132 
1 
n 
Grösse 
9 
6.77 
8 
6.56 
2 
6.46 
1 
6.27 
8 
7.86 
8 
6.86 
1 
7-79 
5 
6.43 
9 
6-57 
0 
7.28 
4 
7-52 
8 
7-36 
523 
7 
6.25 
3 
7-15 
6 
7.48 
6 
7.18 
4 
7.66 
0 
6.62 
5 
6.07 
7 
8.09 
5 
7.67 
5 
7.67 
.1 
6-93 
0 
7-3 2 
556 
1 
6.80 
*5 
7.04 
3 
6.56 
56 
7-05 
h 
5.88 
7.10 
Zone o° bis -}- 20° Declination. 133 
B.D. 
Sternzeit 
I 
II 
III 
!V 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
00 
0 1 
0 
0 
i 2 9™ 
1 7°4 
i6?4 
1784 
i6?4 
16890 
4i?5 
8.9269 
8.9540 
2 80 
i 32 
20.4 
21.5 
25-3 
22.4 
22.40 
51-4 
9.1620 
9.2148 
0.0936 
— 0.23 
6.46 
1 108 
i 34 
13.0 
12.6 
13.0 
11*7 
12.58 
5 1 -9 
8.6761 
8.7306 
0.3906 
+ 0.98 
7.67 
2 84 
i 35 
14.1 
12.5 
14-3 
13-5 
13.60 
51.6 
8.7427 
8.7962 
0.3250 
+ 0.81 
7-50 
8 94 
1 37 
20.6 
18.4 
24.2 
21.4 
21.15 
45-5 
9.1146 
9.1504 
0.0292 
— 0.07 
6.62 
3 93 
i 39 
ii.8 
11.8 
12.3 
12.6 
12.12 
50.6 
8.6443 
8.6944 
0.4268 
+ 1.07 
7-76 
5 104 
i 41 
25-7 
22.6 
27.6 
27.4 
25.82 
47.8 
9.2780 
9.3198 
0.1986 
— 0.50 
6.19 
9 47 
1 43 
26.3 
24.9 
28.5 
24.0 
25.92 
45-9 
9.2812 
9.3180 
10 168 
1 45 
15.0 
15*1 
18.5 
16.5 
16.28 
41.9 
8.8954 
8.9233 
Mittel aus den Vergleiclisternbeobaehtungen: 9.1116; 9.13x5; 9.1206. 
Zur Reduction benutzt: 9.1212. 
Zone 19 
1886 October 2g. 
Beobachter: Kcmpf. Photometer: D. Vergleichsterne: Nr. 44 
und Nr. 46. Luft: 1 
—2. 
io°4Ó04 
B 
0 
”04 
CM 
tn 
O • 
00 
2885 
3°?4 
27-5 
28872 
4286 
9-3635 
9.3928 
9 5111 
22 13 
23.8 
19*5 
26.6 
21.3 
22.80 
42.9 
9.1766 
9.2065 
5 4821 
22 17 
15.0 
14.0 
15.8 
12.6 
14-35 
47.8 
8.7884 
8.8302 
0.4207 
+ 1.05 
7-59 
5 4826 
22 19 
13-9 
13-5 
17-3 
14.0 
14.68 
48.1 
8.8076 
8.8502 
0.4007 
-f-1.00 
7-54 
4 4706 
22 21 
20.5 
22.3 
24.0 
21.6 
22.10 
49-3 
9.1509 
9.1970 
0.0539 
+ 0.13 
6.67 
5 4830 
22 24 
26.4 
21.4 
28.6 
23-3 
24.92 
47-5 
9-2493 
9.2902 
0.0393 
— 0.10 
6.44 
5 4834 
22 26 
35-3 
36.6 
40.4 
34-6 
36.72 
48.4 
9-5533 
9.5968 
0.3459 
— 0.86 
5.68 
8 4714 
22 28 
19.2 
17.6 
19.4 
16.0 
18.05 
45-i 
8.9823 
9.01 71 
0.2338 
+ 0.58 
7.12 
10 4604 
22 30 
23-5 
25-3 
26.3 
24.8 
24.98 
43-4 
9.2512 
9.2822 
9 5111 
22 32 
19.1 
19.0 
22.5 
20.6 
20.30 
42.5 
9.0805 
9.1096 
3 4599 
22 35 
21.5 
19.6 
22.6 
20.0 
20.92 
50.6 
9* 1 °5 5 
9-I556 
0.0953 
+ 0.24 
6.78 
4 4722 
22 37 
1 7 • 5 
16.9 
17.7 
16.0 
17.02 
49.6 
8.9329 
8.9799 
0.2710 
+ 0.68 
7.22 
4 4726 
22 39 
14.0 
14.9 
17.0 
15-4 
15-32 
49.8 
8.8439 
8.8915 
0.3594 
+ 0.90 
7-44 
6 4889 
22 40 
22.1 
20.6 
24-5 
23.6 
22.70 
47.1 
9-I730 
9.2129 
0.0380 
-b 0.09 
6.63 
7 4745 
22 43 
19.1 
18.6 
19.7 
16.7 
18.52 
46.7 
9.0039 
9.0427 
0.2082 
4-0.52 
7.06 
9 49*3 
22 45 
13.8 
12.6 
14.0 
11-7 
13.02 
44.2 
8.7055 
8-7383 
0.5126 
+ 1.28 
7.82 
10 4604 
22 48 
23.6 
26.3 
28.4 
26.1 
26.10 
44-4" 
9.2868 
9.3200 
9 5111 
22 50 
22.5 
22.5 
23.6 
21.3 
22.48 
42-5 
9.1650 
9.1941 
Mittel aus den Vergleiclisternbeobaehtungen: 9.2997; 9.1959; 9.2570. 
