302 
Müller und Kempf, Photometrische Durchmusterung 
302 
B.D. 
Sternzeit 
I 
II 
t—1 
1—1 
HH 
IV 
J 
z 
log sin 2 / 
corrig. 
für Ext. 
Difl. 
in log. 
Diff. in 
Grössen 
Grösse 
9°2239 
7 h 37 m 
2 I?8 
1985 
2 I ?4 
1984 
20852 
5081 
9.0895 
9.1380 
o 2313 
7 42 
19.2 
17.9 
I9.O 
18.1 
18.55 
52.7 
9-0053 
9.0628 
0.1330 
4 - 0.33 
7.28 
0 2335 
7 44 
21.6 
18.0 
2 1.4 
19-5 
20.12 
52.5 
9-0731 
9.1298 
0.0660 
4 - 0.17 
7.12 
1 2142 
7 46 
19-5 
17-5 
I9.I 
18.6 
18.68 
52.2 
9.0111 
9.0667 
0.1291 
4- 0.32 
7.27 
2 2039 
7 48 
24.6 
22.5 
22.9 
22.4 
23.10 
51.0 
9- 18 7 3 
9.2387 
0.0429 
— 0.11 
6.84 
3 2014 
7 50 
29.8 
25.0 
27.O 
25.2 
26.75 
50.0 
9.3066 
9-3548 
0.1590 
— 0.40 
6-55 
4 2029 
7 53 ! 
27.4 
25.2 
2Ó.6 
26.5 
26.42 
48.6 
9.2966 
9.3406 
0.1448 
— 0.36 
6-59 
10 1818 
7 56 
2 9-5 
23.0 
26.5 
25-1 
26.02 
42.4 
9.2843 
9 - 3 I 32 
9 2239 
7 58 
21.6 
18.1 
2 1.0 
20.0 
20.18 
48.1 
9.0756 
9.1182 
Mittel aus den Vergleichsternbeobachtungen: 9-1779; 9.1939; 9.2157. Zur Reduction benutzt: 9.1958. 
*) 7° 1997 dupl. Zuerst die südlich vorangehende Componente gemessen. 
Zone 443. 1891 März 17. 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 20 und Nr. 22. Luft: 1 
—2. 
9°2239 
8 h 4 m 
2 2?4 
i8?i 
i 9 °5 
1 9?o 
19875 
4786 
9.0576 
9.0988 
9 2374 
8 8 
34-5 
35-7 
35 -o 
36.0 
35-30 
51.8 
9-5236 
9-5778 
19 2251 
8 10 
27.9 
24-5 
24-5 
25.0 
25.48 
37 -i 
9.2674 
9.2871 
0.0477 
-f- 0.12 
6.68 
19 2254 
8 12 
25-4 
21.9 
24-5 
22.0 
23-45 
37-3 
9.1997 
9.2197 
0.1151 
+ 0.29 
6.85 
18 2274 
8 14 
16.0 
14.4 
16.0 
14.4 
15.20 
38.0 
8.8372 
8.8583 
0.4765 
4- 1.19 
7-75 
12 2090 
8 19 
38.5 
36.5 
36.5 
38.8 
37-58 
43-3 
9-5705 
9.6013 
0.2665 
— 0.67 
5-89 
12 2095 
8 20 
27-5 
24.0 
24.0 
24.0 
24.88 
43-5 
9.2480 
9.2792 
0.0556 
4- 0.14 
6.70 
12 2105 
8 22 
20.6 
18.4 
20.1 
18.6 
19.42 
43-4 
9.0436 
9.0746 
0.2602 
4-0.65 
7.21 
9 2239 
8 25 
19.8 
18.7 
20.4 
19.0 
19.48 
46.0 
9.0461 
9.0831 
9 2374 
8 27 
42.4 
34-5 
38.5 
37-6 
38.25 
49.8 
9-5836 
9.6312 
13 2128 
8 3 1 
25.0 
21.2 
21.0 
22.4 
22.40 
41.0 
9.1620 
9.1882 
0.1466 
4- 0.37 
6-93 
13 2131 
8 32 
20.5 
19.1 
20.0 
19.6 
19.80 
40.5 
9-0597 
9.0850 
0.2498 
-f- 0.62 
7.18 
13 2136 
8 34 
23.2 
19.0 
20.5 
19.6 
20.58 
40.7 
9.0919 
9.1 1 76 
0.2 I 72 
-f-0.54 
7.10 
14 2134 
8 35 
20.0 
17.2 
I 9-5 
18.4 
18.78 
40.5 
9 -OI 55 
9.0408 
O.294O 
4 - 0.74 
7-30 
14 2136 
8 37 
49.6 
474 
43 -o 
45-5 
46.38 
39-8 
9 - 7 T 94 
9-7435 
O.4087 
— i .02 
5-54 
13 2164 
8 39 
304 
26.0 
29.2 
27.4 
28.25 
41.0 
9-3503 
9-3765 
O.O41 7 
— 0.10 
6.46 
9 2239 
8 41 
20.0 
18.5 
19.7 
19.4 
19.40 
45 -o 
9.0427 
9.0773 
9 2374 
8 43 
35-5 
31-5 
34-5 
35-0 
34-12 
48.2 
9.4978 
9-5407 
Mittel aus den Vergleichsternbeobachtungen: 9.3383; 9.3572; 9.3090. Zur Reduction benutzt: 9.3348. 
