Full text: Zone 0 [Grad] bis + 20 [Grad] Declination (Theil 1)

174 
175 
Zone o° eis -f- 20° Declination. 
175 
22 * 
Grösse 
7-03 
6.02 
7.10 
7.40 
7-55 
7.68 
6 - 43 
7 - 57 
6.24 
6 - 53 
6.20 
7 - 79 
6.2g 
6.10 
6-39 
6 - 33 
7 - 43 
6.86 
6.66 
5 - 5 i 
6.86 
7-43 
7-53 
7-63 
6.35 
9-32 
7-50 
7-49 
6.97 
5-87 
B.l). 
Sternzeit 
I 
II 
III 
IV 
J 
g 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
ig°i8i8 
io 11 4 m 
22? 7 
2 2?2 
2 I ?5 
2383 
22?42 
4683 
9.1627 
9.2005 
0 2288 
10 7 
14-5 
I4.O 
15-5 
i 3-5 
14.38 
56.7 
8.7902 
8.8646 
0.3367 
4- 0.84 
7.52 
8 2057 
10 9 
16.6 
l6.6 
16.5 
16.0 
16.42 
49-5 
8.9025 
8.9492 
0.2521 
-f-O.63 
7-31 
7 1975 
10 10 
18.1 
I 7.6 
17.6 
16.5 
1745 
50.0 
8.9539 
9.002 1 
0.1992 
4 - 0.50 
7.18 
1 2102 
10 12 
13-5 
14-3 
14.0 
14.0 
13-95 
55-7 
8.7643 
8.8341 
0.3672 
4-0.92 
7.60 
8 2064 
10 14 
19.9 
19-5 
21.5 
18.2 
19.78 
49.0 
9.0589 
9.1041 
0.0972 
4-0.24 
6.92 
0 2312 
10 16 
13-8 
13-9 
14.1 
12.5 
I 3-58 
56.9 
8.7414 
8.8167 
0.3846 
4-0.96 
7.64 
10 1818 
10 17 
21.4 
22.3 
26.0 
23.1 
23.20 
47-5 
9.1909 
9.2318 
11 1588 
10 20 
22.9 
22.1 
22.5 
21.1 
22.15 
54-7 
9.1528 
9.2182 
Mittel aus den 
Vergleichsternbeobachtungen: 9.1709; 9.2079; 9.2250. Zur Reduction benutzt: 9.2013. 
Zone 125. 1887 März 20. 
Beobachter: Müller. 
Photometer: D. Vergleichsterne: Nr. 18 und Nr. 20. Luft: 2 
- 3 - 
10 0 1818 
lO h 23™ 
I9?0 
1984 
19°8 
i9?o 
I983O 
48? 1 
9.0384 
9.0810 
9 2239 
10 26 
15-4 
14.7 
14.7 
15-5 
15.08 
44-3 
8.8305 
8.8635 
10 1837 
IO 28 
24.4 
27.4 
25.O 
24.7 
25-38 
48.5 
9.2642 
9-3079 
0-3355 
— 0.84 
6.11 
10 1840 
IO 29 
18.4 
17-3 
21.2 
18.4 
l8.82 
48.6 
9.0173 
9.0613 
0.0889 
— 0.22 
6-73 
19 2053' 
10 31 
17.4 
17.0 
18.7 
16.5 
I7.4O 
40.2 
8-9515 
8.9763 
0.0039 
— 0.01 
6-94 
ig 206g 
10 33 
15-7 
15.0 
16.9 
15.8 
I 5-85 
40.1 
8.8727 
8.8973 
0.0751 
4- 0.19 
7.14 
15 1862 
10 35 
9-7 
9.8 
II .3 
9-5 
IO.08 
44-3 
8.4862 
8.5192 
0.4532 
4 - 1.13 
8.08 
11 1892 
10 37 
19.7 
18.6 
18.O 
16.0 
18.08 
48.0 
8.9837 
9.0260 
0.0536 
— 0.13 
6.82 
11 1894 
10 38 
1 1*5 
11.2 
I3.6 
1 1-3 
I 1.90 
47-9 
8.6286 
8.6706 
0.3018 
+ 0.75 
7.70 
10 1818 
10 39 
19.6 
19.0 
l8.2 
20.0 
19.20 
49-7 
9.0340 
9.0813 
9 2239 
10 41 
i 5-3 
i 5-3 
154 ' 
15.0 
I 5-25 
45 -o 
8.8400 
8.8746 
13 1972 
10 43 
2 9-5 
31.6 
30.0 
28.0 
29.78 
46.7 
9.3922 
9.4310 
0.4586 
— 11 5 
5.80 
19 2095 
10 45 
17.8 
18.0 
I 7.6 
18.1 
17.88 
4 i -3 
8.9744 
9.0012 
0.0288 
— 0.07 
6.88 
10 1864 
10 47 
29.4 
28.3 
26.4 
304 
28.62 
49-3 
9.3607 
9.4068 
0-4344 
— 1.09 
5.86 
12 1904 
10 48 
24-3 
2 6.6 
24.6 
27.6 
25.78 
47-4 
9.2768 
9 - 3 I 75 
0.3451 
— 0.86 
6.09 
13 1994 
10 50 
18.3 
19.7 
19-3 
17.4 
18.68 
47 -o 
9.0111 
9.0507 
0.0783 
— 0.20 
6-75 
15 1901 
10 51 
9.4 
10.0 
9-5 
10.9 
9-95 
44.8 
8.4750 
8.5091 
0.4633 
4- 1.16 
8.11 
10 1818 
10 54 
20.5 
19.6 
18.8 
17-5 
19.10 
5 i -4 
9.0297 
9.0825 
9 2239 
10 56 
14.6 
14.8 
14.8 
15.0 
14.80 
46.0 
8.8146 
8.8516 
Mittel aus den Vergleichsternbeobachtungen: 8.9723; 8.9779; 8.9671. 
