208 
Müller und Kempf, Photometrische Durchmusterung 
208 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
8 ° 28 5 7 
13h j^m 
26? 7 
2 8?7 
3°?3 
0 • 
C\| 
28835 
45?5 
9-3531 
9.3889 
ii 2780 
13 18 
234 
24.6 
22.8 
22.8 
23.40 
46.9 
9-1979 
9.2372 
18 2972 
13 20 
17-3 
17.2 
20.0 
17.6 
18.02 
39 -o 
8.9809 
9.0036 
0.3270 
+ 0.82 
7.27 
19 2924 
13 22 
28.7 
29.0 
31-5 
27.8 
29.25 
38.8 
9.3780 
9.4004 
0.0698 
— O.17 
6.28 
11 2774 
13 23 
16.1 
14.0 
15.6 
15-1 
15.20 
45-9 
8.8372 
8.8740 
0.4566 
+ 1.14 
7-59 
12 2796 
13 25 
20.7 
22.4 
21.5 
20.5 
21.28 
45 -o 
9.1196 
9 - I 54 2 
0.1764 
+ O.44 
6.89 
13 2899 
13 26 
18.5 
16.4 
194 
17.6 
i 7-98 
44.0 
8.9791 
9.0114 
0.3192 
+ 0.80 
7-25 
13 2901 
13 28 
28.0 
28.5 
27-5 
2 7-5 
27.88 
43-2 
9-3398 
9-3703 
0.0397 
— O.IO 
6-35 
11 2780 
13 29 
25.0 
25-3 
24.9 
23-3 
24.62 
45-9 
9-2395 
9.2763 
8 2857 
13 31 
29-5 
26.5 
28.8 
28.1 
28.22 
44.8 
9-3495 
9-3836 
Mittel aus den Vergleichsternbeobachtungen: 9.3488; 9.3130; 9.3300. Zur Reduction benutzt: 9.3306. 
Zone 208. 1888 
Mai 16. 
Beobachter: Müller. 
Photometer: D. Vergleichsterne: Nr. 30 und Nr. 32. Luft: 
2. 
