232
Müller und Kempf, Photometrische Durchmusterung
232
B.D.
II
Stern zeit I
II
III
IV
J
g
logsin 2 /
corrig.
für Ext.
DifF.
in log.
DifF. in
Grössen
Grösse
1 7°4543
23b18 ra
I 2?8
1084
1287
1184
11882
4289
8.6228
8.6527
0.7242
+ 1.81
8.29
17 4546
23 19
16.7
13-4
15-7
14.2
15.00
43 -o
8.8260
8.8561
0.5208
+ 1-30
7.78
17 4548
23 20
15.8
13-3
17.0
14.0
15.02
42.8
8.8271
8.8568
0.5201
+ 1-30
7.78
17 4549
23 22
22.6
20.3
23.8
20.2
21.72
43 -i
9.1366
9.1669
0.2 IOO
+ 0.52
7.00
16 4502
23 23
I4.7
13.8
14.8
134
14.18
44.0
8.7782
8.8105
0.5664
+ 1-42
7.90
15 4404
23 25
I4.9
134
14.9
14.6
14.42
44.2
8-7925
8.8253
0.5516
+ 1-38
7.86
10 4351
23 27
2 5 -2
23.8
26.5
24.2
24.92
54 -o
9-2493
9.3118
10 4604
23 29
29.I
29.4
29.7
2 8.8
29.25
47.8
9.3780
9.4198
Mittel aus den Vergleichsternbeobachtungen: 9.4062; 9.3587; 9.3658.
Zur Reduction benutzt: 9.3769.
Zone
268.
1888 November 14.
Beobachter: Kempf.
Photometer: D. Vergleichsterne Nr. 42 und Nr. 44. Luft: 1
—2.
IO °435 1
2 i h 59 m
2 9?o
25°5
2885
27-5
27862
4489
9-3323
9.3667
10 4604
22 2
33-5
26.9
30.0
28.2
29.65
42.4
9.3887
9.4176
7 4591
22 4
21.9
19.9
22.0
19.9
20.92
47.1
9-1055
9-1454
0.2308
+ 0.58
7.06
6 4718
22 6
30.0
27.7
29.6
30.0
29.32
47.6
9-3798
9.42 10
0.0448
O.I I
6-37
*) 6 4731
22 8
24.7
20.0
23-3
22.5
22.62
47-9
9.1700
9.2120
0.1642
4- 0.41
6.89
2 4289
22 IO
25.0
22.8
24.2
22.4
23.60
51.8
9.2049
9.2591
0.1171
4- 0.29
6.77
2 4297
22 13
27-5
27.0
27.I
27.0
27-15
52.2
9.3186
9-3742
0.0020
4- 0.01
6.49
1 4418
22 16
26.7
25-9
27.O
29.0
27-15
53 -o
9.3186
9-3772
0.0010
0.00
6.48
IO 4351
22 18
29.0
254
27.7
26.6
27.18
46.5
9 - 3 I 94
9-3577
10 4604
22 21
30.9
28.4
28.5
26.1
28.48
43 -o
9-3567
9.3868
5 4697
2 2 23
34 -o
32.0
324
30-5
32-25
49.9
9-4545
9.5024
O.I 2 Ó 2
— 0.32
6.16
4 4613
22 25
21.0
18.0
I9.O
17-5
18.88
504
9.0200
9.0695
O.3067
+ 0-77
7-25
4 4615
22 27
23.2
21.0
20.6
19.7
21.12
50.8
9 -II 34
9.1642
0.2120
+ 0.53
7.01
3 4501
22 29
25.0
21.5
25.O
22.5
23-50
52.4
9.2014
9-2578
O. I 184
+ 0.30
6.78
6 4754
22 31
33 -o
314
3 I-I
31.0
31.62
49.2
9-4391
9.4849
O.IO87
— 0.27
6.21
7 4630
22 33
16.8
14.6
l6.0
13.6
15-25
48.7
8.8400
8.8843
O.49I9
4 - 1-23
7.71
10 4351
22 35
26.0
22.9
25.O
2 6.6
25.12
48.1
9-2558
9.2984
10 4604
22 37
32.6
30.0
30.0
27-5
30.02
43-7
9-3984
9.4300
Mittel aus den
Vergleichsternb eobachtungen
: 9.3922; 9-3722; 9-3642-
Zur Reduction benutzt: 9.3762.
*) 6° 4731 dupl. Gemessen als ein Stern.
Zone 269.
1888 November 14.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 42 und Nr. 44. Luft: 2-
- 3 -
io°4Ó04
22 h 40 m
2880
2782
2885
2783
2 7-75
43?9
9 - 336 i
9.3682
10 4351
22 43
26.4
22.0
26.3
23-3
24.50
48.9
9-2355
9.2804
17 4438
22 45
24.2
21.7
25.O
22.7
23.40
41.8
9.1979
9.2256
O.I24I
+ 0.31
6.79
16 4401
22 47
13-7
I 1.0
I2.9
11.2
12.20
42.4
8.6499
8.6788
O.6709
4- i .68
8.16
15 4 2 8 i
22 49
14.7
11-5
I4.2
13-3
13.42
43-6
8-7313
8.7627
O.587O
+ i -47
7-95
11 4420
22 50
13-8
114
13-5
12.1
12.70
47-4
8.6842
8.7249
O.6248
4 - 1-56
8.04
19 4555
22 51
16.9
15.6
19-5
17.2
17.30
40.7
8.9466
8.9723
0-3774
4 - 0.94
7.42
19 4564
22 53
17.4
16.0
i8.2
16.2
16.95
40.1
8.9294
8.9540
0-3957
4- 0.99
7-47
10 4351
22 54
24.8
24.9
25-5
24-5
24.92
50.1
9.2493
9.2978
10 4604
22 56
29.1
28.5
28.5
29.7
28.95
45 -o
9.3698
9.4044
14 4478
22 59
17-3
17.2
i 8.2
16.4
1 7.28
45-7
8.9456
8.9819
0.3678
+ 0.92
7.40
14 4479
23 0
19.7
16.8
I9.O
17-5
18.25
45-9
8.9915
9.0283
0.3214
4- 0.80
7.28
14 4493
23 2
14.1
12.3
13-9
12.8
13.28
45-7
8.7223
8.7586
0.5911
4 - 1-48
7.96
16 4407
23 4
18.0
16.6
17.0
17.8
17-35
44.1
8.9491
8.9816
0.3681
4- 0.92
7.40
15 4297
23 5
17.0
14-5
16.4
16.2
16.02
45 -o
8.8817
8.9163
o -4334
+ 1.08
7-56
*) 15 43 °°|
23 8
23 9
8.4
15-7
7.0
14.0
8.0
17.1
7-7
144
7.78
I 5-30
45 -i
45-2
8.2631
8.8428
8.2979
8.8779
1.0518
0.4718
4- 2.63
4-1.18
9.11
7.66
10 4351
23 ii
26.4
25.0
26.3
24-5
25-55
52.1
9.2696
9-3249
10 4604
23 13
31.8
30.0
29.0
27.2
29.50
46.4
9-3847
9.4227
Mittel aus den Vergleichsternbeobachtungen
: 9-3243
; 9 - 35 11 ; 9 - 3738 -
Zur Reduction benutzt: 9.3497.
*) 1504300 dupl. Zuerst die vorangehende Componente gemessen.
