276 
Müller und Kempf, Photometrische Durchmusterung 
27ß 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
12° 
760 
3 h 
32 m 
1987 
17?6 
1789 
i8?o 
i8?30 
4486 
8.9938 
9.0275 
0.3467 
+ 0.87 
7-32 
IO 
758 
3 
33 
16.5 
15-9 
16.3 
16.6 
16.32 
46.3 
8.8974 
8.9352 
0.4390 
+ I.IO 
7-55 
IO 
760 
3 
34 
14.6 
12.2 
14.1 
T 3-5 
13.60 
46.1 
8.7427 
8.7800 
0.5942 
+ 1.49 
7-94 
IO 
770 
3 36 
14.4 
12.1 
14.0 
12.2 
13-18 
46.2 
8.7159 
8-7534 
0.6208 
+ i -55 
8.00 
i 5 
799 
3 
38 
16.O 
15-9 
15-3 
14.4 
1540 
41.2 
8.8483 
8.8749 
0.4993 
+ 1-25 
7.70 
i6 
765 
3 
40 
27.1 
29.8 
30.6 
29.9 
29-35 
40.6 
9.3807 
9.4062 
0.0320 
— 0.08 
6-37 
11 
632 
3 
42 
2 6.0 
21.6 
21.7 
21.1 
22.60 
42.3 
9- l6 93 
9.1980 
IO 
818 
3 
44 
41.9 
36.3 
37 -° 
35-6 
37-70 
47.2 
9-5728 
9.6129 
Mittel aus den Vergleichsternbeobachtungen: 9.3619; 9.3552; 9.4055. 
*) 19 0 886 dupl. Nur die helle, nördliche Componente gemessen. 
Zur Reduction benutzt: 9.3742. 
**) 15 
893 dupl. Nur die helle, nördliche Componente gemessen. 
Zone 378. 1890 Januar 15 
• 
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 12 
und Nr. 14. Luft: 
—2. 
i o° 
818 
3 1 
o 0 m 
J 2 
3985 
3389 
3382 
3383 
34898 
4883 
9.5168 
9.5600 
IO 
1149 
3 
35 
28.4 
24-5 
27.0 
26.8 
26.68 
53-8 
9-3045 
9.3662 
5.82 
1Ó 
822 
3 
38 
39-6 
35 -o 
38.7 
37-5 
37-70 
41.9 
9.5728 
9.6007 
0.1078 
— 0.27 
IO 
828 
3 
39 
33-3 
29.7 
32.5 
31.0 
31.62 
47. 1 
9 - 439 1 
9.4790 
0.0139 
+ 0.03 
6.12 
IO 
855 
3 
41 
16.7 
14.2 
16.5 
14.6 
15-50 
47-9 
8.8538 
8.8958 
0.5971 
+ 1.49 
7-58 
12 
852 
3 
43 
18.3 
17.2 
* 7-3 
16.9 
17.42 
45-2 
8-9525 
8.9876 
0.5053 
+ 1.26 
7-35 
I 2 
884 
3 
44 
27.2 
22.6 
25-4 
24.4 
24.90 
45-8 
9.2486 
9.2851 
0.2078 
+ 0.52 
6.61 
14 
991 
3 
46 
23.0 
21.1 
21.8 
20.8 
21.68 
44.2 
9-1350 
9.1678 
0.3251 
+ 0.81 
6.90 
IO 
818 
3 
47 
38.5 
37 -o 
38.1 
36.0 
37-40 
46.9 
9.5669 
9.6062 
IO 
1149 
3 
49 
28.9 
27-3 
29.1 
27-3 
28.15 
52.1 
9-3475 
9.4028 
8.62 
*W c 
ss?/ 
3 
53 
12.6 
8-3 
10.2 
7-7 
9.70 
42.1 
8-4531 
8.4814 
1.0115 
+ 2.53 
B 5 
3 
54 
21.2 
20.2 
20.4 
20.8 
20.65 
42.0 
9.0947 
9.1228 
0.3701 
~b 0-93 
7.02 
i6 
855 
3 
55 
21.5 
I9.2 
20.0 
19.2 
19.98 
41.7 
9.0673 
9.0948 
0.3981 
-f- 1.00 
7.09 
926 
3 
56 
34-4 
29.4 
31-1 
32.0 
3 i -72 
42.0 
9.4416 
9.4697 
0.0232 
4- 0.06 
6.15 
18 
920 
3 
58 
18.5 
154 
18.7 
15.8 
17.10 
38.6 
8.9368 
8.9589 
0.5340 
+ i -34 
7-43 
18 
923 
3 
59 
20.6 
19.8 
22.6 
21.7 
21.18 
38.5 
9 - 1 1 57 
9 -I 376 
0.3553 
+ 0.89 
6.98 
18 
950 
4 
i 
25.6 
22.5 
26.6 
23.1 
2445 
38.8 
9-2338 
9.2562 
0.2367 
+ 0.59 
6.68 
IO 
818 
4 
3 
37-9 
34-4 
35-1 
39-5 
36.72 
45-6 
9-5533 
9-5893 
IO 
1149 
4 
5 
30.3 
29.2 
29-3 
29.1 
29.48 
50.2 
9.3842 
9-4330 
Mittel aus den 
Vergleichsternbeobachtungen: 9.4631; 9.5045; 9.5112. 
