126
Müller und Kempf, Photometrische Durchmusterung
126
B.D.
Sternzeit
I
II
III
IV
/
2
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 1
1886 October 3.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 44 und Nr. 46. Luft:
2.
io°4Ó04
2 2 h 2g m
3087
2785
2982
2582
28?i 5
4384
9-3475
9-3785
9 5 111
22 35
20.7
19.6
22.5
20.4
20.80
42.5
9.1007
9.1298
7 4853
22 39
23.6
21.4
24.9
22.0
22.98
45 -o
9.1831
9.2177
0.0163
-f- 0.04
6.58
3 4705
22 43
24-5
25-7
28.2
24.0
25.60
48.8
9.2711
9-3157
0.0817
■— 0.20
6-34
3 4713
22 46
27-5
27.2
32.1
25-9
28.18
48.7
9-3483
9.3926
0.1586
— 0.40
6.14
8 4906
22 49
14.5
12.5
14.1
13.0
13-52
43-8
8-7377
8.7696
0.4644
+ 1.16
7.70
3 4745
22 52
18.5
16.2
20.6
18.1
18.35
48.5
8.9961
9.0398
0.1942
+ 0-49
7-°3
3 4751
22 54
20.9
19.9
25-5
17-5
20.95
48.5
9.1067
9.1504
0.0836
+ 0.21
6-75
10 4604
22 58
26.0
25-5
26.5
24.2
25-55
45 -i
9.2696
9.3044
9 5111
23 2
23.8
20.6
24*5
21.0
22.48
42.6
9.1650
9-1943
4 4894
23 5
14.7
14*5
16.2
14-5
14.98
48.1
8.8249
8.8675
0.3665
+ 0.92
7.46
4 4896
23 8
18.4
21.5
25*5
19-5
21.22
48.5
9-1173
9.1610
0.0730
+ 0.18
6.72
0 4912
23 IO
15-4
14.8
18.4
154
16.00
52.3
8.8807
8.9367
0.2973
+ 0.74
7.28
3 4763
23 12
13.2
12.1
16.5
13-5
13.82
49.6
8-7563
8.8033
0.4307
+ 1.08
7.62
5 5065
23 15
13.6
12.7
15-7
12.7
13.68
46.9
8.7477
8.7870
0.4470
+ 1.12
7.66
6 5060
23 17
14.0
14.6
18.0
15.0
15.40
46.0
8.8483
8.8853
0.3487
00
d
+
7.41
10 4604
23 20
24.6
25.0
24.0
21.5
23.78
47.0
9.2111
9.2507
9 5111
23 23
20.4
23.0
22.2
19.1
21.18
43-2
9-1157
9.1462
Mittel aus den Yergleichsternbeobaehtungen: 9.2541; 9.2494; 9.1984.
Zur Reduction benutzt: 9.2340.
Zone 2
1886 October 5.
Beobachter: Müller. Photometer: Ci. Vergleichsterne: Nr. 45 und Nr. 47. Luft: 2
— 3 -
8°4997
2 2 h 3 111
I 6?2
17?6
i6?8
1683
16872
4582
8.9179
8-9530
11 4784
22 6
12.0
13.0
11.7
12.4
12.28
40-7
8.6555
8.6812
0 4872
22 9
15-7
15.8
15-7
154
15-65
51.6
8.8619
8.9154
0.1332
— 0.33
4-55
3 4710
22 12
13-3
13-5
12.5
134
13.18
48-3
8.7159
8-7591
0.0231
+ O.06
4.94
8 4874
22 14
9-1
IO.I
9-7
11-3
10.05
43 - 9 .
8.4836
8.5157
0.2665
+ O.67
5-55
13 4971
22 l8
9.4
10.5
9-3
10.7
9.98
38.6
8.4776
8.4997
0.2825
+ O.71
5-59
ii 4875
22 21
17.O
17.4
17-3
17-3
17-25
40.9
8.9442
8.9702
0.1880
— O.47
4.41
ii 4784
22 23
n.7
11*9
1 1-9
13.0
12.12
40.7
8.6443
8.6700
8 4997
22 25
16.2
15-4
15.8
17.1
16.12
44.2
8.8870
8.9198
9 5122
22 28
11.6
12.1
11.4
12.5
11.90
43-3
8.6286
8.6594
0.1228
+ O.31
5-19
8 4961
22 30
11.6
13-9
12.6
13.6
12.92
44-3
8.6989
8.7319
0.0503
+ O.13
5.01
16 4831
22 32
10.3
10.3
9-5
114
10.38
36.3
8-5113
8.5299
0.2523
+ O.63
5-51
19 5036
22 34
10.0
11*4
10.5
11-3
10.80
32.4
8-5455
8.5592
0.2230
+ O.56
5-44
3 4818
22 36
13-7
16.5
14.9
14.6
14.92
49-4
8.8214
8.8678
0.0856
0.21
4.67
7 498 i
2 2 40
12.7
13-5
134
13.8
13-35
44-5
8.7268
8.7602
0.0220
+ 0.05
4-93
9 5170
22 42
10.6
11.0
10.7
11.7
11.00
43-4
8.5612
8.5922
0.1900
+ 0.47
5-35
8 4997
22 43
14.7
15*1
14-5
17.0
I 5-32
43-7
8.8439
8.8755
ii 4784
22 45
10.6
I 1.0
11.6
11.1
11.08
41.1
8.5674
8.5938
Mittelaus den Yergleichsternbeobaehtungen: 8.8171; 8.7949; 8.7347.
Zur Reduction benutzt: 8.7822.
Zone 3
1886 October 5.
Beobachter: Kempf.
Photometer :
Ci. Vergleichsterne: Nr. 47 und Nr.
I. Luft:
2.
8°4997
23I1 j gm
i6?6
i8?8
2 I ?0
20?0
19810
4387
9.0297
9.0613
10 8
23 24
11.0
11 -5
12.5
12.5
11.88
42.7
8.6272
8.6567
16 4882
23 3 °
10.6
12.4
I I .2
12.4
11.65
35-8
8.6104
8.6283
O.2663
—]-~ O.67
5.87
4 4997
23 32
13-5
16.0
15-3
16.4
15-30
47-7
8.8428
8.8843
O.OIO3
+ 0.03
5-23
ii 4993
23 35
14.7
15-5
15.0
16.4
15.40
40.8
8.8483
8.8741
0.0205
+ 0.05
5-25
0 4998
23 38
13.2
14.8
15.0
17.4
15.10
51-9
8.8316
8.8861
0.0085
-|- 0.02
5.22
5 5173
23 40 1
18.8
22.0
24.2
234
22.IO
46.7
9.1509
9-1897
O.2951
— O.74
4.46
ii 5°°9
23 43
20.5
21-5
19.8
21.8
20.90
40.4
9.1047
9.1298
O.2352
— 0.59
4.61
