270
Müller und Kempf, Photometrische Durchmusterung
270
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
IO°
4351
2 2 h
17 m
2 I?2
1984
2I?3
1981
20825
4683
9.0785
9-IIÓ3
15
4137
22
20
I9.O
18.3
I7.9
17.1
18.08
44.6
8.9837
9- OI 74
0.0315
4~ 0.08
6.88
14 4268
22
2 I
20.0
18.1
17-3
16.9
18.08
45-o
8.9837
9- oi8 3
0.0306
+ 0.08
6.88
14 4263
22
22
23.2
22.1
24.6
21.0
22.72
45-8
9-1737
9.2102
0.1613
— 0.40
6.40
13
4355
22
23
I5.6
12.8
134
13.0
1370
46.2
8.7489
8.7864
0.2625
4- 0.66
7.46
13
4356
22
24
I 7.O
15-7
l6.8
154
16.22
46.3
8.8922
8.9300
0.1189
+ 0.30
7.10
13
4371
22
27
11*9
12.5
I3.6
11 *5
12.38
47.0
8.6624
8.7020
0.3469
+ 0.87
7.67
IO
3981
22
29
17.1
15.6
16.7
16.4
16.45
54-8
8.9041
8.9700
IO
4351
22
31
21.0
19-9
I9.7
19-7
20.08
47.6
9-0715
9.1127
Mittel aus den Vergleichsternbeobaehtungen: 9.0374; 9.0680; 9.0413.
Zur Reduction benutzt: 9.0489.
Zone 363.
1889 November 22.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42.
Luft: 1-
—2.
IO C
3981
2 0 h
54 m
2 I?2
i5°4
2o?5
1588
18822
4487
8.9901
9.0240
IO
4351
20
55
2I.9
20.0
23-5
18.4
20.95
41.7
9.1067
9.1342
3
4065
20
57
l6.2
13-5
154
13.0
14.52
52.2
8.7984
8.8540
0.2387
+ 0.60
7.40
5
4190
20
58
20.6
18.4
22.0
19.9
20.22
50.7
9.0772
9.1 276
0.0349
— 0.09
6.71
5
4209
2 1
0
I9.4
17.2
2 I. I
16.8
18.62
50.1
9.0084
9.0569
0.0358
4- 0.09
6.89
7
4130
2 I
2
I 2.2
11.0
12.3
11.2
11.68
48.7
8.6126
8.6569
0.4358
+ 1.09
7.89
7
4133
21
3
17.2
154
154
15-1
15-78
48.8
8.8689
8-9I35
0.1792
+ o-45
7-25
2
3932
2 I
4
2 I .O
19.0
2 I.9
19.0
20.22
53-4
9.0772
9- 1 3 73
0.0446
— 0.11
6.69
IO
3981
2 I
6
18.4
16.6
l8.8
17.0
17.70
45-7
8.9658
9.0021
IO
4351
2 I
7
23-4
20.3
23.O
18.4
21.28
42.0
9.1196
9.1477
0
4265
2 I
11
I4.6
12.4
I4.4
11.8
13-30
56.2
8.7236
8.7956
0.2971
4-0.74
7-54
3
4097
2 I
13
24.O
194
2 1.8
20.0
21.30
53-5
9.1204
9.1809
0.0882
— 0.22
6.58
7
4175
2 I
14
I4.6
12.0
15-5
12.8
13-72
49.4
8.7501
8.7965
0.2962
4- 0.74
7-54
8
4190
21
16
i8.2
154
17-3
15-9
16.70
48.7
8.9169
8.9612
0-1315
+ 0.33
7-13
9
4233
2 I
17
23-3
19-5
2O.4
18.2
20.35
47-5
9.0826
9-1235
0.0308
— 0.08
6.72
4
4210
2 I
19
13.2
11.6
I4.6
12.9
13.08
52.0
8.7094
8.7643
0.3284
4- 0.82
7.62
IO
398 i
21
20
20.8
18.0
20.7
17.1
19-15
47.0
9.0319
9-0715
IO
4351
2 I
22
24.1
20.3
23.O
20.6
22.00
42.6
9.1472
9-1765
Mittel aus den Vergleichsternbeobachtungen: 9.0791; 9.0749; 9.1240. Zur Reduction benutzt: 9.0927.
Zone 364.
1889 November 22.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42
. Luft: 1
—2.
IO C
*4351
2 l h
2 6 m
2580
20?4
2486
2280
23800
4288
9- i8 38
9-2135
IO
3981
2 1
29
20.4
18.7
20.0
19.4
19.62
47.8
9.0521
9.0939
IO
4180
21
31
1 6.7
154
16.1
15.0
15.80
45-4
8.8700
8.9056
0.2527
+ 0.63
7-43
IO
4189
2 1
32
22.5
19-5
20.4
18.6
20.25
45-7
9.0785
9.1148
0.0435
4- 0.11
6.91
IO
4192
21
33
12.5
11.1
12.4
12.5
12.12
45-6
8.6443
8.6803
0.4780
4- 1.19
7-99
12
4225
2 1
35
16.0
13-5
15.O
14-3
14.70
44.2
8.8088
8.8416
0.3167
4-0.79
7-59
12
4226
2 1
37
14.7
13.8
16.O
14.2
14.68
44.1
8.8076
8.8401
0.3182
4- 0.80
7.60
12
4229
21
38
16.4
14-5
154
16.0
15-58
43-8
8.8581
8.8900
0.2683
4-0.67
7-47
IO
3981
21
40
20.6
18.5
19.4
18.9
19-35
49.0
9.0406
9.0858
IO
4351
2 1
43
25.O
22.0
23.6
23.0
23.40
43-8
9 .Ì 979
9.2298
15
4047
2 1
46
14.1
11.9
13-9
1 1-5
12.85
42.1
8.6943
8.7226
0-4357
4- 1.09
7.89
l6
4150
2 1
47
i8.2
16.0
16.9
: 5-5
16.65
41.6
8.9144
8.9417
0.2 166
+ 0.54
7-34
l6
4153
2 1
48
24.9
22.7
24.1
26.1
24-45
41.6
9-2338
9.2611
0.1028
— 0.26
6-54
l6
4162
2 1
50
l8.0
17*5
18.O
19.0
18.12
41-5
8-9855
9.0126
0.1457
4- 0.36
7.16
I I
4153
2 1
51
17-5
15.0
16.4
14-5
15-85
45-8
8.8727
8.9092
0.2491
4- 0.62
7.42
l8
4402
2 1
53
19-5
15*5
20.0
18.0
18.25
39-8
8.9915
9.0156
0.1427
+ 0.36
7.16
IO
3981
2 1
55
20.5
19.4
2O.9
20.0
20.20
50.6
9.0764
9.1265
IO
4351
2 1
57
23.6
23.0
22-5
21.0
22.52
44.8
9.1664
9.2005
Mittel aus den Vergleichsternbeobachtungen: 9.1537; 9.1578; 9.1635.
Zur Reduction benutzt: 9.1583.