8°28 57 
I 3 h I 3 m 
3i?o 
2588 
28?4 
26? 7 
27898 
4586 
9.3426 
9.3786 
ii 2780 
13 15 
21.7 
22.6 
25.6 
22.0 
22.98 
47.0 
9.1831 
9.2227 
10 2804 
13 16 
17.0 
15.6 
18.6 
17.0 
17-05 
47-4 
8.9344 
8-9751 
0.2987 
+ 0.75 
7.20 
10 2805 
13 18 
14.7 
14.7 
14.7 
14.9 
14-75 
47.6 
8.8117 
8.8529 
0.4209 
4-1.05 
7-50 
IO 2816 
i 3 19 
16.6 
17.0 
16.7 
154 
16.42 
47-5 
8.9025 
8.9434 
0-3304 
4-0.83 
7.28 
19 2937 
13 21 
16.7 
15-3 
17-3 
1 5-6 
16.22 
38-9 
8.8922 
8 - 9 i 47 
0-3591 
4- 0.90 
7-35 
13 22 
20.4 
18.4 
20.5 
18.4 
19.42 
38.6 
9.0436 
9.0657 
0.2081 
4~ 0.52 
6.97 
) *9 2959j 
13 23 
13.0 
11-4 
13-7 
12.3 
12.60 
38.5 
8.6775 
8.6994 
o -5744 
+ i -44 
7.89 
11 2780 
13 24 
22.2 
20.4 
21.4 
20.9 
21.22 
46.2 
9 -H 73 
9.1548 
8 2857 
13 26 
24.8 
26.8 
27-3 
28.6 
26.88 
44.9 
9-3105 
9-3449 
H 2853 
13 30 
1 5-7 
154 
16.5 
15-4 
1 5-7 5 
43-4 
8.8674 
8.8984 
0-3754 
+ 0.94 
7-39 
10 2818 
13 31 
19.2 
174 
18.9 
17.8 
18.32 
46.9 
8.9947 
9.0340 
0.2398 
+ 0.60 
7-05 
**110 282 2! 
13 33 
9-5 
74 
10.5 
8.7 
9.02 
46.2 
8.3906 
8.4281 
0.8457 
4- 2.11 
8.56 
13 34 
16.9 
14.7 
17-5 
16.1 
16.30 
46.1 
8.8964 
8-9337 
0.3401 
+ 0.85 
7-30 
15 2845 
13 36 
134 
12.3 
144 
12.9 
13-25 
42.2 
8.7204 
8.7489 
0.5249 
4 -1.31 
7.76 
13 2928 
13 38 
22.1 
21.4 
22.5 
21.9 
21.98 
44.1 
9 .Ì 4 Ó 4 
9.1789 
0.0949 
+ 0.24 
6.69 
19 2961 
J 3 39 
14.8 
* 5-5 
15-5 
144 
15-05 
38.3 
8.8288 
8.8504 
0.4234 
4-1.06 
7-51 
11 2780 
13 41 
22.0 
21.1 
22.7 
21.7 
21.88 
44.8 
9.1426 
9.1767 
8 2857 
13 43 
28.4 
28.3 
27-3 
26.5 
27.62 
44.2 
9-3323 
9-3651 
Mittel aus den Vergleichsternbeobachtungen: 9.3007; 9.2498; 9.2709. Zur Reduction benutzt: 9.2738. 
*) 1902939 dupl. 
Zuerst die südliche Componente gemessen. 
**) 10 2823 dupl. 
Zuerst die südliche Componente gemessen. 
Zone 20Q. 1888 Mai 16. 
Beobachter: Kempf. 
Photometer: 
D. Vergleichsterne: Nr. 32 und Nr. 34. Luft: 
2. 
O 
00 
0 
13 h 48*“ 
2 I?4 
22 ?I 
2 2?4 
2 380 
2 282 2 
4482 
9-1553 
9.1881 
9 3203 
13 52 
18.4 
18.4 
22.5 
17.4 
19.18 
52.2 
9-0331 
9.0887 
18 3010 
13 54 
”•5 
II -4 
12.8 
11.8 
11.88 
38.0 
8.6272 
8.6483 
0.5025 
4- 1.26 
8.06 
18 3OI9 
13 55 
12.0 
11-5 
12.9 
10.6 
ii -75 
37-8 
8.6178 
8.6386 
0.5122 
4- 1.28 
8.08 
10 2853 
13 57 
16.7 
16.5 
19.0 
17.0 
17-30 
45-3 
8.9466 
8.9819 
0.1689 
4- 0.42 
7.22 
II 2800 
13 58 
14.6 
14-5 
16.0 
4-5 
14.90 
44.6 
8.8203 
8.8540 
0.2968 
+ 0.74 
7-54 
II 2801 
13 59 
16.8 
17.0 
18.5 
15.0 
16.82 
44.0 
8.9229 
8.9552 
0.1956 
+ 0.49 
7.29 
19 2966 
14 1 
24-5 
24-5 
23.6 
23-5 
24.02 
36.0 
9.2193 
9-2375 
0.0867 
— 0.22 
6.58 
II 2780 
14 3 
24.2 
22.6 
26.9 
22.0 
23.92 
43-3 
9.2159 
9.2467 
9 3203 
14 5 
19-5 
16.4 
20.2 
19-5 
18.90 
50.8 
9.0209 
9.0716 
13 2946 
14 8 
12.5 
13.0 
I4.6 
12.9 
13-25 
41-3 
8.7204 
8.7472 
0.4036 
4- 1.01 
7.81 
13 2953 
14 9 
14-5 
14.6 
18.5 
15.6 
15.80 
41.8 
8.8700 
8.8977 
0.2531 
+ 0.63 
743 
12 2838 
14 12 
19.2 
17.8 
l8.6 
17.1 
18.18 
42.5 
8.9883 
9.0174 
0.1334 
4- 0.33 
7-13 
16 2789 
14 13 
24.0 
22.4 
25.O 
21.9 
23-32 
38.2 
9 -I 95 I 
9.2165 
0.0657 
— 0.16 
6.64 
16 2790 
14 14 
15.0 
15-5 
IÓ.O 
H -3 
15.20 
384 
8.8372 
8.8589 
0.2919 
4 0.73 
7-53 
19 2972 
14 16 
16.5 
16.5 
17-3 
15-8 
16.52 
36.1 
8.9077 
8.9260 
0.2248 
+ 0.56 
7-36 
11 2780 
14 17 
24.4 
21.5 
23.0 
20.6 
22.38 
42.5 
9.1613 
9.1904 
9 3203 
14 19 
20.0 
18.5 
21.4 
20.6 
20.12 
49-3 
9 - 073 I 
9.1192 
Mittel aus den Vergleichsternbeobachtungen: 9.1384; 9.1592; 9.1548. 
Zur Reduction benutzt: 9.1508.