Zone 444. 1891 März 17. 
Beobachter: Kempf. 
Photometer: 
D. Vergleichsterne: Nr. 20 und Nr. 
22. Luft: 
2. 
9 ° 2 3 7 4 
8 h 49 m 
3882 
3 280 
3388 
3485 
34862 
4787 
9.5089 
9-5504 
9 2239 
8 52 
21.0 
17.0 
20.5 
18.4 
19.22 
44.4 
9.0349 
9.0681 
4 2328 
8 54 
21.7 
18.7 
19-5 
20.6 
20.12 
51.2 
9-0731 
9.1252 
O.1946 
4 - 0.49 
7-05 
4 2333 
8 55 
18.5 
18.4 
20.5 
16.8 
18.55 
51-5 
9-0053 
9.0584 
O.2614 
-f- 0.65 
7.21 
3 2379 
8 57 
24.0 
21.1 
2 1.1 
23.1 
22.32 
52.3 
9.1590 
9.2150 
0.1048 
+ 0.26 
6.82 
2 2325 
8 58 
x 9-7 
18.8 
18.4 
174 
18.58 
52.9 
9.0066 
9.0648 
0.2550 
+ 0.64 
7.20 
2 2323 
9 0 
19.1 
17.6 
18.4 
18.4 
18.38 
53-2 
8-9975 
9.0569 
O.2629 
+ 0.66 
7.22 
2 2334 
9 3 
25.0 
22.1 
234 
21.6 
23.02 
52.8 
9.1845 
9.2423 
0.0775 
4- 0.19 
6-75 
9 2374 
9 4 
37-7 
33-5 
36.O 
354 
35-65 
46.5 
9 - 531 1 
9.5694 
9 2239 
9 6 
21.2 
17.8 
20.0 
18.5 
19.38 
43-9 
9.0418 
9-0739 
7 2314 
9 8 
17.6 
1 7-5 
18.O 
1 7-5 
I 7-65 
47-5 
8-9635 
9.0044 
0.3154 
4-0.79 
7-35 
7 2330 
9 11 
52.5 
45-0 
46.9 
47-9 
48.08 
47.6 
9-7432 
9.7844 
O.4646 
— 1.16 
5-40 
1 2471 
9 13 
15.0 
134 
13.8 
12.5 
13.68 
53-9 
8-7477 
8.8098 
0.5100 
+ 1.28 
7.84 
3 2408 
9 15 
26.6 
26.0 
28.6 
254 
26.65 
52-3 
9.3036 
9-3596 
0.0398 
— 0.10 
6.46 
4 2378 
9 17 
17-5 
15-5 
1 7-5 
15.8 
16.58 
51-4 
8.9108 
8.9636 
O.3562 
—1“ 0.89 
7-45 
*) 5 2384Ì 
9 19 
16.4 
19-5 
18.9 
16.2 
17-75 
49.8 
8.9682 
9.0158 
0.3040 
4- 0.76 
7-32 
9 21 
30.5 
29.9 
30.5 
27.6 
29.62 
49-7 
9-3879 
9-4352 
O.I154 
— 0.29 
6.27 
9 2374 
9 23 
38.6 
33-5 
33-5 
34-5 
35.02 
45-2 
9 - 5 I 76 
9-5527 
9 2239 
9 25 
21-5 
18.0 
20.2 
20.8 
20.12 
43-4 
9-0731 
9.1041 
Mittel aus den Vergleichsternbeobachtungen : q.^oq^; q.3216; q.3284. 
Zur Reduction benutzt: 9.3198. 
) 5 2 3°4 dupl. Zuerst die südlich vorangehende Componente gemessen. Messungen sehr unsicher.