282 
Müller und Kempf, Photometrische Durchmusterung 
282 
B.D. 
Sternzeit 
I 
11 
III 
IV 
J 
Z 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
9 ° 34 2 4 
19 11 5Ó m 
3585 
3186 
3283 
29?0 
32810 
5280 
9.4508 
9-5057 
io 3573 
19 58 
24-5 
21.5 
22.4 
21.1 
22.38 
45-2 
9-1613 
9.1964 
i6 3390 
20 0 
31.0 
29.9 
29.0 
28.0 
29.48 
42.4 
9.3842 
9 - 4 I 3 I 
0.0616 
— O.15 
6.23 
16 3405 
20 1 
22.1 
20.0 
21.5 
20.0 
20.90 
42.5 
9.1047 
9 -I 338 
0.2177 
+ O.54 
6.92 
18 3582 
20 3 
18.0 
15-9 
16.2 
16.5 
16.65 
40.9 
8.9144 
8.9404 
0.4111 
+ 1.03 
7.41 
17 348 i 
20 5 
15-1 
14.0 
14.0 
12.9 
14.00 
41-3 
8.7674 
8.7942 
0.5573 
+ i -39 
7-77 
12 3422 
20 7 
16.6 
13.6' 
13.0 
I4.O 
14.30 
46.5 
8.7854 
8.8237 
0.5278 
4 - 1-32 
7.70 
ii 3379 
20 8 
20.0 
18.0 
19.7 
l8.1 
18.95 
47.1 
9.0231 
9.0630 
0.2885 
+ 0.72 
7.10 
9 3424 
20 IO 
31-7 
29.4 
28.5 
29.O 
29.65 
53-7 
9.3887 
9.4500 
10 3573 
20 12 
27.0 
21.8 
22.6 
23-5 
23.72 
46.4 
9.2090 
9.2470 
Mittel aus den Vergleichsternbeobachtungen: 9.3551; 9.3510; 9.3485. Zur Reduction benutzt: 9.3515 
*) 1203383 dupl. Zuerst die südlich vorangehende Componente gemessen. 
Zone 
393 - 
1890 September 18. 
Beobachter: Müller. 
Photometer: D. Vergleichsterne: Nr. 38 und Nr. 40. Luft: 1 
—2. 
i ° 0 3 5 7 3 
20 h I5 m 
2 2?8 
1984 
21?0 
1980 
20°55 
4687 
9.0907 
9-1295 
10 3981 
20 17 
21.7 
17-5 
18.7 
17.7 
18.90 
42.5 
9.0209 
9.0500 
9 3951 
20 19 
19.4 
17.7 
18.O 
17.9 
18.25 
45-8 
8 - 99 1 5 
9.0280 
0.0765 
+ 0.19 
7-03 
5 4007 
20 2 1 
15.6 
14.1 
14.9 
14.0 
14.65 
49.6 
8.8059 
8.8529 
0.2516 
-ho.63 
7-47 
2 3753 
20 23 
17-5 
14.1 
1 7.0 
14.0 
15-65 
53-2 
8.8620 
8.92 14 
0.1831 
4- 0.46 
7-30 
2 3756 
20 25 
18.0 
14.8 
16.2 
15-3 
16.08 
53-3 
8.8849 
8.9447 
0.1598 
4- 0.40 
7.24 
i 3854 
20 2Ó 
18.5 
17-3 
1 7.6 
16.0 
17-35 
53-9 
8.9491 
9.01 12 
0.0933 
+ 0.23 
7.07 
8 3951 
20 28 
26.0 
23.0 
22.3 
23-9 
23.80 
47-9 
9.2118 
9-2538 
0.1493 
— 0.37 
6.47 
10 3573 
20 30 
22.6 
18.9 
234 
19.7 
21.15 
48.1 
9.1146 
9-1572 
10 3981 
20 32 
21.7 
17.6 
19.1 
18.1 
19.12 
43-3 
9.0306 
9.0614 
9 3968 
20 33 
14-3 
11.8 
134 
12.0 
12.88 
47.1 
8.6963 
8.7362 
0.3683 
4- 0.92 
7.76 
9 3979 
20 34 
18.0 
16.4 
17.8 
16.8 
17-25 
47.0 
8.9442 
8.9838 
0.1207 
+ 0.30 
7.14 
0 4088 
20 36 
19.7 
17.0 
19-5 
18.6 
18.70 
55-9 
9.0120 
9.0827 
0.02 18 
+ 0.05 
6.89 
i 3865 
20 38 
32.2 
26.7 
27.1 
2Ó.6 
28.15 
54-8 
9-3475 
9-4134 
O.3089 
— 0.77 
6.07 
2 3765 
20 39 
18.1 
15.0 
15-7 
15-7 
16.12 
54-2 
8.8870 
8.9503 
0.1542 
+ 0.39 
7-23 
3 3882 
20 40 
19.9 
17.6 
18.2 
17.9 
18.40 
53-4 
8.9984 
9-0585 
O.O460 
4- 0.11 
6-95 
10 3573 
20 42 
23.1 
18.9 
23.8 
19.2 
21.25 
49.4 
9.1185 
9.1649 
10 3981 
20 44 
20.8 
18.2 
19.0 
18.6 
I 9 -I 5 
44.0 
9.0319 
9.0642 
Mittel aus den Vergleichsternbeobachtungen: 9.0898; 9.1093; 9.1145. Zur Reduction benutzt: 9.1045 
