140 
141 
Zone o° bis -f- 20° Declination. 
141 
Pubi, des Astrophys. Obs. zu Potsdam. Bd. IX. 
18 
Grösse 
7.66 
7-30 
7.22 
7-54 
7-3 2 
7-31 
6.74 
7-83 
7.42 
7.06 
6.76 
6.18 
7-49 
6.76 
6.69 
6 - 57 
7 - 54 
7-50 
6.77 
6.51 
7.14 
6.46 
6.01 
6.32 
7-57 
7-83 
6.13 
6.77 
7-33 
6.30 
B.D. 
Sternzeit 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
9 ° 
5277 
i 1 
3 1 m 
1985 
20? 2 
20?7 
20?4 
20° 20 
4884 
9.0764 
9.H99 
14 4866 
1 
35 
13.0 
114 
13-7 
11-7 
I245 
51-2 
8.6673 
8.7194 
0.3757 
+ O.94 
7.70 
13 4989 
1 
37 
19.2 
16.0 
17.9 
16.5 
I7.4O 
52.1 
8.9515 
9.0068 
0.0883 
-b 0.22 
6.98 
18 
5059 
1 
39 
21.2 
18.4 
19.0 
18.0 
I 9 -I 5 
47.8 
9.0319 
9-0737 
0.0214 
4- 0.05 
6.81 
17 4818 
1 
41 
14.0 
12.4 
13.0 
12.4 
12.95 
49.0 
8.7009 
8.7461 
0.3490 
+ O.87 
7-63 
14 4879 
1 
43 
16.4 
15.0 
15.0 
13.6 
15.00 
51.6 
8.8260 
8.8795 
0.2 I 56 
+ 0.54 
7-30 
19 
5028 
1 
45 
17.0 
14.6 
1 5 - 1 
16.4 
I 5-78 
47-5 
8.8689 
8.9098 
O.1853 
+ O.46 
7.22 
9 
51 11 
1 
47 
20.0 
17.2 
20.1 
18.9 
I9.O5 
56.3 
9.0275 
9.1000 
9 
5277 
1 
50 
19.4 
19.0 
21.2 
18.0 
I9.4O 
50-3 
9.0427 
9.0919 
Mittel aus den Vergleichsternbeobachtunge 
n: 9.0807; 9.1087; 9.0959. 
Zur Reduction benutzt: 9.0951. 
Zone 
39 - 
l886 
November 23. 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 4 und Nr. 6. 
Luft: I- 
-2. 
IO° 
168 
2 1 
56 m 
I 1980 
1780 
2 2?0 
i 8?5 
19 V12 
4682 
9.0306 
9.0681 
8 
385 
2 
58 
27-3 
25-5 
30.5 
27.6 
27.72 
43-9 
9-3352 
9.3673 
6.91 
7 
362 
3 
1 
20.5 
19.0 
22.9 
19.4 
20.45 
45-8 
9.0867 
9.1232 
O.O905 
4- 0.23 
7 
371 
3 
3 
17.4 
17.4 
18.9 
17.6 
17.82 
46.1 
8.9715 
9.0088 
O.2049 
4- 0.51 
7.19 
9 
319 
3 
5 
1 4-9 
14-5 
18.O 
15.6 
15-75 
43-3 
8.8674 
8.8982 
0.3155 
4-0.79 
7-47 
9 
321 
3 
6 
21.9 
18.2 
2 1.0 
19-5 
20.15 
43-3 
9.0744 
9.1052 
O.IO85 
4- 0.27 
6-95 
9 
323 
3 
8 
21.4 
21.5 
2 6.0 
21.9 
22.70 
43-7 
9-1730 
9.2046 
O.OO91 
—b 0.02 
6.70 
5 
338 
3 
10 
19.0 
18.4 
23.O 
19.4 
19-95 
47-7 
9.0660 
9 * 1 °7 5 
O.IOÓ 2 
4- 0.27 
6-95 
10 
168 
3 
12 
17.6 
19-5 
23-5 
18.5 
19.78 
47-7 
9.0589 
9.1004 
8 
385 
3 
14 
2 6.8 
27.9 
27.O 
29.9 
27.90 
44-5 
9.3404 
9-3738 
O.O378 
6-59 
1 
431 
3 
15 
22.4 
22.2 
27.O 
21.8 
23-35 
52.1 
9.1962 
9 - 25 I 5 
— 0.09 
4 I 5 { 
3 
18 
ii -4 
13.0 
13.8 
11*9 
12.52 
52.9 
8.6721 
8.7303 
0.4834 
+1.21 
7.89 
) 0 
3 
20 
14.0 
12.5 
I4.O 
12.8 
13-32 
53-0 
8.7249 
8.7835 
O.4302 
~b i .08 
7.76 
0 
421 
3 
21 
14.4 
14-5 
15-5 
14-5 
14.72 
53 -i 
8.8100 
8.8690 
0.3447 
4- 0.86 
7-54 
6 
392 
3 
23 
26.0 
244 
28.2 
28.4 
26.75 
46.7 
9.3066 
9-3454 
O.I 3 I 7 
— 0.33 
6-35 
6 
398 
3 
26 
28.5 
29.4 
29.0 
28.4 
28.82 
47-5 
9.3662 
9.4071 
O.1934 
— 0.48 
6.20 
7 
402 
3 
27 
28.5 
28.0 
26.4 
31-9 
28.70 
46.6 
9.3629 
9.4015 
O.1878 
— 0.47 
6.21 
10 
168 
3 
29 
19.0 
17.0 
21.4 
19.1 
19.12 
49.4 
9.0306 
9.0770 
8 
385 
3 
32 
24.2 
24.2 
25.1 
27-5 
25-25 
45-5 
9.2600 
9.2958 
Mittel aus den Vergleichsternbeobachtungen: 9.2177; 9.2371; 9.1864. Zur I^eduction benutzt: 9.2137. 
