250
Müller und Kempf, Photometrische Durchmusterung
250
B.D.
Sternzeit
I
n
m
IV
J
2
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
8 C
385
1 h 1 9™
3384
_ ,0.
33 o
3585
3685
34872
4583
9 - 5 11 1
9.5464
7
347
1 2 1
39-7
40.9
41.7
38.6
40.22
45-2
9.6201
9-6552
0.2673
— O.67
6.01
4
367
1 23
25.2
26.0
26.0
2Ó.3
25.88
48.8
9.2800
9.3246
0.0633
+ O.I 6
6.84
2
346
1 24
24-5
20.0
22.5
23.0
22.50
50.2
9-1657
9.2145
0.1734
+ 0-43
7.11
2
347
i 25
28.0
24.9
27.0
25.0
26.22
5°-9
9.2905
9.3416
0.0463
+ O.12
6.80
O
369
1 27
20.5
17.0
21.6
18.9
19.50
52.0
9.0470
9.1019
0.2860
+ O.72
7.40
O
370
1 28
21.9
20.1
22.5
23.1
21.90
52.9
9-1434
9.2016
0.1863
+ 0.47
7-15
IO
168
1 30
23.0
21.0
24.7
21.8
22.62
41-5
9.1700
9- 1 9 7 1
8
385
1 32
36.2
35 -o
374
37-6
36.55
44.6
9.5498
9-5835
Mittel aus den Vergleichsternbeobachtungen : 9.378
3 ; 9 - 395 1 ; 9-3903-
Zur Reduction benutzt: 9.3879.
Zone 313. 1889 Januar g.
Beobachter: Müller.
Photometer :
D. Vergleichsterne: Nr. 48 und Nr.
2. Luft:
1.
9 f
5277
1 b 3 8 m
2 5?o
2I?3
2484
2 2?7
23835
4980
9.1962
9.2414
9
47
1 41
32.6
29.6
30.8
31-7
3 1 - I 8
45-6
9.4282
9.4642
IO
4958
1 43
18.8
18.6
18.0
18.4
18.45
49.9
9.0007
9.0486
O.2929
4 0-73
7-25
IÓ
4954
1 45
27.0
27.2
27-3
26.4
26.98
44.6
9-3135
9.3472
O.OO57
0.0 I
6.51
17
4956
1 46
19.7
17.4
20.2
18.0
18.82
43-2
9 -OI 73
9.0478
O.2937
4 - 0.73
7-25
19
5129
1 48
15.0
13.6
16.7
14.9
15-05
41.6
8.8288
8.8561
0.4854
+ 1.2 I
7-73
19
5138
1 49
16.6
14.2
13.8
14.2
14.70
41.6
8.8088
8.8361
0.5054
4 I. 2 Ó
7.78
19
5 H 7
i 51
21.0
24.2
25.8
22.9
23.48
4 i -3
9.2007
9.2275
0.1140
+ O.29
6.81
9
5277
i 52
24.8
22.5
244
24.1
23-95
50-5
9.2169
9.2667
9
47
i 54
31.2
28.7
31-7
27.7
29.82
46.6
9-3932
9.4318
17
4964
i 56
17-3
16.7
18.3
18.0
I 7-58
43-7
8.9601
8 - 99 1 7
0.3498
4- 0.87
7-39
15
4872
1 58
27-3
26.9
27.5
26.0
26.92
46.0
9 - 3 ii 7
9-3487
O.OO72
— 0.02
6.50
12
5022
i 59
18.7
1 5-7
17.0
16.4
16.95
48.6
8.9294
8-9734
O.3681
+ 0.92
7-44
16
5003
2 0
16.0
154
16.0
14.0
15-35
44.2
8.8456
8.8784
O.4631
+ i . 1 6
7.68
IO
5004
2 1
42.8
43 -o
43-5
43 -i
43.10
50.0
g.6692
9.7174
0-3759
— 0.94
5-58
*h 1
2 3
13.0
10.9
11.2
10.5
11.40
49-3
8.5918
8.6379
O.7036
+ 1.76
8.28
\
2 4
1 7*4
15.8
17.8
14.6
16.40
49.4
8.9015
8.9479
O.3936
+ 0.98
7-50
9
5277
2 6
21.8
22.5
24.0
20.5
22.20
52.0
9.1546
9.2095
9
47
2 7
32.8
30.0
28.0
28.6
29.85
47-7
9.3940
9-4355
Mittel aus den Vergleichsternbeobachtunge
n: 9-35 2 8; 9 3493 ; 9-3225.
Zur Reduction benutzt: 9.3415.
*) ii° 5068 dupl. Zuerst die vorangehende Componente gemessen.
Zone 314. 1889 Januar g.
Beobachter: Kempf.
Photometer:
13 . Vergleichsterne: Nr. 48
und Nr. 2. Luft: 1
9 C
47
2 h IO m
3 2?6
3185
3685
3388
33860
48?o
9.4861
9.5284
9
5277
2 12
27.6
25.0
26.9
25-3
26.20
52.7
9.2899
9-3474
15
47
2 13
23.6
23.0
244
21-5
23.12
43-7
9.1880
9.2196
O.1850
+ 0.46
6.98
IO
31
2 15
20.8
19-5
22.4
20.5
20.80
48-5
9.1007
9 -H 44
0.2Ó02
4- 0.65
7- 1 7
10
32
2 1Ó
26.0
24.0
25.0
21.5
24.12
48-5
9.2227
9.2664
O.I382
4-0.35
6.87
17
33
2 17
15.0
15.0
1 7.0
15.0
15-50
42.0
8.8538
8.8819
O.5227
+ I- 3 1
7-83
11
44
2 19
18.5
15-5
174
18.0
17-35
47-3
8.9491
8.9895
0.4151
4 - 1.04
7-56
12
25
2 20
30.5
26.0
29.O
294
28.72
46.5
9-3635
9.4018
0.0028
+ 0.01
6-53
9
5277
2 22
26.5
24.0
25.1
254
25-25
53-9
9.2600
9.3221
9
47
2 24
30-5
30.9
31-1
32.5
31-25
49-3
9.4300
9.4761
13
46
2 2Ó
254
23.6
30.0
26.9
26.48
46.3
9.2985
9-3363
O.0683
4- 0.17
6.69
! 9
64
2 28
25.0
22.5
25-5
23.6
24-15
41.2
9.2237
9-2503
0.1543
4- 0.39
6.91
18
51
2 29
27.6
26.5
30.1
26.5
27.68
41.6
9-3340
9 - 36 i 3
O.O433
4- 0.11
6.63
*9
73
2 3 1
18.0
15-9
18.7
174
i 7 - 5 o
40-7
8-9563
8.9820
O.4226
4- 1.06
7-58
15
59
2 32
24.4
23.0
28.0
24.9
25.08
45 -oj
9-2545
9.2891
O.II 55
+ 0.29
6.81
15
63
2 33
31.8
33 -i
35-2
34-5
33-65
44.8
9.4872
9 - 52 I 3
O. I I 67
— 0.29
6.23
9
47
2 34
32.5
30.0
33-5
28.4
31.10
50.4
9.4262
9-4757
9
5277
2 36
23-9
24-5
24.9
21.5
23.70
55-6
9.2083
9.2776
Mittel aus den Vergleichsternbeobachtungen: 9.4379; 9.3991; 9.3767. Zur Reduction benutzt: 9.4046.
