134
Müller und Kempf, Photometrische Durchmusterung
134
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 21.
1886 October 29.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 4
und Nr. 6. Luft: 1.
IO°
168
o*
30“
20?5
i 8?5
20?5
1785
19825
4285
9.0362
9-0653
8
385
0
34
29.4
26.2
364
31.0
30.72
48.6
9.4166
9.4606
2
270
0
38
34 -o
31.6
36.7
324
33-68
5 1 - 1
9.4879
9 - 539 6
0.2795
— 0.70
5-98
6
275
0
40
18.5
17.0
21.5
20.3
19.32
47.0
9-0393
9.0789
0.1812
4~ O.45
7-13
9
235
0
43
19.7
17.4
19-5
19.7
19.08
44-3
9.0288
9.0618
0.1983
+ O.50
7.18
8
292
0
45
22.0
20.6
22.5
2 1.6
2 1.68
46.0
9-1350
9.1 720
0.0881
+ 0.22
6.90
i
347
0
47
26.9
29.0
32.2
29.2
29.32
52.8
9-3798
9-4377
0.1776
— O.44
6.24
5
274
0
54
24.1
21.0
23.1
21.3
22.38
48.5
9-1613
9.2050
0.0551
+ °- I 4
6.82
IO
168
0
57
20.1
20.4
20.1
I9.6
20.05
41.6
9.0702
9-0975
8
385
1
0
314
29.6
35-3
27.6
30.98
46.5
9.4232
9.4615
2
3 11
1
3
35 -o
31.0
32.5
31.0
3248
50.9
9-4575
9.5086
0.2485
— 0.62
6.06
3
273
1
4
19.4
16.4
17-3
17.4
1 7.62
49.6
,8.9620
9.0090
0.2511
+ 0.63
7-31
7
313
1
6
21.0
18.1
18.5
18.3
18.98
46.2
9.0244
9.0619
0.1982
+ 0.50
7.18
7
317
1
8
16.4
17.2
15.6
16.O
16.30
46.0
8.8964
8-9334
0.3267
+ 0.82
7-50
7
321
1
10
22.2
18.5
23.1
22.3
21.52
46.2
9.1290
9.1665
0.0936
+ 0.23
6.91
9
264
1
11
17-5
18.0
20.6
20.0
19.02
43-9
9.0262
9.0583
0.2018
4 - 0.50
7.18
IO
168
1
14
18.6
18.0
22.3
19-3
19-55
41.5
9.0492
9.0763
8
385
1
17
25-5
27.0
31.6
30.8
28.72
45-4
9-3635
9 - 399 1
Mittel aus den Vergleichsternbeobachtungen: 9.2630
; 9- 2 795; 9- 2 377- Zur Reduction benutzt: 9.2601.
Zone 22.
1886 October 29.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 4
und Nr. 6. Luft: 2.
8°
385
i h
19™
2585
2480
2Ó?5
2687
25868
4582
9.2737
9.3088
io
168
1
23
15.0
17.2
17.7
15.2
16.28
41.5
8.8954
8.9225
9
266
1
27
19.6
17.7
17-5
18.4
18.30
43-4
8.9938
9.0248
0.0947
+ 0.24
6.92
6
324
1
29
18.6
1 7.2
18.1
16.5
1 7.60
46.4
8.9611
8.9991
0.1204
+ 0.30
6.98
7
324
1
31
23.0
23-3
24.6
24.O
23.72
45-0
9.2090
9.2436
0.1241
— 0.31
6-37
5
285
1
33
15-9
15.0
15-7
I4.7
I5-32
47-3
8.8439
8.8843
0.2352
+ 0.59
7.27
3
288
1
34
13.8
11 -5
13-5
12.3
12.78
49. 1
8.6896
8-7351
0.3844
+ 0.96
7.64
3
289
1
36
14.7
16.5
18.0
15.2
16.10
49-5
8.8859
8.9326
0.1869
4 - 0.47
7-15
IO
168
1
38
15-7
17.0
18.1
15-5
16.58
41.7
8.9108
8.9383
8
385
1
40
27.8
25.2
24.6
234
25.25
44-3
9.2600
9.2930
7
347
1
42
28.0
27.7
30.7
32.6
29-75
44.6
9-39I3
9.4250
0.3055
— 0.76
5-92
2
346
1
44
1 7-7
15-5
17.6
I9.2
17 - 5 °
49-7
8-9563
9.0036
0.1159
+ 0.29
6.97
2
347
1
46
19.6
19.6
20.2
2 1.6
20.25
50-3
9.0785
9.1277
0.0082
— 0.02
6.66
4
367
1
47
18.6
18.0
18.6
i8.2
18.35
48.1
8.9961
9.0387
0.0808
+ 0.20
6.88
o
369
1
49
13-5
12.0
14-3
13-5
13-32
51-4
8.7249
8-7777
0.3418
4-0.85
7-53
o
37 °
1
5 1
16.7
154
18.5
15.2
16.45
52.3
8.9041
8.9601
0.1594
4- 0.40
7.08
IO
168
1
53
17.0
18.4
19.i
14.6
17.28
42.2
8.9456
8.9741
8
385
1
55
26.4
234
254
244
24.90
43-6
9.2486
9.2800
Mittel aus den Vergleichsternbeobachtungen: 9.1157; 9.1156; 9.1271.
Zur Reduction benutzt: 9.1195.
Zone 23.
1886 October 30.
Beobachter: Kempf.
Photometer: D. Ver (
^leichsterne : Nr. 40
und Nr. 42. Luft:
2.
IO°
398 i
20 1
3 2 m
2 3?o
21?0
2 l?l
2 0?9
21850
4383
9.1282
9.1590
IO
4351
20
34
25.1
22.2
22.9
23.6
23-45
41.6
9- I 997
9.2270
8
4200
20
38
23.2
22.5
25.0
22.7
23-35
45-6
9.1962
9.2322
0.0576
— 0.14
6.66
7
4210
20
40
27.6
26.5
304
28.0
28.12
46.7
9-3467
9-3855
0.2109
— 0.53
6.27
3 4138
20
43
20.0
18.3
20.5
17.O
18.95
50.2
9.0231
9.0719
0.1027
+ 0.26
7.06
0
4314
20
45
19.0
18.1
19.O
18.O
18.52
53-2
9.0039
9.0633
0.1113
+ 0.28
7.08
5
4295
20
47
20.7
18.2
20.0
20.0
19.72
^8.7
9-0563
9.1006
0.0740
4- 0.18
6.98
7
4252
20
50
22.5
23-5
23.O
21.8
22.70
46.7
9 - I 73 °
9.2 118
0.0372
— 0.09
6.71
IO
3981
20
52
21-5
21.4
22.0
20.0
21.22
44.6
9-“73
9-I5IO
