187 
Zone o° bis -4- 20 0 Declination. 
187 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
ii°2 4 85 
11 1 ' 49 m 
2 2?3 
22?I 
2I?4 
2 I?6 
21885 
4286 
9*1415 
9.1708 
4 2604 
11 50 
21.3 
I9.2 
22.9 
I9.7 
20.78 
48.8 
9.0999 
9.1445 
0.1 I 2 I 
— 0.28 
5-17 
18 2592 
11 52 
23.6 
23-5 
24.9 
24.4 
24.10 
34-3 
9.2220 
9.2380 
O.2056 
— 0.51 
4.94 
*)ig 2584 
ii 54 
234 
23-7 
23.6 
20.7 
22.85 
34 -i 
9.1784 
9 .I 94 I 
O.IÓI 7 
— 0.40 
5-05 
17 2504 
ii 56 
14.8 
154 
15-9 
I4.6 
15.18 
354 
8.8361 
8.8535 
0.1789 
+ 0.45 
5-90 
17 2 533 
ii 5 8 
20.3 
18.5 
20.0 
18.9 
19.42 
36.2 
9.0436 
9.0621 
O.O297 
— 0.07 
5-38 
14 2549 
12 0 
I4.O 
13-5 
15.0 
15-4 
14.48 
38.6 
8.7960 
8.8181 
O.2143 
+ O.54 
5-99 
9 2560 
12 2 
I 7.2 
14.0 
16.3 
14-5 
15-50 
434 
8.8538 
8.8848 
11 2485 
12 3 
22.9 
20.0 
22.6 
24.8 
22.58 
42.0 
9.1686 
9.1967 
Mittel aus den Vergleichsternbeobachtungen: 9.0262; 9.0304; 9.0407. 
Zur Reduction benutzt: 9.0324. 
*) 1902584 dupl. Gemessen die hellere, 
folgende Componente. 
Zone 155. 1887 Mai 14. 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 26 und Nr. 28. Luft: 2 
- 3 - 
11°2440 
13 5 l m 
31-5 
31-5 
34 ?° 
35 -i 
33?02 
4685 
9.4727 
9 - 5 IIO 
9 2798 
13 54 
27.I 
30.3 
28.9 
27.1 
28-35 
43-5 
9.3531 
94843 
8 2617 
13 56 
I9.O 
18.2 
20.7 
19-5 
19-35 
47.6 
9.0406 
9.0818 
o -3493 
4 " 0.87 
7.12 
8 2619 
13 5 8 
2I.9 
20.9 
23.0 
22.0 
21.95 
47.6 
9.1453 
9.1865 
0.2446 
+ O.61 
6.86 
9 2648 
14 0 
23.O 
22.9 
24.2 
244 
23.62 
46.6 
. 9.2056 
9.2442 
0.1869 
4~ O.47 
6.72 
5 2654 
14 '2 
18.3 
21.5 
19-5 
19.0 
19.58 
51.0 
9.0504 
9.1018 
0.3293 
*4“ 0.82 
7.07 
4 2631 
14 4 
23-5 
25.0 
27-5 
23.0 
24-75 
52.1 
9.2438 
9.2991 
0.1320 
+ 0.33 
6.58 
2 2560 
14 6 
36.0 
37 -o 
42-5 
38.0 
38.38 
53-5 
9.5860 
9.6465 
0.2154 
— 0.54 
5-71 
11 2440 
14 IO 
28.6 
33 -o 
31-9 
32.9 
31.6° 
484 
9.4386 
9.4818 
9 2798 
14 12 
24.8 
27.7 
26.5 
29.6 
27 .I 5 
44.0 
9.3186 
9-3509 
7 2568 
14 14 
36.6 
31-5 
39-5 
37 -o 
36.15 
49-2 
9.5416 
94874 
0.1563 
— 0.39 
5.86 
8 2639 
14 l8 
40.5 
38.1 
474 
45 -i 
42.78 
48.3 
9.6640 
9.7072 
0.2761 
— 0.69 
5-56 
6 2660 
14 21 
24-5 
22.5 
28.6 
25.6 
25-30 
50.2 
9.2616 
9.3104 
0.1207 
+ 0.30 
6-55 
4 2653 
14 24 
24.4 
22.1 
26.4 
28.4 
2542 
52.6 
9.2622 
94193 
0.1118 
4- 0.28 
6-53 
3 2703 
14 2Ó 
30.6 
304 
354 
33-6 
32.50 
52.9 
9.4604 
9.5186 
0.0875 
— 0.22 
6.03 
0 3002 
14 28 
23.0 
21.0 
21.6 
20.5 
21.52 
55-6 
9.1290 
9.1983 
0.2328 
4 ~ 0.58 
6.83 
11 2440 
14 30 
28.3 
29.4 
36.5 
31.6 
3145 
504 
94350 
9.4845 
9 2798 
14 32 
27.6 
27.4 
29.0 
27-5 
27.88 
44.8 
9.3398 
9-3739 
Mittel aus den Vergleichsternbeobachtungen: 9.4477; 9.4163; 9.4292. 
