246 
Müller und Kempf, Photometrische Durchmusterung 
246 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
ii° 
96 
i 1 
i6 m 
i8?9 
I 7 ?2 
i8?7 
1/84 
18805 
4186 
8.9823 
9.0096 
IO 
252 
1 
17 
16.5 
l6.1 
18.6 
13-5 
16.18 
42.3 
8.8901 
8.9188 
19 
279 
1 
20 
21.8 
20.3 
21.8 
19.4 
20.82 
32.8 
9-1015 
9 *i 1 57 
0.1605 
— O.40 
5-52 
8 
273 
1 
21 
37 -o 
32.1 
33-6 
32.6 
33 - 82 
44.0 
9 - 49 11 
9-5234 
0.5682 
— 1.42 
4-50 
2 
290 
1 
23 
29.0 
25.2 
28.0 
26.2 
27.10 
50.1 
9 - 3 1 7 1 
9-3656 
0.4104 
— 1-03 
4.89 
1 7 
289 
1 
25 
25-7 
21.3 
23.0 
22.5 
23.12 
35-5 
9.1880 
9-2055 
0.2503 
— O.63 
5-29 
8 
345 
1 
27 
3 i -7 
27.9 
3 1-I 
30.9 
30.40 
44.8 
9.4084 
9.4425 
0.4873 
1.22 
4.70 
i 
410 
1 
29 
18.6 
16.9 
19.0 
17.8 
18.08 
52.0 
8.9837 
9.0386 
0.0834 
0.2 I 
5 - 7 1 
11 
96 
1 
30 
20.4 
16.9 
19.7 
16.2 
18.30 
42.2 
8.9938 
9.0223 
IO 
252 
1 
32 
16.0 
14.0 
154 
13.2 
14.65 
42.0 
8.8059 
8.8340 
Mittel aus den Vergleichsternbeobachtungen: 8.9731; 8.9642; 8.9282. Zur Reduction benutzt: 8.9352. 
Zone 303. 1889 Januar 2. 
Beobachter: Iiempf. 
Photometer: 
D. Vergleichsterne: Nr. 8 
und Nr. 10. Luft: 
2. 
9 ° 
472 
2 1 
3 ! m 
19?i 
i6?o 
l8?0 
i8?o 
i 7°78 
4487 
8.9696 
9-0035 
11 
632 
2 
34 
22.9 
24.O 
24.1 
22.5 
23-38 
47-3 
9.1972 
9.2376 
18 
632 
2 
37 
19.0 
I7.9 
17.9 
18.1 
18.22 
39-2 
8.9901 
9 -OI 3 I 
0.1410 
+ 0.35 
7.60 
18 
633 
2 
39 
3 i -7 
34 -o 
31.O 
31.0 
31.92 
38.8 
9-4465 
9.4689 
0.3148 
— O.79 
6.46 
18 
634 
2 
43 
1 1-5 
10.1 
10.0 
8.6 
10.05 
38.7 
8.4836 
8.5058 
0.6483 
4 * I.62 
8.87 
18 
636 
2 
45 
15-5 
16.1 
194 
18.6 
17.40 
38.5 
8.9515 
8-9734 
0.1807 
+ O.45 
7.70 
*)i8 
637 
2 
47 
16.0 
15-3 
154 
14.9 
15.40 
38.1 
8.8483 
8.8696 
0.2845 
4 - 0.71 
7.96 
**)i 7 
724 
2 
49 
24.0 
19-5 
22.1 
22.6 
22.05 
38.8 
9.1491 
9 - 1 7 1 5 
0.0174 
— 0.04 
7.21 
17 
731 
2 
52 
23-7 
21.8 
234 
21.5 
22.60 
39-4 
9.1693 
9.1927 
O.O386 
— 0.10 
7 -i 5 
11 
632 
2 
55 
25-5 
25.6 
25.O 
27.0 
25.78 
45-4 
9.2768 
9.3124 
9 
472 
2 
57 
21.4 
18.4 
22.2 
16.5 
19.62 
43-4 
9.0521 
9.0831 
15 
62 1 
3 
0 
27.9 
26.3 
28.0 
28.5 
27.68 
39-9 
9-3340 
9.3582 
O.2041 
— 0.51 
6-74 
16 
602 
3 
3 
22.9 
25.8 
24-3 
24-5 
24.38 
38.7 
9.2314 
9-2536 
O.O995 
— 0.25 
7.00 
15 
633 
3 
5 
24.6 
24.6 
254 
24-5 
24.78 
39-6 
9.2447 
9.2684 
O.II43 
— 0.29 
6.96 
14 
702 
3 
8 
34-4 
32.7 
364 
35-5 
34.88 
40-7 
9 - 5 I 46 
9-5403 
0.3862 
— 0.97 
6.28 
IO 
577 
3 
10 
35 -o 
37-3 
37-3 
33 -o 
35-65 
43-8 
9 * 53 11 
9-5630 
0.4089 
— 1.02 
6.23 
I I 
614 
3 
12 
17.1 
16.5 
18.5 
15-5 
16.90 
43-2 
8.9269 
8-9574 
O.1967 
+ O.49 
7-74 
11 
632 
3 
14 
24-5 
22.6 
234 
23-5 
23-50 
43-9 
9.2014 
9-2335 
9 
472 
3 
17 
20.5 
17-4 
194 
18.6 
18.98 
42.9 
9.0244 
9-°543 
Mittel aus den Vergleichsternbeobachtunge 
n: 9.1206; 9.1977; 9.1439. 