*) o°4i5 dupl. Zuerst die vorangehende Componente gemessen. 
Zone 
40. 
1886 
November 23. 
Beobachter: Müller. 
Photometer: D. Vergleichsterne: Nr. 6 und Nr. 8. 
Luft: 2— 
- 3 - 
8° 
385 
3 h 
37 m 
2 6?4 
2I?5 
2.6?0 
2I?7 
23890 
4589 
9.2152 
9.2520 
9 
472 
3 
41 
14.2 
12.0 
14.2 
13-3 
13.42 
42.7 
8.7313 
8.7608 
7 
405 
3 
43 
19.8 
21.3 
18.6 
17.8 
19.38 
47-4 
9.0418 
9.0825 
0.1103 
— 0.28 
6.58 
2 
406 
3 
45 
234 
19-3 
22 .7 
23.6 
22.25 
51-7 
9-1565 
9.2103 
O.2381 
— 0.60 
6.26 
3 
373 
3 
47 
15-7 
IÓ.O 
15-5 
15.0 
15-55 
50.7 
8.8565 
8.9069 
O.0653 
4-0.16 
7.02 
5 
374 
3 
49 
22.4 
21-5 
20.4 
19-5 
20.95 
49.2 
9.1067 
9 -I 525 
O.1803 
— 0.45 
6.41 
5 
377 
3 
51 
16.0 
154 
154 
15-5 
15-58 
49-3 
8.8581 
8.9042 
O.0680 
4 - 0.17 
7-03 
9 
353 
3 
52 
18.8 
18.O 
20.2 
17.4 
18.60 
45 -o 
9.0075 
9.0421 
O.0699 
— 0.17 
6.69 
4 
437 
3 
54 
21.4 
21.3 
20.0 
20.4 
20.78 
50.6 
9.0999 
9.1500 
0.1778 
— 0.44 
6.42 
8 
385 
3 
56 
22.6 
21.5 
22.3 
2 x.o 
21.85 
47.2 
9-1415 
9.1816 
9 
472 
3 
59 
12.4 
13-3 
15.0 
13.6 
13-58 
42.9 
8.7414 
8.7713 
8 
424 
4 
1 
ii -5 
I 1.0 
II.8 
11.4 
11.42 
46.5 
8.5933 
8.6316 
0.3406 
4 - 0.85 
7.71 
0 
469 
4 
3 
12.0 
12.5 
IÓ.O 
134 
13.48 
54-5 
8.7351 
8.7997 
0.1725 
4-0.43 
7.29 
1 
503 
4 
6 
14.6 
134 
I 7.0 
14.0 
14-75 
53-4 
8.8117 
8.8719 
0.1003 
4- 0.25 
7.n 
1 
509 
4 
7 
134 
14-5 
15.0 
1 5 *6 
14.62 
53-5 
8.8042 
8.8647 
0.1075 
4- 0.27 
7-13 
8 
443 
4 
9 
17.4 
16.7 
19-3 
17.8 
17.80 
46.5 
8.9706 
9.0089 
0.0367 
— 0.09 
6-77 
2 
450 
4 
10 
15.6 
14.7 
14-5 
16.0 
15.20 
52.1 
8.8372 
8.8925 
0.0797 
4- 0.20 
7.06 
8 
385 
4 
12 
21-5 
21.0 
22.4 
21.5 
21.60 
48.6 
9.1320 
9.1760 
9 
472 
4 
H 
12.8 
10.5 
134 
12.7 
12.35 
43-4 
8.6604 
8.6914 
Mittel aus den Vergleichsternbeobachtunge 
n: 9.0064; 8.9765; 8.9337. Zur Reduction benutzt: 8.9722.