
115.08 
114.850 
0.998.— 60 Herculis. (5.0 u. 11.0) 
E 17*079 58 SE 19054" 
+ 1.1 
+ 1.1 
+ 0.2 
+ 0.8 
310 6 
910 0 
310 24 
310 10.0 
=+ 0.018 
+ 0.018 
-i- 0.021 
+ 0.019 
53.71 
53.61 
53.71 
53.677 
Temp. 
به 
8.7 + 
10.0-- 
+-10.7 
1 
—+10.7 
+-10.1 
— 4,5 
III | 2-10. 
= 
Vergr. 
IV 
IV 
III 
11 
11 
|| 
III 
II 
II 
III 
IH 
11 
Sternzeit. 
19% 5m 
15 54 
20 34 
18 33 
19 15 
18 42 
19 30 
21 2 
20 41 
21 1 
Epoche. 
1889.6 
1890.5 
1890.6 
1890.2 
19 28 
19 40 
14 37 
1890.7 
1890.7 
1890.7 | 
1890.7 
1890.7 
1890.7 
1889.9 
1890.7 
1890.8 
1890.5 
1890.7 
1890.7 
1891.2 
1890.9 
Mélanges mathém. et astron. T. VII, p. 214. 
