268
Müller und Kempf, Photometrische Durchmusterung
268
B.D.
Sternzeit
i ;
II
111
IV
J
z
log sin' 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
ii°
632
2 h
5 m
20?6
1984
2I?5
21 ? 1
20865
5084
9-°947
9.1442
i 7
666
2
7
32.0
28.7
28.3
30.8
29-95
40.4
9.3966
9.4217
0.4004
— 1.00
6.25
17
676
2
8
2 1.0
19.4
19.6
20.5
20.12
41-3
9.0731
9.0999
0.0786
— 0.20
7-05
19
643
2
9
23-5
18.6
21.4
19.9
20.85
38.4
9.1027
9.1244
0.1031
— O.26
6.99
18
581
2
11
I4.O
11.9
13.6
12.5
13.00
39-7
8.7042
8.7281
0.2932
•+■ 0-73
7.98
657
2
12
25-5
25-5
25-5
27.4
25.98
43-3
9.2831
9 - 3 I 39
0.2926
— 0.73
6.52
16
559
2
13
13-7
12.0
14.0
I 3 -I
13.20
42.1
8.7172
8-7455
0.2758
-j- 0.69
7-94
9
472
2
!5
16.0
14.7
16.9
15-5
15-78
45-8
8.8689
8.9054
11
632
2
17
20.5
19.4
20.8
21.0
20.42
49.1
9.0854
9.1309
Mittel aus den Vergleichsternbeobachtungen: 9.0113; 9.0344; 9.0182.
Zur Reduction benutzt: 9.0213.
Zone 358.
1889 November 14.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 40 und Nr. 42. Luft:
2.
IO°
3981
2 2 U
2 m
i 9?9
i8?7
l8?l
i6?4
18828
5184
8.9929
9-0457
IO
4351
22
4
22.0
21.9
19.4
17.6
20.22
45-3
9.0772
9 -i 125
14
4149
22
7
9-5
8.2
10.4
8.5
9-15
45-2
8.4029
8.4380
0.6205
+ i -55
8-35
H
4150
22
9
18.5
17.4
19.7
20.6
19.05
46.2
9.0275
9.0650
0.0065
— 0.02
6.78
14
4158
22
11
18.9
15-6
17-5
16.8
1 7.20
45-9
8.9417
8.9785
0.0800
-j- 0.20
7.00
15
4040
22
12
22.5
23.8
23.0
20.4
22.42
45-4
9.1627
9.1983
0.1398
— 0.35
6-45
15
4038
22
13
15.8
12.4
12.6
12.9
13.42
45-2
8-7313
8.7664
0.2921
+ 0.73
7-53
16 4118
22
15
12.6
10.6
11-5
11-5
n -55
44.8
8.6030
8.6371
0.4214
+ 1-05
7.85
IO
3981
22
17
16.9
15.2
16.8
17-7
16.65
53-2
8.9144
8.9738
IO
4351
22
!9
20.1
18.5
I 9-9
19-5
19.50
46.6
9.0470
9 -o 855
18 4365
22
21
27.2
27.0
25-5
27.1
26.70
44.1
9-3051
9-3376
0.2791
— 0.70
6.10
l 7
4201
22
23
17-5
15-5
16.4
16.3
16.42
44-5
8.9025
8-9359
0.1226
+ 0.31
7.11
17 4206
22
24
17-5
13.6
16.2
17-5
16.20
45 -o
8.8912
8.9258
0.1327
+ 0.33
7-13
16
4119
22
25
16.9
15-9
16.0
16.4
16.30
45-7
8.8964
8.9327
0.1258
+ 0.31
7 - 1 1
12
4209
22
28
12.9
11.0
13.6
11.9
12-35
49-5
8.6604
8.7071
0.3514
+ 0.88
7.68
13
4259
22
29
15-3
13.2
14.0
13-5
14.00
49.0
8.7674
8.8126
0.2459
-j- 0.61
7.41
IO
3981
22
31
19-5
16.8
16.2
17.0
17-38
55 -o
8.9505
9.0172
IO
4351
22
33
21.0
19.0
19-5
21.1
20.15
47-9
9.0744
9.1164
Mittel aus den Vergleichsternbeobachtungen: 9.0791; 9.0297; 9.0668.
Zur Reduction benutzt: 9.0585.
Zone
359 -
1889 November 14.
Beobachter:
Müller. Photometer
D. Vergleichsterne: Nr. 4
und Nr. 6. Luft: 2.
IO C
168
23’
34 m
i6?7
I4?0
i6?o
1487
15-35
4681
8.8456
8.8829
8
385
23
36
21.0
2 I .O
20.0
20.0
20.50
55 -o
9.0887
9-1554
18
277
23
39
26.9
25-3
25.6
22.0
24-95
43-8
9-2503
9.2822
0.2783
— 0.70
5 - 9 8
18
283
23
40
16.2
12.4
15.2
13-9
14.42
43-9
8-7925
8.8246
0-1793
+ o -45
7-13
19
340
23
41
27.6
27.8
26.9
26.1
27.10
44.1
9-3171
9.3496
0.3457
— 0.86
5.82
19
342
23
43
15.6
14.1
I 5 - 1
13.6
14.60
44.1
8.8030
8-8355
0.1684
-f- 0.42
7.10
13
351
23
44
14-5
12.4
14-3
13.0
13-55
48.3
8.7396
8.7828
0.22 I I
+ 0.55
7-23
14
357
23
46
28.0
25-7
26.5
27.2
26.85
46.8
9.3096
9-3487
0.3448
— 0.86
5.82
IO
168
23
48
16.7
13-5
15.8
14.0
15.00
45 -o
8.8260
8.8606
8
385
23
50
21.4
19.0
20.7
19-5
20.15
53-3
9.0744
9 - 134 I
17
339
23
52
13-5
10.8
12.3
10.4
ii -75
44.0
8.6178
8.6501
0.3538
+ 0.88
7-56
12
315
23
54
10.0
8.0
8.7
8.1
8.70
48.2
8-3595
8.4024
O.601 5
+ 1-50
8.18
12
317
23
55
I 5-7
14.4
14.8
13-5
14.60
48.5
8.8030
8.8467
O.I572
+ 0.39
7.07
16
281
23
57
15.2
12.1
16.3
13-4
14.25
45-2
8.7824
8.8175
O.1864
+ 0.47
7-15
16
283
23
58
12.5
9.0
12.1
10.4
11.00
44.6
8.5612
8-5949
O.4O9O
+ 1.02
7.70
14
392
23
59
10.4
8.2
9.2
9.2
9-25
46.4
8.4123
84503
0.5536
+ 1-38
8.06
IO
168
O
1
16.0
13.2
15-7
13-9
14.70
44.0
8.8088
8.8411
8
385
0
3
20.4
19.7
22.0
20.5
20.65
51-9
9.0947
9.1492
Mittel aus den Vergleichsternbeobachtungen: 9.0192; 8.9973; 8.9952. Zur Reduction benutzt: 9.0039