Zur Reduction benutzt: 8.9724 
Zone 126. 1887 März 20. 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 20 
und Nr. 22. Luft: 2 
— 3 - 
g °2239 
II 11 O m 
1780 
1585 
1987 
i6?o 
17805 
4682 
8.9344 
8.9719 
9 2374 
I 1 2 
36.1 
33-8 
34-8 
374 
35-52 
43-7 
9-5283 
9-5599 
5 2248 
11 4 
21.5 
22.2 
21.5 
21.0 
2 i -55 
49.4 
9-1301 
9-1765 
0.0830 
4- 0.21 
6-77 
1 2381 
11 6 
13.0 
12.5 
13.0 
11-3 
1245 
53-4 
8.6673 
8.7274 
0.5321 
+ 1-33 
7.89 
8 2289 
11 7 
20.4 
19-5 
20.5 
19.0 
19.85 
46.9 
9.0618 
9.1011 
0.1584 
4~ 0.40 
6.96 
9 2262 
11 9 
29.1 
314 
3 i-i 
28.5 
30.02 
45-8 
9.3984 
9-4349 
0.1754 
— 0.44 
6.12 
4 2269 
11 11 
19-5 
19.0 
20.1 
18.5 
19.28 
504 
9-°375 
9.0870 
0.1725 
4-0.43 
6.99 
9 2269 
11 12 
25-5 
29.1 
30.0 
31.6 
29.05 
46.4 
9-3725 
9.4105 
0.1510 
— 0.38 
6.18 
9 2239 
11 15 
16.8 
17-5 
174 
19.0 
17.68 
47-3 
8.9649 
9 -oo 53 
9 2374 
11 17 
32.1 
33-8 
34 -i 
364 
34.10 
44-3 
9.4974 
9-5304 
4 2276 
11 19 
18.0 
18.9 
18.7 
16.6 
18.05 
51.6 
8.9823 
9-0358 
0.2237 
4-0.56 
7.12 
4 2283 
I I 20 
14.0 
16.4 
17.2 
14.4 
15-50 
50.8 
8.8538 
8.9045 
0.3550 
— |— O.89 
7-45 
3 2311 
II 22 
18.5 
20.0 
20.6 
19.9 
19-75 
51.6 
9.0576 
9.1111 
0.1484 
+ 0.37 
6-93 
8 2316 
II 23 
14-5 
13-9 
15-7 
15.0 
14.78 
47.1 
8.8134 
8-8533 
0.4062 
4-1.02 
7-58 
6 2259 
II 25 
25.6 
22.4 
25.0 
27.8 
25.20 
49-31 
9.2584 
9-3045 
0.0450 
O.I I 
6-45 
1 2403 
I I 26 
18.4 
19.8 
234 
19.8 
20.35 
53-8 
9.0826 
9-1443 
0.1152 
4-0.29 
6.85 
9 2239 
I I 29 
16.6 
17.0 
20.5 
15.0 
17.28 
48.5 
8.9456 
8.9893 
9 2374 
II 30 
274 
32.9 
36.0 
34-6 
32.72 
44.9 
9-4657 
9.5001 
Mittel aus den 
Vergleichsternbeobachtungen: 9.2659; 9.2679; 9.2447. Zur Reduction benutzt: 9.2595.
	        
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