195 Zone o° bis -f~ 20° Declination. 195 
11 
in 
Grösse 
- 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
IO° 
4351 
21 1 
‘48 m 
2 2?4 
2 I?4 
21 ?o 
i g?i 
20898 
448 o 
9-1079 
9.1402 
18 
4137 
21 
50 
1 7-i 
17-3 
18.5 
15.6 
17.12 
43-3 
8.9378 
8.9686 
0.1082 
4- 0.27 
7.07 
15 
3872 
21 
52 
18.7 
19.2 
19.9 
19.8 
19.40 
46.4 
9.O427 
9.0807 
0.0039 
— 0.01 
6.79 
6.89 
15 
3877 
21 
53 
14.2 
14.0 
15-3 
14-3 
1445 
46.3 
8-7943 
8.8321 
0.2447 
-|- 0.61 
7.41 
5 
14 
397° 
21 
56 
14.6 
13.6 
14.4 
12.4 
13-75 
47-7 
8.7520 
8-7935 
0.2833 
+ 0.71 
7-51 
6.44 
14 
3974 
2 1 
57 
20.6 
20.3 
20.6 
19.4 
20.22 
48.0 
9.0772 
9-”95 
0.0427 
O.I I 
6.69 
o 
7.02 
11 
39°6 
21 
59 
l8.6 
18.4 
18.0 
17.2 
18.05 
50.2 
8.9823 
9.03 n 
0.0457 
-f- 0.11 
6.91 
ö 
0.46 
10 
3981 
22 
0 
l8.6 
17.4 
18.8 
15-7 
17.62 
51.2 
8.9620 
9.0141 
0 
7-5° 
10 
4351 
22 
1 
I9.7 
20.4 
22.5 
21.0 
20.90 
45-o 
9-1047 
9-1393 
o 
7.84 
Mittel aus den Vergleichsternbeobachtunge 
n: 9.0672; 9.0864; 9.0767. 
Zur Reduction benutzt: 9.0768. 
Zone 175 
. 1887 October 26. 
o 
6.84 
Beobachter: Kempf. Photometer: D 
. Vergleichsterne: Nr. 42 und Nr. 44. Luft: 2 
— 3 - 
6 
7.00 
io‘ 
4351 
22} 
yin 
2389 
2385 
2385 
2 2?6 
23838 
4585 
9- I 97 2 
9.2330 
6 
7.00 
IO 
4604 
22 
10 
28.5 
27.4 
30.1 
27.9 
28.48 
42.6 
9-3567 
9.3860 
6 
7-30 
17 4478 
22 
12 
13.0 
13.0 
13.6 
11.8 
12.85 
38.2 
8.6943 
8-7157 
0.5798 
+ 1-45 
7-93 
6 
6.80 
16 
442 5 
22 
14 
l8.0 
20.3 
22.6 
20.5 
20.35 
39-2 
9.0826 
9.1056 
0.1899 
-1- 0.47 
6-95 
2 
7.96 
18 4668 
22 
15 
I7.4 
17.8 
18.i 
I 7* 1 
17.60 
37-6 
8.9611 
8.9816 
0.3139 
+ 0.78 
7.26 
19 
4590 
22 
17 
I 7.2 
16.0 
19.0 
15-5 
16.92 
36.5 
8.9279 
8.9468 
0.3487 
+ 0.87 
7-35 
11 
4457 
22 
19 
I 7.2 
15-5 
1 7-1 
15-5 
16.32 
44.4 
8.8974 
8.9306 
0.3649 
4- 0.91 
7-39 
> 36 . 
15 
43G 
22 
20 
l6.0 
18.9 
21.5 
19.0 
18.85 
40-3 
9.0187 
9.0436 
0.2519 
+ 0.63 
7 - 11 
IO 
4351 
22 
22 
23.O 
23.1 
23-1 
24.9 
23-52 
46.8 
9.2021 
9.2412 
IO 
4604 
22 
24 
26.8 
25-5 
26.9 
25.0 
26.05 
43- 1 
9-2853 
9-3I56 
14 4518 
22 
26 
27-5 
24-5 
304 
27.0 
27.32 
41.9 
9.3236 
9-35I5 
0.0560 
— 0.14 
6-34 
11 
4470 
22 
28 
13.0 
14.4 
15-5 
13.6 
14.12 
44.1 
8.7746 
8.8071 
0.4884 
+ 1.22 
7.70 
5-78 
A -»A 
18 4695 
22 
30 
14.0 
14.1 
15-5 
14.0 
14.40 
38.4 
8.7913 
8.8130 
0.4825 
-f- 1.21 
7.69 
0 
Q 
14 
4530 
22 
31 
20.6 
21.0 
23.0 
20.2 
2 1.20 
41-5 
9-ii65 
9.1436 
0.1519 
+ 0.38 
6.86 
O 
0.20 
15 
434° 
22 
33 
24.4 
26.8 
2 7-3 
26.4 
26.22 
41-3 
9.2905 
9-3I73 
0.0218 
— 0.05 
6-43 
2 
7.46 
18 
4719 
22 
34 
18.4 
18.2 
18.5 
20.0 
18.78 
37-8 
9-OI55 
9.0363 
0.2592 
+ 0.65 
7- I 3 
7 
7.21 
IO 
435 1 
22 
36 
25-5 
24.2 
24.1 
24.7 
24.62 
48.1 
9-2395 
9.282 1 
I 
5-73 
IO 
4604 
22 
38 
24.4 
254 
27-5 
26.6 
25.98 
43-9 
9.2831 
9 - 3 I 52 
2 
7-3 6 
Mittel aus den Vergleichsternbeobaclitungen: 9.3095; 9.2784; 9.2987. 