Zone 
394 - 
1890 September 18. 
Beobachter: Kempf. Photometer: D 
Vergleichsterne: Nr. 40 und Nr. 42 
Luft : I 
—2. 
io°398i 
24 57 m 
2I?5 
i8°9 
20?0 
i8?i 
19862 
5088 
9.0521 
9.1028 
10 4351 
22 0 
27-3 
23.0 
2 Ó.I 
23.2 
24.90 
45.0 
9.2486 
9.2832 
15 4171 
22 3 
16.6 
14.9 
16.4 
14.8 
15.68 
41.4 
8.8636 
8.8906 
O.3024 
4- 0.76 
7-56 
15 4181 
22 4 
22.5 
16.5 
I9.8 
19-5 
19.58 
41.7 
9.0504 
9.O779 
0.1151 
4- 0.29 
7.09 
15 4185 
22 6 
14.0 
11-5 
I4.9 
12.1 
13.12 
41.7 
8.7120 
8-7395 
0.4535 
4 -1.13 
7-93 
15 4187 
22 8 
16.0 
12.6 
I4.O 
11-5 
13-52 
41.9 
8-7377 
8.7656 
O.4274 
4-1.07 
7.87 
16 4291 
22 9 
20.1 
16.5 
20.0 
19.7 
19.08 
41.2 
9.0288 
9-0554 
0.1376 
4- 0.34 
7.14 
16 4288 
22 I I 
19.0 
15-5 
17.8 
15.6 
16.98 
41-3 
8.9309 
8-9577 
0.2353 
4-0.59 
7-39 
*)io 4307 <[ 
22 13 
22 14 
17.0 
19-5 
13-5 
16.5 
I5.6 
i 8.5 
15.0 
18.1 
15-28 
18.15 
46.8 
46.9 
8.8417 
8.9869 
8.8808 
9.0262 
O.3 122 
O.IÓ68 
4- 0.78 
+ 0.42 
7.58 
7.22 
10 3981 
22 17 
21.0 
18.5 
20.0 
18.0 
19.38 
53-2 
9.0418 
9.1012 
10 4351 
22 ig 
27-5 
23-5 
24.O 
24-5 
24.88 
46.6 
9.2480 
9.2865 
19 4423 
22 2 1 
2 5-5 
21.7 
22.9 
23.1 
23 - 3 ° 
39-7 
9.1944 
9.2183 
O.O253 
— 0.06 
6-74 
19 4426 
22 22 
22.4 
19-5 
20.5 
18.4 
20.20 
40.1 
9.0764 
9.1010 
O.O92O 
-4 0.23 
7-03 
18 4517 
22 24 
21.1 
17.6 
2O.4 
19-5 
I9.65 
40.6 
9-0534 
9.0789 
O. I I41 
4- 0.29 
7.09 
18 4525 
22 25 
17.8 
18.7 
19-5 
19.0 
i 8.75 
41.2 
9.0142 
9.0408 
O. I 522 
4- 0.38 
7.18 
17 4355 
22 2Ó 
234 
21.7 
20.1 
17.9 
20.78 
41-5 
9.0999 
9.1270 
O.0660 
4-0.17 
6.97 
12 4378 
22 28 
41-5 
37 -i 
37-8 
37-5 
38.48 
46.3 
9-5879 
9.6257 
O.4327 
— 1.08 
5-72 
10 4351 
22 30 
27.0 
22.5 
23.6 
23-5 
24.15 
47-7 
9.2237 
9.2652 
10 3981 
22 33 
22.0 
17.4 
19.0 
20.0 
I9.60 
55-3 
9-0513 
9- 1 193 
Mittel aus den Vergleichsternbeobachtungen 
: 9.1930; 9.1939; 9.1922. Zur Reduction benutzt: 9.1930. 
*) io°4307 dupl. Zuerst die südlich vorangehende Componente gemessen. Messungen unsicher.