[x. 8. 11 
Bemerkungen. 
Positionsw. 
Refraction 
Bilder. 
Refraction. 
Distanz. 
0.2418. (4263; B=7.7; 0=72) . 
a = 5h41"9 8-—.--20?49' 
75799 
75.56 
75.29 
75.42 
75.565 
45.42 
A+B u. €. , 
2 
+ 07084 |1619 8 | + 0.2 |2—3 
+ 0.040 1160 59 | — 0.3 |3 Eilige Beobachtung. 
4-0.033 ۱160 54 |+ 0.2138 Merz'sches Mikrometer. 
—+0.032 1161 8 |+-0512—3 
+ 0.035 |161 2.2 + 0.2 
c .910. (7.8 u. 8.0) 
a= 54875 8 = -+ 9ه‎ 
هو‎ 0.017 [130 30 | -+ 0.61 3—4 
+ 0.015 1130 21 | 1.2 |45 
| 45.430| + 0.016 |0 25.5| = 0.9 | | 
45.44 
Temp. 
— 1:6 
— 0.6 
— 2.0 
— 3.9 
— 0.2 
— 0.1 
Vergr. 
1 
1 
1 
III 
| 
7. RENZ, BEOBACHT. VON 51 DOPPELSTERNEN MIT GROSSER DISTANZ 
Sternzeit, 
5hg4m 
3 48 
& l 
6 50 
6 31 
8 37 
Epoche. 
1890.1 
1890.1 
1890.1 
1890.1 
1890.1 
1890.2 
1890.2 
1890.2 | a 
0.2.545.— 0.213. = S Aurigae. (4— 30: B—7.5; C—110; D= 9.5) 
a= 55272 8 — + 2 
zw 
45.96 | 4-0.013/293 19 |+0.213 
46.25 | + 0.014 292 46 ۱+09 Sans دع‎ 
45.67 | + 0.013292 47 |-- 0.2 2— 
46.34 | 4-0.013|292 39 اوه با‎ 4 id Sis 
: Fadenbeleuchtung. ۴6 
46.21 | 0.014 |292 33 |+0.1|4 الو ری میا‎ 
16.086! + 0.018 |292 488-02 | | 
Au. D. 
127,81 | + 0.045 |349 46 |+ 0.6|3 Merz’sches ی ی‎ 
1 R ew. 
127.52 |+ 0.045 |349 47 |+ 0613 e 2 
127.21 | +0.041 |349 20 |+02|4 
127.11 | + 0.051 |349 31 | + 1,0134 
127.59 | + 0.041 1349 44 | ۱9 
mm 
127.403 + 0.045 1349 87.1 + 0.5 
P 
— 0.1 
+ 7.7 
— 9.6 
— 0.1 
— 3.9 
— 2.0 
— 0.1 
— 0.1 
— 8.8 
+ 0.8 
9 10 
11 6 
7 43 
7 41 
9 58 
1890.2 
1890.8 
1891.1 
1891.1 
1891.1 
1890.8 
1890.1 
1890.7 
Mélanges mathém. et astron. T. VII, p. 208. 
