Zone o° bis -f~ 20 ° Declination. 
167 
166 
167 
Grösse 
6.24 
7.61 
7-50 
7.64 
7.04 
6.4} 
6.61 
7.40 
6-55 
6-34 
7.41 
7.46 
749 
6.78 
6.29 
6.52 
6.76 
7- 2 3 
7-38 
744 
7. 11 
7- 2 5 
7 - 5 2 
6.77 
6.78 
6-55 
6.28 
7.04 
6.76 
7.62 
6.48 
7.68 
B.D. 
Sternzeit 
I 
II 
III 
IV 
/ 
2 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
10° 
1818 
7I1 4 gm 
20?5 
2I?3 
2I?5 
20?5 
20895 
4286 
9.1067 
9.1360 
9 
2239 
7 
50 
16.2 
I 7.2 
18.2 
17-5 
17.28 
48.8 
8.9456 
8.9902 
6 2087 
7 
53 
24-5 
24.O 
27-5 
28.0 
26.00 
48.1 
9.2837 
9.3263 
0.2743 
— O.69 
6.26 
3 
2124 
7 
55 
15.0 
15.0 
17.9 
16.5 
16.10 
50.9 
8.8859 
8.9370 
0.1150 
4- O.29 
7.24 
0 
2 449 
7 
56 
28.1 
29.7 
35-6 
36.0 
32.35 
53-9 
9.4569 
9.5190 
0.4670 
— I - 1 7 
5-78 
7 
2066 
7 
58 
28.1 
33-5 
34-5 
31.0 
31-78 
46.2 
9.4430 
9.4805 
0.4285 
— 1.07 
5-88 
7 
2068 
7 
59 
21.7 
20.4 
22.5 
234 
22.00 
46.6 
9.1472 
9-!858 
0.1338 
— 0.33 
6.62 
2 
2138 
8 
1 
12.2 
134 
154 
13-5 
13.62 
50.9 
8-7439 
8.7950 
0.2570 
—f- 0.64 
7-59 
10 
1818 
8 
3 
21.5 
20.0 
24.0 
20.1 
21.40 
42.2 
9- I2 43 
9 - i 5 2 8 
9 
2239 
8 
5 
15-7 
15.0 
16.3 
15.6 
15-65 
47-5 
8.8620 
8.9029 
Mittel aus (len Vergleichsternbeobachtungen: 9.0652; 9.0631; 9.0278. 
Zur Reduction benutzt: 9.0520. 
Zone 105. 1887 März 1. 
Beobachter: Müller. 
Photometer: D. Vergleichsterne: Nr. 22 
und Nr. 24. Luft: 3. 
9 C 
2374 
9 h 48 ,n 
22?2 
2 2?4 
2483 
2I?7 
22865 
4480 
9.1712 
9.2035 
11 
2372 
9 
51 
I4.7 
15.0 
16.6 
15.0 
15-32 
45 -i 
8.8439 
8.8787 
9 
53 
15.6 
14.O 
16.4 
i 3-7 
14.92 
52.2 
8.8214 
8.8770 
0.1761 
+ 0-44 
6.84 
; j 
9 
54 
9-7 
7.0 
9-3 
8-3 
8.58 
52.1 
8-3475 
8.4028 
0.6503 
+ 1.63 
8.03 
8 
2512 
9 
56 
15-4 
13.O 
15.6 
14.2 
14-55 
47-7 
8.8001 
8.8416 
0.2115 
+ 0-53 
6-93 
3 
2519 
9 
58 
16.6 
15-5 
17.1 
17.7 
16.72 
52-7 
8 - 9 i 79 
8-9754 
0.0777 
-f- 0.19 
6-59 
3 
2521 
9 
59 
22.2 
20.4 
23.6 
21.0 
21.80 
52.2 
9.1396 
9.1952 
0.1421 
— 0.36 
6.04 
4 
2501 
10 
0 
13.0 
11.0 
144 
ii-3 
12.42 
52.0 
8.6652 
8.7201 
0.3330 
+ 0.83 
7-23 
9 
2374 
10 
2 
22.4 
22.7 
234 
21.7 
22.55 
43-5 
9-1675 
9.1987 
11 
2372 
10 
4 
15-7 
154 
17-3 
14.7 
I 5-78 
44.1 
8.8689 
8.9014 
6 
2470 
10 
5 
16.4 
12.7 
14.0 
13-3 
14.10 
49.0 
8-7734 
8.8186 
0.2345 
+ 0.59 
6.99 
7 2 405 
10 
7 
12.6 
114 
13.6 
10.6 
12.05 
48.7 
8.6394 
8.6837 
0.3694 
+ 0.92 
7-32 
9 
2523 
10 
8 
20.0 
18.0 
20.2 
18.5 
19.18 
46.2 
9-0331 
9.0706 
0.0175 
— 0.04 
6.36 
8 
2532 
10 
9 
31-3 
28.5 
29.8 
28.5 
29.52 
46.9 
9-3852 
9.4245 
0.3714 
— 0-93 
5-47 
0 
2821 
10 
11 
11.6 
10.4 
13.2 
10.2 
ii -35 
55-3 
8.5881 
8.6561 
0.3970 
+ 0.99 
7-39 
1 
2597 
10 
13 
13.0 
11.4 
13-7 
ii *7 
12.45 
53-6 
8.6673 
8.7282 
0.3249 
+ 0.81 
7.21 
3 
2539 
10 
14 
12.7 
12.3 
13-7 
12.1 
12.70 
52.3 
8.6842 
8.7402 
0.3129 
+ 0.78 
7.18 
11 
2372 
10 
16 
16.0 
14.8 
16.4 
16.3 
15.88 
43-2 
8.8743 
8.9048 
9 
2374 
10 
18 
25.0 
23-5 
22.7 
22.7 
23.48 
43-2 
9.2007 
9 - 2 3 12 
Mittel aus den Vergleiehsternbeobachtungen: 9.0411; 9.0501; 9.0680. 
