198 
199 
Zone o° bis -f- 20 0 Declination. 
199 
Grösse 
6.70 
7-75 
7.24 
6.38 
7.89 
7-45 
8.06 
7.40 
7.16 
6 - 93 
5-93 
7 - 03 
5-83 
6.27 
6.96 
7-55 
7.18 
6.24 
6 - 43 
7.21 
7.84 
6.72 
6.83 
7 - 3 2 
6.83 
; 7-38 
7.41 
1 6.98 
) 7.16 
• 6.55 
13 .D. 
Sternzeit 
1 
II 
III 
IV 
/ 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
IO c 
4351 
2 1 1 
3 8 m 
2 Ó ( . , 2 
2 4 ( -4 
2582 
2385 
24882 
4384 
9.2460 
9.2770 
14 
4293 
21 
40 
18.2 
18.0 
18.8 
16.0 
17-75 
40.9 
8.9682 
8.9942 
0.2267 
+ 0-57 
7-37 
19 4408 
21 
41 
22.7 
25.6 
26.4 
25-5 
25-05 
364 
9-2535 
9.2723 
0.0514 
— 0.13 
6.67 
19 
4419 
21 
42 
2O.9 
19.0 
20.6 
19.7 
20.05 
36.1 
9.0702 
9.0885 
0.1324 
+ 0.33 
7-13 
16 
4259 
21 
44 
25.8 
26.0 
27.0 
26.9 
26.42 
39 -o 
9.2966 
9 - 3 I 93 
0.0984 
— 0.25 
6-55 
18 
4505 
21 
45 
I9.O 
21.0 
21.2 
20.9 
20.52 
37-6 
9.0895 
9.1IOO 
0.1109 
4~ 0.28 
7.08 
12 
4348 , 
21 
47 
20.8 
19-5 
19.0 
19.8 
19.78 
43-4 
9.0589 
9.0899 
0.1310 
+ 0.33 
7-13 
10 
3981 
21 
50 
21.0 
19.0 
21.1 
22.7 
20.95 
50.0 
9.1067 
9-1549 
10 
4351 
21 
52 
24.O 
22.7 
27.2 
25.2 
24.78 
44-3 
9.2447 
9.2777 
Mittel aus den Vergleichsternbeobachtungen: 9.2394; 9.2071; 9.2163. Zur Reduction benutzt: 9.2209. 
Zone 185. 
1887 November 17. 
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 1 
—2. 
IO C 
4351 
2 I 1 
5 6 m 
2I?3 
20?3 
22?4 
21?6 
21840 
4486 
9- I2 43 
9.1580 
IO 
3981 
21 
59 
19-3 
l6.6 
l8.6 
16.4 
17.72 
5 1-1 
8.9668 
9.0185 
15 
4171 
22 
1 
12.4 
I2.3 
14-3 
13-4 
13.10 
41.2 
8.7107 
8-7373 
0.3382 
+ 0.85 
7-65 
15 
4181 
22 
2 
17.6 
16.O 
19.0 
17. 1 
17.42 
41.6 
8.9525 
8.9798 
0.0957 
4- 0.24 
7.04 
19 
4423 
22 
4 
I9.8 
18.7 
19.6 
19.6 
19.42 
38.0 
9.0436 
9.0647 
0.0108 
+ 0.03 
6.83 
19 4426 
22 
5 
IÓ .2 
16.5 
17.7 
16.3 
16.68 
384 
8.9159 
8.9376 
0.1379 
+ 0-34 
7.14 
18 
4517 
22 
7 
18.9 
18.7 
18.3 
17.0 
18.22 
38.8 
8.9901 
9.0125 
0.0630 
+ 0.16 
6.96 
4307 { 
22 
9 
14-5 
11*4 
13-4 
12.3 
12.90 
464 
8.6976 
8.7356 
0.3399 
+ 0.85 
7-65 
)lO 
22 
10 
17.2 
14.7 
16.6 
12.4 
15.22 
46.5 
8.8383 
8.8766 
0.1989 
+ 0.50 
7-30 
IO 
4351 
22 
12 
20.8 
20.3 
22.4 
21.4 
21.22 
45-9 
9- 11 73 
9 -I 54 I 
IO 
398 i 
22 
14 
19.0 
15-5 
18.1 
16.5 
17.28 
52-9 
8.9456 
9.0038 
16 4288 
22 
17 
17.0 
14-3 
15.8 
134 
15.12 
41.9 
8.8327 
8.8606 
0.2 I49 
+ 0-54 
7-34 
16 
4291 
22 
18 
16.9 
1 5-1 
15-7 
1 5-6 
15.82 
42.0 
8.8711 
8.8992 
O.I763 
+ 0.44 
7.24 
15 
4185 
22 
20 
1 1*5 
1 1*3 
ii -3 
10.9 
11.25 
43 - 1 
8.5805 
8.6108 
O.4647 
+ 1.16 
7.96 
15 
4187 
22 
21 
12.4 
1 1-7 
12.9 
10.7 
11.92 
43-2 
8.6300 
8.6605 
O.4150 
+ 1-04 
7.84 
18 
4525 
22 
22 
15.0 
14.0 
14.6 
14-3 
14.48 
40.8 
8.7960 
8.8218 
0.2537 
+ 0.63 
7-43 
17 
4355 
22 
24 
17.4 
16.0 
19.0 
16.6 
17-25 
41-3 
8.9442 
8.9710 
O.IO45 
+ 0.26 
7.06 
12 
4378 
22 
25 
33-4 
33 -o 
32-3 
32.7 
32-85 
46.0 
9.4687 
9-5057 
O.4302 
— 1.08 
5-72 
IO 
398 i 
22 
28 
18.5 
16.7 
18.1 
15.6 
17.22 
54-6 
8.9427 
9.0077 
IO 
4351 
22 
30 
21.4 
20.0 
19.8 
19.0 
20.05 
47-5 
9.0702 
9.1111 
Mittel aus den Vergleichsternbeobachtungen: 9.0883; 9.0789; 9.0594. Zur Reduction benutzt: 9.0755. 
