368 
Müller und Kempf, Photometrische Durchmusterung 
368 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 / 
corri g. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
14 0 4074 
2 2 h 4 ,n 
i 4 ?7 
I 2?2 
I 2?0 
9?7 
12? 15 
4682 
8.6464 
8.6839 
0.4703 
-h 1.18 
7.98 
19 4195 
22 6 
16.7 
14.2 
15.0 
13-7 
14.90 
41.8 
8.8203 
8.8480 
0.3062 
+ 0.77 
7-57 
10 3981 
22 8 
21.0 
18.5 
18.O 
18.6 
19.02 
52.1 
9.0262 
9.0815 
10 4351 
22 10 
25.8 
20.4 
2 2.4 
22.8 
22.85 
45-8 
9.1784 
9.2149 
16 4053 
22 13 
14.6 
I 1.2 
I 1.6 
11-9 
12.32 
45-7 
8.6583 
8.6946 
0.4596 
4 - 1.15 
7-95 
16 4103 
22 14 
14.1 
I 2.2 
13.2 
12.2 
12.92 
45 -i 
8.6989 
8-7337 
0.4205 
4- 1.05 
7-85 
10 4189 
22 16 
25.0 
22.8 
2 I.9 
19.4 
22.28 
49.8 
9-1576 
9.2052 
0.05 IO 
— 0.13 
6.67 
7 4467 
22 19 
ii -4 
10.0 
10.6 
9.2 
10.30 
5 1 -i 
8.5047 
8.5564 
0.5978 
4 - 1.50 
8.30 
10 3981 
22 22 
22.2 
19.8 
21.1 
17.0 
20.02 
53-9 
9.0689 
9 -I 3 IO 
10 4351 
22 24 
23.1 
20.6 
22.6 
22.0 
22.o8 
47.1 
9.1502 
9.1901 
Mittel aus den Vergleichsternbeobachtungen: 9.1538; 9.1482; 9.1605. 
Zur Reduction benutzt: 9.1542. 
Revisions 
-Zone 12. 
1890 November 7. 
Beobachter : Kempf. 
Photometer : 
D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 
2. 
io°398i 
2 I h 2 Ó m 
24?0 
20?8 
2385 
2 i?o 
2 2?3 2 
4786 
9.1590 
9.2002 
10 4351 
2 i 28 
29.4 
26.4 
29.6 
26.5 
27.98 
42.9 
9.3426 
9-3725 
18 4168 
21 3 ° 
19.7 
17-5 
20.5 
17.6 
18.82 
41.0 
9-0173 
9-0435 
0.2255 
4-0.56 
7-36 
12 4059 
21 34 
29.0 
26.0 
28.4 
27.0 
27.60 
45-6 
9-3317 
9-3677 
0.0987 
— 0.25 
6-55 
14 4074 
21 36 
16.5 
12.5 
15-5 
13-5 
I4.5O 
43-2 
8.7972 
8.8277 
0.4413 
+ I.IO 
7.90 
19 4195 
21 38 
19.0 
15-5 
17.0 
16.2 
16.92 
38.7 
8.9279 
8.9501 
0.3189 
4- 0.80 
7.60 
10 3981 
21 41 
23.0 
19.6 
23-7 
22.6 
22.22 
49.1 
9-1553 
9.2008 
10 4351 
21 43 
29.0 
25-7 
26.5 
23-5 
26.18 
43-8 
9.2893 
9 - 32 II 
16 4053 
21 46 
17.6 
15.0 
17.1 
15-9 
16.4O 
42.7 
8.9015 
8.9310 
0.3380 
+ 0.85 
7-65 
16 4103 
21 48 
16.2 
14.7 
17.1 
14.8 
I 5-70 
42.3 
8.8647 
8.8934 
0.3756 
4-0.94 
7-74 
10 4189 
21 50 
29.6 
25-7 
26.4 
27.0 
27.18 
47.2 
9-3194 
9-3595 
0.0905 
— 0.23 
6-57 
7 4467 
21 53 
15.6 
11.2 
13.2 
11-5 
12.88 
48.7 
8.6963 
8.7406 
0.5284 
4 - 1.32 
8.12 
10 3981 
21 55 
22.6 
20.6 
22.8 
22.5 
22.12 
50.6 
9 -i 5 i 6 
9.2017 
10 4351 
21 57 
29.O 
24.0 
27.0 
24.0 
26.00 
44.8 
9.2837 
9.3178 
Mittel aus den Vergleichsternbeobachtungen: 9.2864; 9.2609; 9.2598. 
Zur Reduction benutzt: 9.2690. 
Revisions-Zone 13. 
i8go December 15. 
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 2 
— 3- 
io°46o4 
O^ i4 m 
2880 
2387 
2587 
2583 
25868 
5286 
9-2737 
9-3308 
17 4693 
O 19 
26.6 
22.8 
24.9 
23-5 
24-45 
44.0 
9.2338 
9.2661 
0.0016 
0.00 
6.54 
12 4760 
O 22 
14.2 
12.8 
13-5 
13.2 
13.42 
48.6 
8 . 73 I 3 
8-7753 
0.4892 
4- i.22 
7.76 
9 51 ii 
O 24 
25.0 
21.1 
22.5 
20.6 
22.30 
47.1 
9-1583 
9.1982 
Mittel 
aus den Vergleichsternbeobachtungen: 9.2645. Zur Reduction benutzt: 9.2645. 
Revisions 
-Zone 14. 
1890 December 15. 
Beobachter: 
Müller. Photometer 
Ci. Vergleichsterne: Nrr. 
1, 3 und 5. Luft: 2. 
0 
0 
00 
O b 37 m 
2083 
22?3 
20?2 
2385 
21858 
4283 
9-1312 
9-1599 
14 in 
0 39 
24.1 
23.1 
22.3 
21.2 
22.68 
37-5 
9.1723 
9.1926 
0.0917 
— 0.23 
5-64 
11 96 
O 41 
22.O 
22.5 
22.6 
20.4 
2 1.88 
41.0 
9.1426 
9.1688 
4 293 
0 44 
37-4 
36.6 
38.O 
33-3 
36.32 
48.7 
9-5451 
9.5894 
0.4885 
— 1.22 
4-65 
io 252 
0 46 
16.4 
18.3 
I 7.8 
16.4 
I 7 .22 
43-5 
8.9427 
8-9739 
Mittel 
aus den Vergleichsternbeobachtungen: 9.1009. Zur Reduction benutzt: 9.1009. 
Revisions-Zone 15. 
1890 December 15. 
Beobachter: Kempf. 
Photometer : 
D. Vergleichsterne: Nr. 4 und Nr. 6. 
Luft: 1— 
-2. 
io° 168 
O h 54 ™ 
19?6 
1780 
20?5 
1985 
19815 
4186 
9.0319 
9.0592 
8 385 
0 57 
32.0 
29-5 
28.5 
27.9 
29.48 
46.8 
9.3842 
9-4233 
9 167 
1 0 
19.4 
16.7 
14.9 
15.8 
16.70 
42.8 
8.9169 
8.9466 
0.3035 
4- 0.76 
7-44 
*) 2 211 
1 2 
21.7 
20.2 
2 I.4 
20.5 
20.95 
49-5 
9.1067 
9-1534 
0.0967 
4- 0.24 
6.92