160
Müller und Kempf, Photometrische Durchmusterung
160
B.D.
Sternzeit
I
11
111
IV
J
lüg sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grosse
Zone 87
1887 Februar 13
Beobachter: Müller.
Photometer:
D. Verglcichsterne: Nr. io
und Nr.
12. Luft:
1.
11°
632
43
1 7?6
15°°
I 787
17?o
16882
43-7
8.9229
8-9545
IO
8l8
5
45
26.4
28.4
28.0
25.6
27.10
42.3
9-3171
9-3458
5
899
5
47
Ho
14.8
15.8
i 5-5
15-15
47-5
8.8344
8.8753
0.2904
+ O.73
7.18
5
905
5
49
17.0
17.6
18.2
18.4
1 7.80
47.6
8.9706
9.0118
0.1539
+ O.38
6.83
3
872
5
5 i
12.6
11.8
15.O
12.7
13.02
49-5
8-7055
8.7522
04135
+ 1-03
7.48
3
864
5
53
12.5
11.4
13.O
12.9
12.45
49.6
8.6673
8 - 7 1 43
O.4514
+ I.I 3
7.58
2
947
5
55
20.6
20.0
19-5
19.7
19-95
50.6
9.0660
9.1161
O.O496
4-0.12
6-57
O
1056
5
56
21.5
20.4
19.4
20.4
20.42
52-5
9.0854
9.1421
0.0236
4- 0.06
6.51
6
923
5
58
18.8
16.6
18.5
19.0
18.22
46.2
8.9901
9.0276
O.1381
+ 0.35
6.80
IO
818
6
0
27.1
29.9
294
274
28.45
42.6
9-3559
9-3852
11
632
6
2
16.8
18.5
18.6
14.8
17.18
45-2
8.9407
8.9758
3
903
6
4
15.0
15.8
17-5
17-3
16.40
49-5
8.9015
8.9482
O.2175
+ 0.54
6.99
4
949
6
5
20.0
21.7
22.3
21.9
21.48
49.0
9- I2 74
9.1726
0.0069
— 0.02
6-43
3
948
6
7
16.3
16.6
16.6
16.4
16.48
49.9
8.9057
8-9536
O.2121
+ 0.53
6.98
2
965
6
11
19-3
J 7-5
20.2
20.0
19.25
51.2
9.0362
9.0883
0.0774
+ 0.19
6.64
I
1021
6
13
18.0
17-3
18.4
18.4
18.02
52.3
8.9809
9.0369
0.1288
4-0.32
6-77
I
1032
6
14
254
25-7
26.4
26.2
25.92
5 i -7
9.2812
9-3350
O.1693
— 0.42
6.03
IO
818
6
16
26.7
31.6
29.0
27.7
28.75
43-2
9-3643
9.3948
I I
632
6
19
1 5-5
16.2
1 7-3
16.4
16.35
46.7
8.8990
8.9378
Mittel aus den Vergleichsternbeobachtungen: 9.1502; 9.1805; 9.1663. Zur Reduction benutzt: 9.1657.
Zone 88.
1887 Februar 13
#
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 14 und Nr.
16. Luft:
1.
IO°
1149
7 1
44 ™
2 7?i
2980
3082
2780
28832
45 °i
9-3523
9-3871
11
1588
7
47
26.0
25.0
24-3
24.4
24.92
4 i -5
9.2493
9.2764
5
I 5 H
7
49
22.1
20.5
21.4
22.5
21.62
47-9
9.1328
9.1748
0.12x8
4- 0.30
6.77
9
1496
7
5 i
26.6
25-5
29.O
2 8.8
27.48
44-5
9.3282
9.3616
O.065O
— 0.16
6.31
9
1510
7
53
33 -o
30.7
29.O
35 -o
31.92
44.4
9.4465
9.4797
O.183I
— 0.46
6.01
2
1530
7
56
18.4
15.8
22.5
18.1
18.70
51.2
9.0120
9.0641
O.2325
4- 0.58
7-05
I
1665
7
58
18.4
19.7
20.5
19-5
19.52
52.2
9.0479
9-1035
O.I931
4- 0.48
6-95
5
1543
7
59
25.0
24-5
27-3
27.0
25-95
48.8
9.2822
9.3268
O.O302
— 0.08
6-39
IO
1149
8
1
26.0
24.7
2 8.6
28.5
26.95
46.5
9.3126
9-3509
11
1588
8
4
22.5
22.0
23.0
2 7.2
23.68
42.1
9.2076
9-2359
9
1539
8
6
19-5
19.8
2 2.0
19.6
20.22
44-7
9.0772
9.1111
O.1855
+ 0.46
6-93
7
1618
8
7
19.6
19.4
21.4
20.9
20.32
46.3
9.0813
9.1191
0-1775
4-0.44
6.91
3
1584
8
9
20.1
19-5
22.1
24.6
21.58
50.7
9.1312
9.1816
O.II5O
4-0.29
6.76
3
1609
8
11
33-9
36.0
38.O
41.1
37-25
50.8
9-5639
9.6147
0.3181
— 0.80
5-67
5
1577
8
13
254
23-5
25.O
24.5
24.60
48.6
9.2388
9.2828
0.0138
4-0.03
6.50
5
1580
8
14
24.4
23.8
24.4
28.2
25.20
48.7
9.2584
9.3027
0.0061
— 0.02
6-45
IO
1 149
8
16
25-5
24-3
27.O
26.9
25.92
47-9
9.2812
9.3232
11
1588
8
19
24-5
20.1
23-9
22.6
22.78
42.9
9-1759
9.2058
Mittel aus den Vergleichsternbeobachtungen
: 9-33i8; 9.2934; 9.2645. Zur Reduction benutzt: 9.2966.
Zone 89. 1887 Februar 13.
Beobachter: Müller.
Photometer:
1 ). Verglcichsterne: Nr. 14
und Nr. 16. Luft:
.
ii°
1588
8’
1 21 ra
2 i?o
2I?3
2380
2084
2 1842
4380
9-1251
9-1552
IO
1149
8
24
22.7
23-3
234
20.7
22.52
48.6
9.1664
9.2 104
8
1712
8
26
28.7
27-3
28.6
26.0
27.65
46.8
9-3332
9-3723
0.2102
— 0.53
5-94
o
1871
8
28
18.4
18.9
20.6
19.6
19.38
54-9
9.0418
9.1081
0.0540
4-0.14
6.61
6
1594
8
30
174
16.5
174
18.4
17.42
48.3
8-9525
8-9957
0.1664
+ 0.42
6.89
7
1684
8
32
26.0
234
26.O
26.4
25-45
47.8
9.2664
9.3082
0.1461
— 0.37
6.10
9
1603
8
34
16.8
15-7
20.3
16.4
I 7-30
46.1
8.9466
8.9839
0.1782
+ o -45
6.92
2
1640
8
36
24.6
24-5
24.2
24.6
24.48
52.4
9.2348
9.2912
0.1291
— 0.32
6.15
I I
1588
8
38
19.6
21.7
: 9-7
2 1.0
20.50
44.1
9.0887
9.1212