*) IO° 
4307 dupl. Zuerst die vorangehende Componente gemessen. 
Zone 
186. 
1887 November 
17 - 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 2 und Nr. 4. 
Luft: I- 
-2. 
9 ' 
47 
22} 
39 m 
29?0 
2 8? 1 
3082 
2783 
28865 
4787 
9 - 36 i 5 
9.4030 
10 
168 
22 
42 
17-5 
17.6 
19-3 
18.3 
18.18 
51.6 
8.9883 
9.0418 
15 
69 
22 
45 
19.0 
18.6 
19-3 
18.5 
18.85 
41.9 
9.0187 
9.0466 
O.I979 
4-0.49 
7.18 
15 
73 
22 
46 
20.5 
20.0 
21.0 
19.8 
20.32 
41.9 
9.0813 
9.1092 
0.1353 
4-0.34 
7-03 
15 
74 
22 
47 
17.2 
17.0 
l8.8 
18.0 
17-75 
41.8 
8.9682 
8-9959 
O.2486 
4- 0.62 
7-31 
IO 
57 
22 
49 
18.5 
17.6 
18.5 
16.0 
17-65 
45-9 
8.9635 
9.0003 
O.2442 
4- 0.61 
7-30 
12 
47 
22 
5 1 
18.4 
15.6 
I 7.6 
17.4 
17-25 
44.4 
8.9442 
8.9774 
O.2671 
4- 0.67 
7-36 
l8 
67 
22 
52 
18.4 
19.0 
21.5 
20.3 
19.80 
38.1 
9-0597 
9.0810 
O.1635 
4" 0.41 
7.10 
9 
47 
22 
54 
33-3 
32.5 
30.0 
28.1 
30.98 
46.5 
9.4232 
9.4615 
IO 
168 
22 
56 
18.0 
19.4 
20.4 
17-5 
18.82 
49.9 
9 -OI 73 
9.0652 
17 
67 
22 
58 
2 1.6 
22.6 
22.0 
21.8 
22.00 
38-4 
9.1472 
9.1689 
O.0756 
4-0.19 
6.88 
13 
69 
23 
0 
14.0 
14.1 
15.O 
13.0 
14.02 
42.8 
8.7686 
8.7983 
O.4462 
4- 1.12 
7.81 
13 
73 
23 
2 
12,5 
16.0 
13.8 
13.2 
13.88 
42.1 
8.7600 
8.7883 
O.4562 
+1.14 
7-83 
19 
83 
23 
3 
15.0 
14.0 
15.6 
13-7 
14.58 
36.5 
8.8018 
8.8207 
O.4238 
4- i .06 
7-75 
I 2 
57 
23 
5 
24.9 
25.0 
25.8 
24-5 
25-05 
43 -o 
9-2535 
9.2836 
O.O391 
— 0.10 
6-59 
I 2 
59 
23 
7 
26.2 
24.9 
20.8 
24.4 
25.58 
43 -i 
9.2705 
9.3008 
O.O563 
— 0.14 
6-55 
9 
47 
23 
9 
29.2 
27.0 
20.8 
28.0 
27-75 
45-4 
9 - 336 i 
9 - 37 I 7 
IO 
168 
23 
11 
20.4 
19.6 
22.0 
19.2 
20.30 
48-3 
9.0805 
9 - 1 23 7 
Mittel aus den Vergleichsternbeobachtungen: 9.2224; 9.2634; 9.2477. 
Zur Reduction benutzt: 9.2445. 
25*