Zur Reduction benutzt: 9.1541. 
*) 18 637 dupl. Gemessen die hellere, 
nördliche Componente. 
**) 17 724 dupl. Gemessen die hellere, südlich vorangehende Componente. 
Zone 304. 1889 Januar 3. 
Beobachter: Kempf. 
Photometer: 
D. Vergleichsterne: Nr. 14 
und Nr. 16. Luft: 
I. 
IO° 
1149 
5 1 
2 m 
3185 
338 i 
3389 
3384 
32898 
4580 
9.4717 
9-5063 
11 
1588 
5 
4 
29.0 
254 
28.0 
27.0 
27-35 
49-5 
9-3245 
9-3712 
16 
1326 
5 
7 
29-5 
24.0 
24.6 
28.0 
26.52 
4 i -5 
9.2997 
9.3268 
0.0986 
4 0.25 
6.72 
17 
1447 
5 
9 
23-5 
22.4 
23.0 
22.5 
22.85 
39-8 
9.1784 
9.2025 
O.2229 
4 O.56 
7-03 
IO 
1335 
5 
11 
33 -o 
38.6 
37-5 
34-2 
35.82 
46.8 
9-5346 
9-5737 
0.1483 
— 0.37 
6.10 
12 
1361 
5 
13 
29.8 
27.0 
29.4 
27.6 
28.45 
44.8 
9-3559 
9.3900 
O.0354 
4 O.O9 
6.56 
l8 
1423 
5 
15 
21.4 
19.0 
ig.g 
21.3 
20.40 
39 -i 
9.0846 
9- io 75 
0-3179 
+ O.79 
7.26 
19 
1559 
5 
16 
18.5 
19.9 
18.1 
18.5 
18.75 
37-9 
9.0142 
9 - 035 I 
O.3903 
4 O.98 
7-45 
IO 
1149 
5 
18 
30.1 
30-5 
3 i -5 
32.0 
31.02 
43-9 
9.4242 
9-4563 
I I 
1588 
5 
20 
31.0 
26.6 
28.7 
31.0 
29.32 
47.8 
9-3798 
9.4216 
l6 
1352 
5 
23 
23.2 
19.0 
21.6 
21.4 
21.30 
40.4 
9.1204 
9- I 455 
O.2799 
4- 0.70 
7.17 
l6 
1354 
5 
24 
35 -o 
43-2 
39-6 
43-2 
40.25 
40.3 
9.6206 
9-6455 
0.2201 
— 0.55 
5-92 
15 
1412 
5 
26 
23.2 
20.6 
22.4 
25.0 
22.80 
40.6 
9.1766 
9.2021 
O.2233 
4- 0.56 
7-03 
15 
1416 
‘ 5 
27 
24.9 
23.1 
23-9 
24.0 
23.98 
40.8 
9.2179 
9-2437 
O.1817 
4- 0.45 
6.92 
IO 
1370 
5 
29 
26.5 
22.0 
234 
21.2 
23-30 
45 - 1 
9.1944 
9.2292 
0.1962 
4 0.49 
6.96 
11 
1408 
5 
3 i 
22.5 
21.6 
24.0 
22.6 
22.68 
43-9 
9 -I 723 
9.2044 
0.22 IO 
+ 0.55 
7.02 
IO 
1149 
5 
33 
34 -o 
34-5 
29.4 
28.1 
31-50 
43 -i 
9.4362 
9.4665 
11 
1588 
5 
35 
28.5 
24.0 
27.0 
25.6 
26.28 
46.4 
9.2923 
9-3303 
Mittel aus den Vergleichsternbeobachtungen: 9.4388; 9.4389; 9.3984. Zur Reduction benutzt: 9.4254.