Zur Reduction benutzt: 9.4929 
*) 150887 dupl. Zuerst die vorangehende Componente gemessen. 
Zone 379. 1890 Januar 15. 
Beobachter: Kempf. Photometer: 1 ). Vergleichsterne: Nr. 14 
und Nr. 16. Luft: 
[—2. 
IO° 
1149 
5 1 
2Ó m 
3584 
28°5 
3188 
32?0 
31892 
4385 
9.4465 
9-4777 
11 
1588 
5 
29 
28.0 
26.0 
28.1 
27.9 
27.50 
46.9 
9.3288 
9.3681 
8.00 
*) 9 
1 345 < | 
5 
31 
13.6 
13.2 
14.4 
15.0 
14.05 
45-2 
8.7704 
8.8055 
0.6137 
+ i -53 
5 
32 
20.4 
18.7 
20.6 
19.6 
19.82 
45 -i 
9.0605 
9-0953 
0.3239 
+ 0.81 
7.28 
o 
1546 
5 
34 
36.8 
31.6 
34-6 
34 -i 
34.28 
53-3 
9.5014 
9 - 56 ii 
0.1419 
— 0.35 
6.12 
6 
1 3 5 1 
5 
37 
29.4 
25.2 
25.6 
28.1 
27.08 
47-5 
9-3165 
9-3574 
0.0618 
+ 0.15 
6.62 
7 
1409 
5 
38 
23-5 
21.5 
22.6 
22.0 
22.40 
46.4 
9.1620 
9.2000 
0.2 I92 
+ 0.55 
7.02 
3 
1359 
5 
40 
20.9 
18.5 
20.4 
18.5 
19.58 
50.3 
9.0504' 
9.0995 
O.3197 
0.80 
7.27 
3 
1371 
5 
41 
32.0 
3 i-i 
31.8 
31.0 
31.48 
50.6 
9-4357 
9.4858 
0.0666 
— 0.17 
6.30 
IO 
1149 
5 
43 
37 -o 
29-5 
34-7 
29-5 
32.68 
42.7 
9.4647 
9.4942 
11 
1588 
5 
45 
29.6 
23.2 
25-9 
26.1 
26.20 
45-5 
9.2899 
9-3257 
5 
1380 
5 
47 
20.7 
17.0 
20.0 
16.0 
18.42 
47.6 
8-9993 
9.0405 
0.3787 
4- 0.95 
7.42 
4 
1414 
5 
49 
35-7 
3 1-I 
30.1 
334 
32.58 
49.4 
9.4623 
9.5087 
0.0895 
— 0.22 
6.25 
9 
*376 
5 
51 
24.9 
21.5 
23-5 
22.0 
22.98 
43-6 
9.1831 
9.2145 
0.2047 
+ 0.51 
6.98 
8 
i486 
5 
52 
39-5 
32.0 
324 
324 
34.08 
44.8 
9.4969 
9 - 53 IO 
0.1 I 18 
— 0.28 
6.19 
9 
1393 
5 
54 
23.0 
19.0 
* 9-9 
20.5 
20.60 
44-5 
9.0927 
9.1261 
O.2931 
0.73 
7.20 
i 
1531 
5 
55 
27.8 
25-4 
28.5 
27.0 
27.18 
52.3 
9 - 3 I 94 
9-3754 
O.O438 
4- 0.11 
6.58 
IO 
1149 
5 
57 
35-5 
29.8 
34-5 
34 -o 
33-45 
42.3 
9.4827 
9 - 5 II 4 
11 
1588 
5 
59 
31.8 
23.8 
26.0 
25.2 
26.70 
44.4 
9-3051 
9-3383 
Mittel aus den Vergleichsternbeobachtungen: 9.4229; 9.4100; 9.4248. 
Zur Reduction benutzt: 9.4192. 
*) 9 ° 
1345 dupl. Zuerst die nördlich vorangehende Componente gemessen.