NEBST EINER UNTERSUCHUNG ÜBER SYSTEMATISCHE FEHLER. 451 
Bemerkungen. 
Refraction 
Positionsw. 
Refraction 
Vergr 
Temp. 
Distanz 
Bilder. 
0.5. 141. (4 =6.8; B —85; C—98; D = 10.2) 
a =6 "268 8 = + 0 
At B, 
IH|— 2701 497836 | 4- 07016! 73946 |— 011 2-81 Merz’sches Mikrometer. 
IT| — 2.8| 42.61 | + 0.018| 73 81 | +0۱4 
I| — 0.6| 42.48 | + 0.017 | 73 58 0.0/8 
III! — 9.6| 42.35 | + 0.013۱ 74 8 0.0| 4—8 
42.450|-4- 0.016 | 73 50.8 0 
Au. C+ D. 
2 
II|— 2.01 45.51 |+0.0141117 6 [--0.1|2—8| Merz’sches Mikrometer. 
III| — 2.3| 45.97 | + 0.014 117 1 |+ 0.۵ | وس‎ 
II|— 0.5| 45.80 |+ 0.014 1117 8 |-- 0.1/8 
M| — 9:6| 45.71 |2- 0.018 1117 10 |--0.1| 8—4 
45.748 + 0.014 1117 6.2) +- 0.1 
(xxx1v)] 
Sternzeit. 
Epoche. 
- 
c. 233. (7.5 u. 7.8) 
a = 6277۸ 8 — + 77 
—0.2|4 
IL] — 0.21 58.51 | + 0.019 ۱949 13 
IIl! — 0.4| 53.46 | + 0.028 248 25 | — 0.1|4 
| | | 58.485 + 0.024 m 19.0 — 0.2 | | 
c. 944 — 56 Aurigae. (5.3 u 9.0.) 
a = 08888 . à = تھ‎ 17 
III — 0.71 45.84 |+ 0.018] 22 18 |+0.7]3 
IIl — 5.41 45.91 |+0.017| 22 26 9ه‎ 
| | | 45.875) + 0.018 | 22 22.0] + 0.7 | | 
B. A.C. 2751. (4=6.5; B—92; 0-7 D=8.8) 
a = 80778 ê= + 59037 
Au D. 
II | + 7.5| 95.27 |+0.052| 8 84 [12/2 
T !+10.3| 95.11 |+ 0.052| 8 88 |-- 1,2 | 2—4| Bilder sehr unruhig. 
| | | 95-190] 0.052 | 8 36.0| +12] | 
1890.1 | 9^88» 
1890.2 |10 14 
1890.2 | 9 58 
1891.1| 7 57 
1890.4 
1890.1 | 9 55 
1890.2 |10 27 
1890.2 | 9 47 
1891.1| 7 49 
1890.4 
1890.2 | 7 26 
1890.2 | 9 28 
1890.2 | 
1890.2 |10 16 
1891.2 |10 0 
1890.7 | 
18904 |15 27 
1890.4 |15 29 
1890.4 
Mélanges mathém. et astron, T. VII, p. 209. 