Zur Reduction benutzt: 9.2955 
Zone 176 
. 1887 October 26. 
5 
7.69 
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 42 und Nr. 44 
Luft: 2- 
- 3 - 
1 
7-25 
IO r 
4604 
22 1 
43 "’ 
2 4 ?6 
2383 
2587 
2387 
24832 
4481 
9.2295 
9.2620 
1 
7-95 
IO 
4351 
22 
46 
22.5 
19.8 
21-5 
19.4 
20.80 
49.2 
9.1007 
9.1465 
3 
6.87 
*) 1 9 
4638 
22 
47 
13-1 
114 
134 
12.2 
12.52 
38.4 
8.672 1 
8.6938 
O.5198 
-1- 1-3° 
7.78 
4 
7-58 
18 
4729 
22 
49 
8.6 
74 
9.2 
7-7 
8.22 
39-o 
8.3105 
8.3332 
O.8804 
+ 2.20 
8.68 
0 
7.64 
17 
4519 
22 
51 
15-4 
13.0 
134 
14.0 
13-95 
40.6 
8.7643 
8.7898 
O.4238 
+ I.06 
7-54 
16 
4475 
22 
53 
14.6 
14.6 
14.6 
134 
14.30 
4 r -5 
8.7854 
8.8125 
O.4OI I 
+ 1.00 
7.48 
15 
4375 
22 
55 
22.0 
22.8 
25-3 
22.7 
23.20 
42.5 
9.1909 
9.2200 
O.O064 
0.02 
6.46 
72. 
11 
4502 
22 
56 
18.5 
154 
17.2 
14-3 
16.35 
46.6 
8.8990 
8.9376 
O.2760 
4- 0.69 
7- 1 7 - 
10 
4351 
22 
58 
21.5 
19.7 
20.5 
19-5 
20.30 
50-5 
9.0805 
9- I 3°3 
10 
4604 
22 
59 
25-7 
24-3 
25-7 
24.2 
24.98 
45-2 
9.2512 
9.2863 
17 
4528 
2 3 
2 
10.3 
10.5 
10.3 
10.4 
10.38 
41.6 
8.5113 
8.5386 
O.6750 
4- 1-69 
8.17 
18 
4743 
23 
4 
11 .7 
9.6 
11-3 
10.4 
10.75 
40.8 
8.5415 
8.5673 
O.6463 
+ I.Ó2 
8.10 
15 
4379 
23 
5 
17.7 
15-7 
16.0 
16.5 
16.48 
42.9 
8.9057 
8.9356 
O.2780 
4- 0.70 
7.18 
1 
7.84 
i6 
4486 
23 
7 
18.7 
16.3 
18.3 
16.0 
I7-32 
42.7 
8.9476 
8-977 1 
O.2365 
4- 0.59 
7.07 
) 
7.20 
10 
4498 
23 
8 
15.0 
i3*5 
14.1 
13.0 
13.90 
47-7 
8.7612 
8.8027 
O.4109 
4- 1-03 
7-51 
8.48 
10 
4499 
23 
9 
15-3 
13.6 
154 
13.0 
14-32 
48.4 
8.7866 
8.8301 
0.3835 
-f- 0.96 
7-44 
7-44 
10 
43 5 1 
23 
11 
23-3 
20.7 
234 
194 
21.70 
52.0 
9-1358 
9- I 9°7 
7-50 
10 
4604 
23 
I 3 
25.6 
22.5 
26.4 
22.6 
24.28 1 46.3 
9.2281 
9.2659 
1 
7.27 
Mittel aus den 
Vergleichsternbeobachtungen: 9.2043 
; 9.2083; 9.2283. Zur Reduction benutzt: 9.2136. 
*) 19 0 
4638 dupl. Als ein 
Stern gemessen.