Zur Reduction benutzt: 9.2509. 
Zone 20 
1886 October 2g 
Beobachter: Miiller. Photometer: D. 
Vergleichsterne : Nr. 44 und Nr. 46. 
Luft: 1- 
-2. 
io°4Ó04 
22 h 58 m 
23 ?2 
21?7 
2480 
21?7 
22865 
45°i 
9.1712 
9.2060 
9 5111 
23 O 
2O.4 
16.6 
19.4 
17.7 
18.52 
42.6 
9-0039 
9.0332 
6 4919 
23 2 
23.2 
20.6 
24.1 
21.5 
22.35 
48-5 
9.1602 
9.2039 
0.0608 
—0.15 
6-39 
i 4560 
23 4 
13-3 
ii-9 
H-7 
13.8 
13.42 
52-9 
8-7313 
8.7895 
0-3536 
+ 0.88 
7.42 
3 4640 
23 6 
13-7 
12.6 
15.6 
14.0 
13.98 
5 1 - 1 
8.7662 
8.8179 
O.3252 
+ 0.81 
7-35 
9 4939 
23 8 
12.6 
12.0 
14.2 
13.0 
12.95 
45-2 
8.7009 
8.7360 
O.4071 
+ 1.02 
7-56 
AQioi 
23 10 
13.6 
10.7 
12.4 
11.6 
12.08 
49-7 
8.6415 
8.6888 
0-4543 
+ 1.14 
7.68 
1 J A 
23 12 
10.4 
11 *3 
11.4 
10.5 
IO.90 
49.8 
8-5534 
8.6010 
0.5421 
+ 1-36 
7.90 
10 4604 
23 14 
22.2 
24-3 
26.7 
23-5 
24.18 
46.4 
9.2247 
9.2627 
9 5111 
23 16 
19-3 
18.3 
20.4 
18.2 
19.05 
43-o 
9.0275 
9.0576 
3 4644 
23 18 
16.4 
14-5 
16.4 
14.7 
15-50 
52.2 
8.8538 
8.9094 
0.2337 
+ 0.58 
7.12 
9 4948 
23 21 
16.6 
17.2 
19-3 
18.1 
1 7.80 
45-9 
8.9706 
9.0074 
0.1357 
+ 0.34 
6.88 
6 4940 
23 23 
23-5 
25-5 
27.0 
23-5 
24.88 
49.6 
9.2480 
9.2950 
0.1519 
— 0.38 
6.16 
4 479 1 
23 25 
13-4 
11*7 
14.4 
13.6 
13.28 
50.8 
8.7223 
8-7731 
0.3700 
+ 0.92 
7.46 
9 4975 
23 27 
16.4 
15-2 
17.6 
16.8 
16.50 
46.3 
8.9067 
8.9445 
0.1986 
+ 0.50 
7.04 
5 4947 
23 29 
10.7 
10.6 
13.2 
10.6 
11.28 
50.4 
8.5828 
8.6323 
0.5108 
+ 1.28 
7.82 
10 4604 
23 31 
22.9 
234 
24.2 
20.6 
22.78 
48.0 
9-1759 
9.2182 
9 5111 
23 33 
18.O 
18.6 
22.5 
19.1 
19-55 
43-6 
9.0492 
9.0806 
Mittel aus den Vergleiclisternbeobaehtungen: 9.x 196; 9.1602; 9.1494. 
Zur Reduction benutzt: 9.1431 
*) 5 0 4910 dupl. Zuerst die südlichere Componente gemessen. Beobachtungen 
etwas schwierig. 
* 
Pubi, des Astrophys. Obs. zu Potsdam. Bd. IX. 
17