156
Müller und Kempf, Photometrtsche Durchmusterung
156
B.D.
Sternzeit
I
II
III
iv 1
J
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Difi'. in I
Grössen j
Grösse
Zone 77.
1887 Februar 9.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 6 und Nr. 8.
Luft: 1 —
2.
9 °
472
4 h 59 "
13?o
1387
I 5 °3
1583
14832
4680
8.7866
8.8236
8
385
5 i
25.6
25-4
24.7
244
25.02
53-7
9-2525
9 - 3 I 38
15
430
5 4
19-5
20.0
22.1
18.5
20.02
44.6
9.0689
9.1026
O.O407
— 0.10
6.76
13
496
5 6
11.6
14.0
12.7
11.2
12.38
46.5
8.6624
8.7007
O.3612
+ 0.90
7.76
11
434
5 8
15.0
15-3
154
15-7
15-35
48.6
8.8456
8.8896
O.1723
+ 0-43
7.29
IO
418
5 9
10.7
12.9
134
12.7
12.42
49.2
8.6652
8.71 IO
0.3509
+ 0.88
7-74
17
493
5 ”
23-7
22.5
24.O
21.4
22.90
43-3
9.1802
9.2 I IO
O.1491
— 0-37
6-49
18
414
5 13
25-3
22.7
24.7
22.6
23.82
42-5
9.2125
9.2416
O.1797
— 0.45
6.41
8
385
5 15
2 5-7
22.5
25.6
23.6
24-35
55-4
9-2305
9.2990
9
472
5 17
13.6
12.7
15-3
144
14.00
47-4
8.7674
8.8081
18
418
5 19
15.0
14.6
I 7.6
15.6
15 - 7 °
42.7
8.8647
8.8942
O.1677
+ 0.42
7.28
12
445
5 20
12.1
134
I4.O
15.0
13.62
48.4
8-7439
8.7874
O.2745
+ 0.69
7-55
12
452
5 22
23.8
23.6
25-3
23-3
24.00
48.3
9.2186
9.2618
O.1999
— 0.50
6.36
11
445
5 24
26.3
24-3
23.6
23-3
24.38
49-7
9 - 23 I 4
9.2787
0.2 l68
— 0-54
6.32
15
446
5 25
12.8
12.6
14-5
13-3
13-30
45-8
8.7236
8.7601
O.3O18
+ 0.75
7.61
15
447
5 26
12.6
11.6
14.7
13.6
13.12
45-6
8.7120
8.7480
0.3139
+ 0.78
7.64
8
385
5 29
26.3
22.7
26.2
2 1.0
24.05
57-2
9.2203
9.2971
9
472
5 31
14.7
13.0
14.8
14.7
14.30
48.8
8.7854
8.8300
Mittel aus den
Vergleichsternbeobachtungen
: 9.0687; 9-0536; 9-0635-
Zur Reduction benutzt: 9.0619.
Zone 78
1887 Februar 9.
Beobachter : Kempf.
Photometer :
D. Ver
gleichsterne : Nr. 16
und Nr.
18. Luft:
2.
ii°
1588
8 h 30 m
2384
2 7?0
2985
2 5-9
2 6?45
4389
9.2976
9.3297
IO
1818
8 39
22.1
25-7
24.8
25.6
24-55
42.O
9.2372
9-2653
3
1758
8 41
32.1
32.2
334
35 -o
33 - 1 8
50-3
9.4764
9.5256
O.2346
— 0.59
6.09
0
2054
8 43
27.4
28.9
3 i-i
27.6
28.75
53-7
9-3643
9.4256
O.I346
— 0.34
6.34
5
1759
8 44
25.6
21.0
28.4
24.6
24.90
49.2
9.2486
9.2944
O.OO34
— 0.01
6.67
2
1761
8 46
24.5
24.6
26.5
25.2
25.20
51-7
9.2584
9-3122
0.02 12
— 0.05
6.63
2
1776
8 48
16.0
14-5
17.8
16.5
16.20
52.2
8.8912
8.9468
0.3442
+ 0.86
7-54
9
1 766
8 49
19.0
18.4
2 I.4
19-3
19.52
45-3
9.0479
9.0832
O.2078
+ 0.52
7.20
11
1588
8 52
22.4
24.0
30-3
27.0
25.92
45-2
9.2812
9 - 3 I 63
IO
1818
8 54
25-3
23.0
24-5
23-5
24.08
42.2
9.2213
9.2498
5
1790
8 58
22.5
22.4
24.8
28.2
24.48
49-2
9.2348
9.2806
O.OIO4
+ 0.03
6.71
4
1826
8 59
21.0
22.4
27.0
27-5
24.48
50.3
9.2348
9.2840
O.OO7O
+ 0.02
6.70
4
1833
9 i
24-5
25.0
274
24-5
25-35
50.2
9.2632
9.3120
0.02 10
— 0.05
6.63
3
1818
9 3
25-4
29-5
27-5
28.4
27.70
51-4
9-3346
9-3874
O.O964
— 0.24
6.44
7
1844
9 5
15-3
14-5
17.0
16.3
I 5-78
47.6
8.8689
8.9101
O.3809
+ 0.95
7-63
0
2108
9 7
23-9
21.9
25.0
25-5
24.08
54-7
9.2213
9.2867
O.OO43
+ 0.01
6.69
11
1588
9 9
23.5
24-5
27.9
26.3
25-55
46.7
9.2696
9.3084
IO
1818
9 ii
23-4
1 244
24.8
2 6.8
24.85
42.8
9.2470
9.2767
Mittel aus den Vergleichsternbeobachtungcn: 9.2975; 9.2831; 9.2925.
Zur Reduction benutzt: 9.2910
Zone 79.
1887 Februar 10
Beobachter:
Müller.
Photometer
D. Vergleichsterne: Nr. 4
und Nr.
6. Luft : 2.
io c
168
3 h 33 m
h 7?5
I 6?2
i 8?7
17?o
17835
4989
8.9491
8.9970
8
385
3 35
24.7
22.7
27.2
274
25-50
45-6
9.2680
9.3040
17
200
3 37
19-3
17.7
21.0
19.7
19.42
44-5
9.0436
9.0770
O.0577
4-0.14
6.82
16
154
3 39
I9.6
18.4
20.3
18.7
I 9-25
44.8
9.0362
9.0703
O.0644
+ 0.16
6.84
19
238
3 40
21.5
21.4
23.6
21.4
2 1.98
42.7
9.1464
9-1759
O.0412
— 0.10
6.58
17
210
3 42
25-7
25-3
27.7
25.8
26.12
43-9
9.2874
9 - 3 I 95
0.1848
— 0.46
6.22
16
167
3 44
17.8
16.3
20.4
19.2
18.42
45 -i
8.9993
9.0341
0.1006
+ 0.25
6-93
IO
197
3 45
14.7
14.6
16.0
15-9
15-30
50.5
8.8428
8.8926
O.242 I
+ 0.61
7.29
IO
l68
3 47
15-3
14.7
18.1
16.5
16.15
51-5
8.8886
8.9417
