172
Müller und Kempf, Photometrische Durchmusterung
172
B.
1).
Steinzeit
I
II
m
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone X17. 1887 März 14.
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 18
und Nr. 20. Luft :
1.
IO°
1818
9 h
48"*
20?4
1784
2 2?6
1988
20805
45 ?o
9.0702
9.1048
9
2239
9
51
14-5
14.4
18.5
14-5
15.48
43-3
8.8527
8.8835
o
2313
9
53
15.8
13.6
16.3
13.6
14.82
55-2
8.8157
8.8833
0.0712
+ 0.18
7.13
6
1983
9
55
15.6
12.7
I3.6
14.9
14.20
49-7
8.7794
8.8267
0.1278
+ O.32
7.27
5
1997
9
56
25.6
27.6
25-3
24.0
25.62
50.6
9-2 7 1 7
9.3218
0.3673
— O.92
6.03
5
1999
9
58
19.6
18.8
18.2
17.7
18.58
50.0
9.0066
9.0548
0.1003
— O.25
6.70
8
2077
10
0
24.4
234
244
24.2
24.10
47-4
9.2220
9.2627
0.3082
— O.77
6.18
o
2335
10
1
13-7
12.7
1 5-6
144
14.10
55 -i
8-7734
8.8405
0.1140
+ O.29
7.24
IO
1818
IO
3
18.3
18.4
18.5
18.2
18.35
46.2
8.9961
9.0336
9
2239
IO
5
14.2
13.6
15-3
15.0
14-52
43-6
8.7984
8.8298
3
2014
IO
9
19-5
20.4
20.8
19.1
19-95
53-4
g.0660
9.1262
0.1717
— 0.43
6.52
*7
1
IO
IO
21.5
23-7
21.7
22.9
22.45
49-8
9 -Ì 639
9.2115
0.2570
— O.64
6.31
1 9971
IO
12
10.8
13.0
11.1
11-9
11.70
50.0
8.6141
8.6623
0.2922
+ 0-73
7.68
i
2142
IO
13
14.0
13.0
13.0
12.3
13.08
55-4
8.7094
8.7778
0.1767
+ O.44
7-39
8
2oqg
IO
15
19-5
18.6
19-3
18.4
18.95
48.6
9.0231
9.067 1
0.1126
— 0.28
6.67
2
203g
IO
16
15-4
154
16.6
14.6
15-50
54-4
8.8538
8.9180
0.0365
+ O.09
7-04
4
202g
IO
17
18.2
17.7
18.4
18.4
18.18
51-9
8.9883
9.0428
0.0883
0.22
6-73
IO
1818
IO
19
18.1
17.1
18.0
18.3
17.88
47.6
8-9744
9.0156
9
223g
IO
21
14.1
15.0
15.6
154
15.02
44.0
8.8271
8.8594
Mittel aus den Vergleichsternbeobachtungen: 8.9942; 8.9317; 8.9375. Zur Reduction benutzt: 8.9545.
*) 7 0 1997 dupl. Zuerst die hellere, südlichere Componente gemessen.
Zone 118. 1887 März 14.
Beobachter: ICempf. Photometer: I). Vergleichsterne: Nr. 18 und Nr. 20. Luft: 1
—2.
9 °
223g
IO 11
25 m
i6?6
1780
i 8?4
i6?4
17? IO
44?2
8.9368
8.9696
IO
1818
IO
27
20.0
21.0
24-5
19-3
21.20
48.4
9.1165
9.1600
2
22 I 7
IO
30
27.1
23-5
26.5
244
25-38
51-7
9.2642
9.3180
0.2519
— O.63
6.32
2
222 g
IO
31
17.4
174
21.0
19.1
18.72
51-7
9.0129
9.0667
0.0006
0.00
6.95
9
222Ó
IO
33
16.4
17.6
20.1
1 7-3
17-85
44-5
8-9730
9.0064
0.0597
+ 0.15
7.10
o
2546
IO
34
18.5
21.3
20.1
20.1
20.00
53-5
9.0681
9.1286
0.0625
— 0.16
6.79
3
22 ÓI
IO
36
14.0
14.6
15.2
14-9
14.68
50.7
8.8076
8.8580
0.2081
+ 0.52
7-47
4 2236
IO
37
13-5
14.0
154
144
14.32
50.0
8.7866
8.8348
0.2313
4-0.58
7-53
9
22 39
IO
39
16.1
16.1
18.0
17-5
16.92
44-9
8.9279
8.9623
IO
l8l8
IO
41
20.4
19.1
22.0
21-5
20.75
49.9
9.0987
9.1466
0
2566
IO
43
12.8
14.6
144
14-5
14.08
53-2
8.7722
8.8316
0.2345
4- 0.59
7-54
0
2573
IO
44
23.0
21.5
21.6
20.7
21.70
53-2
9- 1 358
9- 1 95 2
0.1291
— 0.32
6.63
5
224O
IO
46
22.7
23-5
26.1
25-5
24-45
49. 1
9-2338
9-2793
0.2132
— 0.53
6.42
3
228o
IO
47
24.7
25.0
27.0
274
26.02
51.0
9.2843
9-3357
0.2696
— 0.67
6.28
6
2224
IO
49
29.2
28.2
28.9
29-5
28.95
47-5
9.3698
9.4107
0.3446
— 0.86
6.09
8
2285
IO
51
17.0
15.6
18.5
17.0
17.02
45-6
8.9329
8.9689
0.0972
4- 0.24
7.19
9
2239
IO
52
1 5-5
19-5
16.5
17.0
17.12
45-6
8.9378
8.9738
IO
l8l8
IO
55
20.4
20.0
234
22.5
21.58
51-5
9-1312
9.1843
Mittel aus den
Vergleichsternbeobachtungen: 9.0648; 9.0545; 9.0790. Zur Reduction benutzt: 9.0661
Zone 119. 1887 März 15.
Beobachter: Müller. Photometer: D. Verg
[eichsterne: Nr. 10
und Nr. 12. Luft:
—2.
1 i c
632
6 u 2 6 m
1787
1 883
1983
i8?o
i8?32
47°3
8.9947
9.0351
IO
818
6
28
30.0
29.8
28.6
2 8.6
29.25
43-8
9.3780
9.4099
11
756
6
30
28.4
26.4
30.6
28.8
28.55
44.2
9-3587
9 . 39 I 5
0.1941
— 0.49
5-96
12
760
6
32
15.0
13-1
15.0
13.2
14.08
43 -i
8.7722
8.8025
0.3949
4 - 0.99
7-44
l 9
884
6
34
11-3
10.0
11-3
12.0
11 -1 5
36.3
8.5729
8.5915
0.6059
4 - I- 5 1
7.96
*)ig
886
6
35
20.2
16.5
18.2
18.7
18.40
36.3
8.9984
9.0170
0.1804
4- 0.45
6.90
**) 1 q
893
6
37
26.4
22.7
23-5
22.8
23-85
36.3
9-2135
9.2321
0.0347
— 0.09
6.36
19
898
6
39
17.1
154
18.6
16.3
16.85
36.8
8.9244
8-9437
0-2537
4- 0.63
7.08
11
632
6
41
16.6
16.7
16.0
17.4
16.68
48.9
8.9159
8.9608
