128
Müller und Kempf, Photometrische Durchmusterung
128
B.D.
Sternzeit
I
II
III
IV
J
z
logsin 2 /
corrig,
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 6.
1886 October 11.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 46 und Nr. 48. Luft:
3 -
9 ° 5 111
22 h 25 m
i8?6
19?8
2I?3
1984
19878
4286
9.0589
9.0882
9 5277
22 29
17.4
16.6
19-3
19.6
18.22
45-2
8.9901
9.0252
0 4950
22 31
36.6
29.4
35-2
32.7
3348
52.2
94833
9-5389
0.5181
— I.30
546
4 4935
22 33
12.6
12.2
14.6
12.4
12-95
48.0
8.7009
8-7432
0.2776
-(— O.69
745
2 4594
22 35
24-5
22.7
27.9
25.6
25.18
50.1
9-2577
9.3062
0.2854
— O.71
6.05
2 4597
22 37
18.5
16.7
20.4
18.1
18.42
49.6
8.9993
9.0463
0.0255
— 0.06
6.70
3 4814
22 39
13-7
14.6
14.0
13-5
13-95
48.7
8.7643
8.8086
0.2 122
+ 0-53
7.29
5 5123
22 41
17.9
18.4
20.4
18.3
i 8.75
46.5
9.0142
9-0525
O.O3 I 7
— 0.08
6.68
9 5111
22 43
17.7
17.0
20.8
17.4
18.22
42.5
8.9901
9.0192
9 5277
22 45
16.4
17-3
19-5
16.8
17 - 5 °
44-3
8-9563
8.9893
0 4963
22 48
18.6
16.8
20.1
18.5
18.50
51-7
9.0030
9.0568
O.O360
— 0.09
6.67
1 4686
22 50
31-5
32-5
32.1
34-5
32.65
50.9
9.4640
9 - 5 I 5 I
O.4943
— 1.24
542
6 5124
22 52
10.7
10.8
II.9
11.0
I I.IO
45-6
8.5690
8.6050
O.4158
+ 1.04
7.80
4 4975
22 53
16.2
15.6
17.6
20.6
17.50
48.0
8.9563
8.9986
0.0222
+ 0.06
6.82
4 4985
22 55
13-5
13-3
14.0
12.6
13.35
48.0
8.7268
8.7691
O.2517
+ O.63
7-39
7 4991
22 57
30.0
33-4
38.7
36.0
34.52
44-3
9.5067
9-5397
O.5189
— 1.30
546
9 5111
22 59
17.0
17.4
19.6
18.4
18.10
42.6
8.9846
9.0139
9 5277
23 I
18.5
15-7
18.6
17-3
17-52
43-6
8-9573
8.9887
Mittel aus den Vergieichsternbeobaehtungen
: 9.0567
; 9.0043; 9.0013. Zur Reduction benutzt: 9.0208.
Zone 7.
1886 October 11.
Beobachter: Kempf. Photometer: D
Vergleichsterne: Nr. 46 und Nr. 48.
Luft: 2-
- 3 -
9 ° 5 2 7 7
23h ym
1989
i8?o
2389
1980
20820
4384
9.0764
9.1074
9 5m
23 II
23.1
21.2
20.7
19.6
21.15
42.8
9.1146
9-1443
5 5150
23 14
12.5
12.5
12.9
11 .5
12-35
46.8
8.6604
8.6995
O.4237
-f- 1.06
7.82
7 5009
23 16
16.5
16.8
20.0
16.6
17.48
45 -o
8-9553
8.9899
0.1333
+ O.33
7.09
8 5058
23 18
14.0
13.0
15-9
14-5
14-35
44.1
8.7884
8.8209
O.3023
+ O.76
742
7 5030
23 20
18.2
15-5
18.5
16.5
17.18
44.4
8.9407
8-9739
O.1493
+ O.37
7-13
0 4999
23 22
20.8
20.5
27.6
22.4
22.82
51-9
9-1773
9.2318
O.IO86
— O.27
6-49
4 5 OI 6
23 24
17.1
14-3
16.6
15.6
15.90
48.0
8.8754
8.9177
0.2055
+ O.51
7.27
9 5111
23 27
21.4
20.3
21.0
20.1
20.70
43-5
9.0967
9-1279
9 5277
23 30
22.7
19.1
22.9
19.0
20.92
42.8
9-1055
9-1352
23 35
12.7
10.9
13-5
11.0
12.02
47.8
8.6372
8.6790
O.4442
+ I.11
7.87
J 4 5 OI 9 i
23 37
9.4
8.0
10.6
8.2
9-05
47.8
8-3935
8-4353
O.6879
+ I- 7 2
8.48
6 5168
23 39
17.7
16.3
23.0
18.0
18.75
45-9
9.0142
9.0510
O.O722
+ 0.18
6-94
0 5018
23 42
18.7
19-5
25-9
22.9
21-75
51-7
9-1377
9 -I 9 I 5
O.0683
— O.17
6-59
7 5059
23 45
21.4
20.4
22.4
20.0
21.05
44.6
9.1107
9.1444
0.0212
— 0.05
6.71
7 5 o6 °
23 47
15.6
14-5
15-9
14.8
15.20
44-7
8.8372
8.8711
O.252I
+ O.63
7-39
9 5 111
23 49
24.2
21.9
19.7
20.0
21.45
44-5
9.1263
9-1597
9 5277
23 52
19.4
18.0
20.5
19.0
19.22
42.8
9.0349
9.0646
Mittel aus den
Vergleichsternbeobachtungen: 9.1259; 9.1315; 9.1122. Zur Reduction benutzt: 9.1232.
*) 4 0 5019 dupl. Die Messung der zweiten, südlicheren Componente schwierig.
Zone 8.
1886 October 19.
Beobachter: Müller.
Photometer :
D. Vergleichsterne: Nr. 40
und Nr. 42. Luft:
2.
io°3981
20“39 m
l6?5
''st“
O •
1983
i6?8
17850
4387
8-9563
8.9879
10 4351
20 42
19.1
21.3
22.4
19-5
20.58
41-5
9.0919
9.1190
7 4441
20 45
14.4
15-3
16.4
154
15.38
45-5
8.8472
8.8830
O.I 577
+ 0-39
7.19
1 4268
20 46
12.3
12.5
12.9
12.0
12.42
51-5
8.6652
8-7183
0.3224
+ O.81
7.61
6 4508
20 48
11.9
10.6
13-7
12.5
12.18
46.1
8.6485
8.6858
0-3549
-1- 0.89
7.69
9 45 o 8
20 50
16.7
18.2
19-3
17.2
I 7-85
42.9
8.9730
9.OO29
0.0378
+ 0.09
6.89
0 4495
20 52
19.1
18.7
22.1
21.2
20.28
52.2
9-0797
9-1353
0.0946
— O.24
6.56
0 4496
20 53
19-7
20.0
21.0
19.0
19.92
51-9
9.0647
9.1 192
0.0785
0.20
6.60
10 3981
20 55
15-7
16.7
16.1
154
15.98
44.8
8.8796
8.9137
10 4351
20 57
20.4
20.0
21.7
19.2
20.32
41.7
9.0813
9.1088
