266
Müller und Kempf, Photometrische Durchmusterung
266
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
*) 3°4473
20 h
48™
i6?6
i6?7
16? 1
i6?4
16845
4885
8.9041
8.9478
0.1984
+ O.50
5.26
12 4501
20
50
17.4
13-5
14.0
12.4
14.32
40.3
8.7866
8.8115
0.3347
4- 0.84
5.60
13 4572
20
52
18.0
15.2
18.7
16.4
17.08
39 - 1
8-9358
8.9587
0.1875
+ 0.47
5-23
8 4261
20
55
24.9
20.3
19-9
19.0
21.02
46.2
9.1095
9 - I 47 °
9 4746
20
57
20.5
24.0
21.6
21.2
21.82
42.9
9 - 1 4°4
9.1703
10 4425
20
59
17-5
14.4
15-5
16.5
15.98
42.0
8.8796
8.9077
0.2385
-j- 0.60
5-36
18 4675
2 I
1
15.0
15-1
17.6
14.4
I 5-52
33-5
8.8549
8.8699
0.2763
-4- 0.69
5-45
4 4606
2 I
3
16.0
14-5
15.0
134
14.72
47-3
8.8100
8.8504
0.2958
+ 0.74
5-50
9 4732
2 I
5
23-4
23.6
22.5
22.6
23.02
42.7
9.1845
9.2140
0.0678
— 0.17
4-59
4 4635
2 I
7
27.1
30.0
27.6
29.4
28.52
47.6
9-3579
9 - 399 1
0.2529
— 0.63
4 -i 3
19 4691
2 I
8
28.2
25-5
28.4
29.0
27.78
33-1
9-3369
9-3514
0.2052
— 0.51
4-25
8 4261
21
10
25.0
22.5
24-5
20.9
23.22
47.2
9.1916
9 - 23 I 7
9 4746
2 I
12
23.0
23.0
24-5
21.6
23.02
42.8
9.1845
9.2142
Mittel aus den Vergleichsternbeobachtungen: 9.0571; 9.1587; 9.2229. Zur Reduction benutzt: 9.1462.
*) 3°4473 dupl. Nur die helle Componente gemessen.
Zone 353. 188g October 16.
Beobachter: Müller. Photometer: Ci. Vergleichsterne: Nr. 43 und Nr. 45. Luft: 3—4.
9 ° 47 4 6
2I h
l6 m
22? 7
2I?8
2 2?6
i8?8
21848
4288
9- I2 74
9 -i 57 i
11 4784
21
19
19.7
15-4
16.3
14.2
16.40
42-3
8.9015
8.9302
6 4811
21
2 I
16.4
13.0
I3.6
H -3
14.32
46.1
8.7866
8.8239
0.2267
+ 0.57
5-49
18 4827
21
23
16.1
11.6
16.3
11.4
13-85
33-6
8.7582
8-7733
0.2773
+ 0.69
5.61
1 4517
21
26
17.0
13.8
l6.6
14.2
15.40
50.6
8.8483
8.8984
0.1522
+ 0.38
5-30
o 4770
21
28
13.6
11.2
I4.O
10.2
12.25
51.6
8.6534
8.7069
0-3437
+ 0.86
5.78
5 4850
2 I
30
18.3
I 5 - 1
15-2
13.0
15.40
47.2
8.8483
8.8884
0.1622
+ 0.41
5-33
16 4582
21
33
25-9
23.0
26.7
23-4
24-75
35-5
9.2438
9.2613
0.2107
— 0.53
4-39
9 4746
2 I
35
22.4
22.0
19.8
19.7
20.98
43 - 1
9 -i °79
9.1382
11 4784
2 I
38
18.7
18.4
17.6
16.6
17.82
41.4
8.9715
8.9985
2 4414
2 I
40
13-5
12.3
13.6
11.6
12.75
50.2
8.6876
8.7364
0.3142
+ 0.79
5 - 7 1
16 4612
2 I
42
13.8
12.0
16.2
11.1
13.28
35-6
8.7223
8.7400
0.3106
+ 0.78
5-70
19 4797
2 I
45
11 -7
10.7
11-5
11-3
11.30
33 -i
8.5843
8.5988
0.4518
+ 1.13
6.05
18 4879
2 I
46
i 3-3
13-5
11.2
1 1-7
12.42
33-3
8.6652
8.6800
0.3706
+ 0.93
5-85
7 4779
21
48
i 3-4
10.9
11.2
12.3
n -95
44.7
8.6322
8.6661
0-3845
+ 0.96
5-88
4 4800
2 I
50
18.0
15-7
16.4
15-4
16.38
47-9
8.9005
8.9425
0.1081
+ 0.27
5-19
9 4746
21
54
22.7
20.0
20.2
18.6
20.38
43-8
9.0838
9-”57
11 4784
2 I
57
18.1
16.9
16.5
17.0
17.12
40.9
8.9378
8.9638
Mittel aus den Vergleichsternbeobachtungen: 9.0437; 9.0683; 9.0398. Zur Reduction benutzt: 9.0506.
Zone 354. 1889 October 27.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 4.
IO°
4604
23 b
44 m
2 2?5
C •
OO
2 2?4
2384
21875
4983
9-1377.
9 .i 838
9
5 111
23
47
21.4
16.2
I9.6
i 7-5
18.68
44.4
9.0111
9.0443
10
4681
23
5 i
27.0
25-3
26.6
24.0
25.72
47-3
9-2749
9 - 3 I 53
0.1992
— 0.50
6.04
18
49 1 7
23
53
13.0
10.2
12.5
10.9
11.65
40.7
8.6104
8.6361
0.4800
+ 1-20
7-74
12
4751
23
55
15.6
12.6
15.2
14.0
14-35
45-6
8.7884
8.8244
0.2917
+ O.73
7.27
14
4730
23
56
21.4
20.4
21.5
22.0
21.32
44-5
9.1212
9- I 546
0.0385
— 0.10
6.44
13
4842
23
58
13-4
12.1
13-7
14.4
13.40
45 -o
8.7300
8.7646
o- 35 i 5
+ 0.88
7.42
11
4724
23
59
12.0
10.7
12.5
12.0
11.80
46.8
8.6214
8.6605
0.4556
+ 1.14
7.68
10
4604
O
1
24-5
22.0
21.5
23-9
22.98
5 1 - 1
9- i 83 i
9.2348
9
5 111
O
4
18.9
17-3
17.6
17.0
17.70
45-5
8.9658
9.0016
Mittel aus den Vergleichsternbeobachtungen: 9.1x41; 9.1182. Zur Reduction benutzt: 9.1161.
Die Beobachtungen wurden wegen plötzlicher Wolkenbildung abgebrochen.
