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

240 
Müller und Kempf, Photometrische Durchmusterung 
240 
B.D. 
Sternzeit 
I 
II 
III 
IV 
J 
z 
log sin 2 J 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
IO° 
4604 
23h 
2 2 m ! 
3185 
2888 
3180 
Ni ! 
• O 
O : 
29858 
47 -i 
9.3869 
9.4268 
9 
5 111 
23 
25 
24.0 
234 
22.9 
22.0 
23.08 
43-3 
9.1866 
9.2174 
11 
4613 
23 
3 ° 
17.7 
16.0 
17.4 
15.6 
16.68 
47-5 
8.9159 
8.9568 
0.3629 
-f- 0.91 
7-45 
19 4748 
23 
31 
17.0 
17.0 
18.1 
17.0 
17.28 
404 
8.9456 
8.9707 
0.3490 
+ 0.87 
7.41 
19 
4754 
23 
32 
37-5 
34-8 
354 
35 -o 
35-68 
39-8 
9-5317 
9-5558 
0.2361 
— O.59 
5-95 
18 4845 
23 
34 
16.5 
14.0 
17.0 
154 
I 5-72 
40.2 
8.8658 
8.8906 
0.4291 
+ U07 
7.61 
14 4668 
23 36 
32.0 
29.4 
33-9 
30.1 
31-35 
44.6 
9-4325 
9.4662 
0.1465 
— O.37 
6.17 
9 4872 
23 
37 
20.7 
18.0 
20.0 
20.5 
19.80 
48.9 
9-0597 
9.1046 
0.2 15 I 
+ O.54 
7.08 
10 
4604 
23 
39 
31.0 
29.4 
29.1 
29.0 
29.62 
48.7 
9-3879 
9.4322 
9 
5 111 
23 
41 
24.7 
23.1 
234 
23.0 
23-55 
44.0 
9.2032 
9-2355 
Mittel aus den Vergleichsternbeobachtungen: 9.3033; 9.3221; 9.3338. Zur Reduction benutzt: 9.3197. 
In der Nähe des Vergleichsterns Nr. 46 sind Streifen am Himmel zu sehen. 
Zone 
288. 
1888 December 13. 
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 1 
—2. 
9 ° 
5 111 
23h 
45 m 
2482 
2I?3 
2 2?9 
2 2?3 
22? 68 
4482 
9 - 1 723 
9.2051 
IO 
4604 
23 
47 
3 T -5 
27-5 
274 
27-5 
28.48 
49.6 
9-3567 
9-4037 
*)i6 4746 
23 
50 
14.7 
13-3 
16.9 
14.0 
14.72 
39-6 
8.8100 
8.8337 
O.4634 
+ 1.16 
7.70 
12 
4838 
23 
51 
24.0 
21.5 
234 
22.6 
22.88 
43-3 
9-1795 
9.2103 
0.0868 
+ 0.22 
6.76 
12 
4843 
23 
53 
16.4 
I4.6 
14.6 
13-1 
14.68 
43 -o 
8.8076 
8.8377 
0-4594 
+ I.I 5 
7.69 
15 4670 
23 
55 
26.6 
24.2 
28.0 
26.8 
26.40 
41.0 
9.2960 
9.3222 
O.O25 I 
— O.06 
6.48 
19 
4949 
23 
56 
25.1 
23.O 
25.2 
24.6 
24.48 
37 -o 
9.2348 
9.2544 
O.O427 
+ O. I I 
6.65 
*9 
4965 
23 
58 
25.2 
2O.7 
23.0 
22.2 
22.78 
36.8 
9-1759 
9.1952 
O.IOI9 
+ O.25 
6.79 
9 
5 111 
23 
59 
22.4 
23.6 
24.6 
21.6 
23-05 
45 -i 
9.1856 
9.2204 
IO 
4604 
O 
1 
28.7 
26.7 
28.3 
2 Ó.I 
27-45 
5 1 - 1 
9-3274 
9-3 79 1 
13 
4944 
O 
3 
15-7 
I3.O 
16.2 
I4.2 
14.78 
42.6 
8.8134 
8.8427 
O.4544 
+ 1 • 14 
7.68 
IO 
4781 
O 
5 
23-7 
22.3 
22.6 
24.6 
23 - 3 ° 
45-4 
9- I 944 
9.2300 
O.0671 
+ 0.17 
6.71 
11 
4838 
O 
6 
27.2 
26.0 
26.1 
24.4 
25.92 
44.6 
9.2812 
9 - 3 H 9 
0.0178 
O.O4 
6.50 
12 
4850 
O 
7 
19.9 
l6.6 
19.9 
17.4 
18.45 
44.2 
9.0007 
9-0335 
0.2636 
-j- 0.66 
7.20 
l8 
5 OI 4 
O 
9 
31.2 
3 !*3 
33-5 
30.0 
31-50 
38.2 
9.4362 
9-4576 
0.1605 
O.4O 
6.14 
l8 
5 ° 21 
O 
10 
23.1 
23.0 
24.6 
21.6 
23.08 
38.2 
9.1866 
9.2080 
0.0891 
+ 0.22 
6.76 
9 
5 111 
0 
12 
21.5 
21.4 
23.0 
22.2 
22.02 
46.1 
9.1479 
9.1852 
IO 
4604 
O 
14 
28.5 
26.5 
28.5 
26.9 
27.60 
52.6 
9 - 33 I 7 
9.3888 
Mittel aus den Vergleichsternbeobachtunge 
n: 9.3044; 9.2998; 9.2870. 
