284
Müller und Kempf, Photometrische Durchmusterung
284
B.D.
Sternzeit
I
II
III
IV
/
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
io° 398 i
20 1 * l6 m
2486
23?2
23-4
2I?5
23818
4285
9.1902
9-2193
8 4007
20 18
22.5
19-5
22.6
20.1
21.18
45-7
9-1157
9.1520
0.1 102
4 0.28
7.12
7 4002
20 20
17.7
15.6
18.7
15-5
16.88
47.1
8.9259
8.9658
O.2964
+ O.74
7-58
9 4039
20 21
21.6
19.0
22.0
I9.O
20.40
44.8
9.0846
9.1187
0.1435
+ O.36
7.20
0 4158
20 23
18.5
14.0
15.8
14.1
15.60
54-2
8.8592
8.9225
0-3397
+ 0.85
7.69
0 4166
20 25
23.0
21.3
23.1
23-3
22.68
54-3
9-I723
9.2360
0.02Ó2
+ O.07
6.91
1 3960
20 26
31.6
28.0
29.4
27.7
29.18
52.9
9.3761
9-4343
O.I721
— 0.43
6.41
10 3573
20 29
28.0
24.4
24-5
24-5
25-35
48.0
9.2632
9-3055
10 3981
K>
0
24.2
22.5
22.6
22.0
22.82
43-2
9- 1 773
9.2078
Mittel aus den Vergleichsternbeobachtungen : 9.2616; 9.2684; 9.2567.
Zur Reduction benutzt: 9.2622.
Zone 398.
1890 September 20.
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 36 und Nr. 38. Luft: 1
—2.
9°«34 2 4
i8 h 47 m
32?3
31^3
3185
2982
31808
45-5
9-4257
9.4615
10 3573
18 50
23-9
21.4
24.4
22.0
22.92
41.8
9.1809
9.2086
6 3593
18 53
21.5
18.4
20.0
19-3
19.80
47-3
9-0597
9.1001
O.2505
4- 0.63
7.01
6 3597
18 54
26.1
22.6
24.6
23.2
24.12
47.6
9.2227
9.2639
O.0867
4- 0.22
6.60
8 3555
18 56
19.9
17.8
2 1.3
174
19.10
45-2
9.0297
9.0648
O.2858
4 0.71
7.09
8 3567
18 58
1 7-i
16.0
l8.8
15.0
16.72
45-6
8.9179
8-9539
0.3967
4 0.99
7-37
9 3534
19 i
20.5
18.3
20.0
20.5
19.82
44.8
9.0605
9.0946
O.2560
4 0.64
7.02
1 3578
19 3
28.3
24.8
28.0
25-7
26.70
52.2
9-3051
9.3607
O.OIOI
— 0.03
6-35
9 3424
19 5
33-8
34-3
29.8
32.2
32-52
46.9
9.4609
9.5002
10 3573
19 8
22.4
21.0
24.8
23-5
22.92
42-3
9.1809
9.2096
4 3589
19 IO
2 1.2
18.4
2 1.6
18.6
19-95
49.8
9.0660
9-II36
0.2370
4- 0.59
6.97
2 3493
19 13
24.1
21.0
23-4
21.7
22.55
52.0
9-i675
9.2224
0.1282
4- 0.32
6.70
2 3498
19 15
23-3
19-3
2 1.2
20.5
21.08
52.4
9.1118
9.1682
0.1824
4 0.46
6.84
6 3626
19 17
19.7
15.0
18.O
174
17-52
48.2
8-9573
9.0002
0.3504
4 0.88
7.26
6 3627
19 18
13.6
10.5
13-9
11-3
12.32
48.4
8.6583
8.701 7
0.6489
4 1-62
8.00
9 3567
19 21
21-5
19.6
20.8
21.6
20.88
45-4
9.1039
9-1395
0.21 I I
4- 0.53
6.91
9 3424
19 23
33-8
31.6
31 • i
314
31.98
48.6
9-4479
9.4919
10 3573
19 25
25-1
22.8
23.8
22.3
23-50
43-i
9.2014
9-23I7
Mittel aus den Vergleichsternbeobachtungen : 9.3351; 9.3549; 9.3618. Zur Reduction benutzt: 9.3506.
Zone
399 .
1890 September 20.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 36 und Nr. 38. Luft:
—2.
9°3424
I9I1
35-9
3083
2988
2 886
31815
4989
9-4275
9-4754
10 3573
19 38
26.5
22.0
21.9
22.7
23.28
43-8
9-1937
9.2256
10 3438
19 40
19.0
16.4
17-3
16.1
17.20
45-5
8.9417
8-9775
O.3792
+ o-95
7-33
ii 3415
19 43
19.0
16.3
18.3
15.6
17.30
44-5
8.9466
8.9800
0.3767
+ 0.94
7-32
12 3446
19 45
18.5
15-1
15-7
16.2
16.38
44-5
8.9005
8-9339
O.4228
4- 1.06
7-44
12 3456
19 51
12.9
10.0
13-i
11.0
ii-75
44-7
8.6178
8.6517
0.7050
4 1.76
8.14
11 3417
19 53
17.2
14.9
16.8
17.2
16.52
45-6
8.9077
8-9437
O.413O
4- 1.03
7.41
13 3593
19 55
27.6
23.0
25.0
25-3
25.22
43-7
9.2590
9.2906
O.0661
4-0.17
6-55
9 3424
19 56
36.0
29.8
29.2
32.3
31.82
52.0
9.4440
9.4989
10 3573
20 0
24.9
20.7
23-9
24.2
23.42
45-4
9.1986
9.2342
18 3623
20 2
27.0
24-3
254
23.1
24-95
40.4
9-2503
9-2754'
O.081 3
4- 0.20
6.58
12 3461
20 4
22.1
18.2
19.8
19.4
19.88
45-3
9.0631
9.0984
O.2583
4 0.65
7-03
12 3467
20 6
18.8
14.0
17.8
17.1
16.92
46.1
8.9279
8.9652
0.3915
4 0.98
7-36
12 3469
20 8
14.6
13.0
13-7
13.6
13-72
46.0
8.7501
8.7871
O.5696
4 1.42
7.80
14 3486
20 11
12.8
10.8
11.8
I 1.0
11.60
44.4
8.6067
8.6399
O.7 l68
4 i-79
8.17
15 3426
20 13
19.6
17.6
17.2
19.0
18.35
43-5
8.9961
9.0273
0.3294
4 0.82
7.20
9 3424
20 15
31.8
30.1
30.2
30.0
30.52
54-3
9-4II4
9-4751
10 3573
20 18
26.0
21.1
2 2.1
23-7
23.22
47.0
9.1916
9.2312
Mittel aus den Vergleichsternbeobachtungen: 9.3505; 9.3666; 9.3531. Zur Reduction benutzt: 9.3567