Zur Reduction benutzt: 9.0531. 
) Ò 
2502 dupl. Die hellere, nördlich vorangehende Componente zuerst gemessen. 
Zone 106. 1887 März 8. 
Beobachter: Kempf. 
Photometer : 
D. Vergleichsterne: Nr. 10 imd Nr. 
12. Luft: 
3 - 
li' 
632 
6 1 32 ln 
17?6 
17?8 
190 
i 8?4 
18832 
4789 
8.9947 
9.0367 
10 
818 
6 
34 
28.0 
32.4 
354 
33-5 
32-32 
44.2 
9.4562 
9.4890 
16 
625 
6 
36 
17.1 
18.2 
20.0 
18.4 
18.42 
43-3 
8.9993 
9.0301 
O.2235 
+ O.56 
7.01 
19 
740 
6 
38 
16.0 
15.6 
16.0 
14.7 
I 5-58 
41.2 
8.8581 
8.8847 
0.3689 
+ O.92 
7-37 
19 
742 
6 
39 
20.6 
20.4 
22.9 
21.3 
21.30 
41-3 
9.1204 
9.1472 
0.1064 
+ O.27 
6.72 
15 
656 
6 
41 
21.0 
18.4 
22.1 
18.8 
20.08 
45 -o 
9-0715 
9.1061 
0.1475 
+ 0-37 
6.8 2 
14 
726 
6 
42 
14.4 
14.1 
16.3 
13.0 
H -45 
45-6 
8-7943 
8.8303 
O.4233 
1.06 
7-51 
15 
661 
6 
44 
2 7-5 
28.9 
27.0 
27.1 
27.62 
44.9 
9-3323 
9.3667 
O. I 1 3 I 
— 0.28 
6.17 
11 
632 
6 
46 
20.0 
18.9 
194 
19.1 
19-35 
49.4 
9.0406 
9.0870 
10 
818 
6 
48 
28.6 
31.0 
29-5 
27-5 
29.15 
45 -i 
9-3753 
9.4101 
18 
661 
6 
50 
20.6 
18.0 
21.6 
19.0 
19.80 
43-5 
9-0597 
9.0909 
O.1627 
—|— O.Z}- I 
6.86 
12 
620 
6 
51 
15.0 
14.0 
15-3 
14.0 
14.58 
48.3 
8.8018 
8.8450 
0.4086 
+ 1.02 
7-47 
11 
639 
6 
53 
28.6 
32.2 
314 
29.0 
30.30 
49.1 
9.4058 
9-4513 
°- I 977 
— 0.49 
5-96 
18 
684 
6 
54 
14.4 
14.0 
15.0 
15.0 
14.60 
43-2 
8.8030 
8-8335 
0.4201 
+ 1-05 
7-50 
15 
670 
6 
56 
11.1 
10.0 
12.0 
IO.I 
10.80 
46.1 
8-5455 
8.5828 
0.6708 
+ 1.68 
8.13 
11 
632 
6 
58 
17-5 
17-5 
19.4 
18.5 
18.22 
50.8 
8.9901 
9.0409 
10 
818 
7 
0 
32.8 
304 
31-5 
28.8 
30.88 
46.0 
9.4207 
9-4577 
Mittel aus den 
V ergleichsternbeobachtunge 
n: 9.2629; 9-2485; 9 - 2493 - 
Zur Reduction benutzt: 9.2536. 
21