Zur Reduction benutzt: 9.2971 
0 1604746 dupl. Gemessen die hellere, 
vorangehende Componente 
Zone 289. 
1888 December 13. 
Beobachter: Kempf. 
Photometer: D. Vergleichsterne: Nr. 6 und Nr. 8. 
Luft: 1— 
2. 
8 C 
385 
O 1 
35m 
2Q?2 
2985 
3284 
3382 
31808 
48?5 
9.4257 
94694 
9 
472 
O 
38 
18.4 
18.4 
18.0 
I 7.O 
17-95 
55.8 
8.9777 
9-0479 
15 
430 
O 
41 
27.6 
28.4 
26.5 
29.I 
27.90 
45-8 
9.3404 
9-3769 
0.1072 
O.27 
6-59 
13 
496 
O 
43 
I 7.O 
16.4 
19.1 
19.7 
18.05 
47-5 
8.9823 
9.0232 
0.2465 
+ O.Ó 2 
7.48 
11 
434 
O 
44 
18.9 
17.6 
17.4 
18.2 
18.02 
49.4 
8.9809 
9.0273 
0.2424 
+ O.61 
7-47 
17 
493 
O 
46 
28.6 
26.4 
29.6 
30.0 
28.65 
43-8 
9 - 36 i 5 
9-3934 
0.1237 
— O.3I 
6-55 
18 
414 
O 
47 
30.0 
29.0 
31-5 
304 
30.25 
43 -o 
9.4045 
9-4346 
0.1649 
O.4I 
6-45 
18 
418 
O 
49 
22.1 
19-5 
20.5 
22.0 
21.02 
42.3 
9.1095 
9 - i 3 8 2 
O.I 3 I 5 
+ 0-33 
7- I 9 
8 
385 
O 
51 
35-4 
304 
32.9 
30.0 
32.18 
47.2 
9.4528 
9.4929 
9 
472 
O 
54 
20.0 
17.0 
18.1 
18.4 
18.38 
53-8 
8-9975 
9.0592 
IO 
418 
O 
56 
18.3 
15-9 
18.7 
17.4 
I 7-58 
49.1 
8.9601 
9.0056 
0.2641 
+ 0.66 
7-5 2 
12 
445 
O 
58 
20.1 
17.6 
19.4 
I9.O 
19.02 
47.1 
9.0262 
9.0661 
0.2036 
+ 0.51 
7-37 
12 
452 
O 
59 
28.0 
30.2 
324 
31.2 
3048 
47. 1 
9.4104 
9-4503 
0.1806 
— 0.45 
6.41 
11 
445 
1 
1 
32-5 
28.5 
31-5 
324 
31-22 
47-9 
9.4292 
9.4712 
0.2015 
— 0.50 
6.36 
15 
446 
1 
3 
16.5 
1 7 - 1 
16.5 
I 7.2 
16.82 
44.0 
8.9229 
8.9552 
0 . 3 H 5 
+ 0.79 
7-65 
15 
447 
1 
4 
17.0 
16.0 
17-5 
15-5 
16.50 
43-5 
8.9067 
8-9379 
0.3318 
+ 0-83 
7.69 
8 
385 
1 
7 
34 -o 
29-5 
35 -o 
32.0 
32.62 
46.0 
9-4633 
9-5003 
9 
472 
1 
IO 
20.7 
16.0 
18.9 
17.6 
18.30 
51-9 
8.9938 
9.0483 
Mittel aus den Vergleichsternbeobachtunge 
n: 9-2587; 9-2760; 9-2743- 
Zur Reduction benutzt: 9.2697.
	        
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