Zur Reduction benutzt: 9.4311. 
t 
Zone 156. 1887 Juni 4. 
Beobachter: Kempf. 
Photometer: D. Vergleich sterne : Nr. 30 
und Nr. 32. Luft: 
3 - 
8° 2 85 7 
i 5 h 57 m 
3284 
3 8?i 
34-0 
3280 
348 i 2 
4880 
9.4978 
94401 
II 2780 
16 1 
22.4 
24.0 
25-5 
27.0 
24.72 
42.7 
9.2428 
9.2723 
2 2881 
16 6 
20.0 
20.7 
22.3 
21.1 
2 1.02 
52.3 
9.1095 
9.1655 
0.1988 
+ 0.50 
6-95 
6 2957 
16 8 
24.1 
24.0 
23-5 
21.6 
23-3° 
48.6 
9.1944 
9.2384 
0.1259 
4- 0.31 
6.76 
7 2865 
IÓ 10 
22.0 
22.5 
24.6 
20.6 
22.42 
48.0 
9.1627 
9.2050 
0.1593 
+ 0.40 
6.85 
3 2956 
16 12 
18.2 
16.6 
20.5 
18.0 
18.32 
514 
8.9947 
9.0471 
0.3172 
+ 0.79 
7.24 
0 3277 
16 14 
40.0 
39-2 
41.8 
42.2 
40.80 
54-8 
9.6304 
9.6962 
0.3319 
— 0.83 
5.62 
5 2954 
16 16 
37 -o 
33-5 
37-6 
324 
35-12 
50.3 
9.5197 
9.5688 
0.2045 
— 0.51 
5-94 
8 2857 
16 20 
304 
28.5 
28.0 
26.9 
28.45 
50.2 
9.3559 
9.4047 
11 2780 
16 23 
22.4 
23-7 
24.0 
22.5 
23-15 
44.0 
9.1891 
9.22 14 
8 2955 
16 27 
19.6 
19.1 
19.7 
21-5 
19.98 
48.1 
9.0673 
9.1099 
0.2544 
4- 0.64 
7.09 
3 2966 
16 29 
20.0 
19-3 
20.1 
20.5 
19.98 
52.8 
9.0673 
9 .I 25 I 
0.2392 
4- 0.60 
7-°5 
0 3297 
16 31 
44-5 
3 8 -3 
42.1 
40.0 
41.22 
55-7 
9.6377 
9.7075 
0.3432 
— 0.86 
5-59 
5 2962 
16 33 
144 
13-5 
14.8 
13.6 
14.08 
51.0 
8.7722 
8.8236 
0.5407 
4 - i -35 
7.80 
16 35 
15.0 
15.6 
15-5 
14-5 
15-15 
50.5 
8.8344 
8.8842 
0.4801 
4- 1.20 
7.65 
j 0 2903 < 
16 37 
15.6 
12.8 
15.8 
134 
14.40 
50.7 
8-7913 
8.841 7 
0.5226 
4 - 1.31 
7.76 
4 2964 
16 39 
14.0 
14.4 
16.5 
16.0 
15.22 
51-9 
8.8383 
8.8928 
0.4715 
4- i . 18 
7.63 
8 2857 
16 42 
30.0 
29.0 
33 -o 
32.0 
31.00 
52-5 
9.4237 
9.4804 
11 2780 
16 44 
25.0 
23.6 
23.8 
25.0 
24-35 
45-7 
9.2305 
9.2668 
Mittel aus den 
Versleichsternbeobachtungen: 9.4062; 9.3131; 9 - 3736 . 
Zur Reduction benutzt: 9.3643. 
*) 6° 2983 dupl. 
Zuerst die nördlich vorangehende Componente gemessen. Messung unsicher.