180
Müller und Kempf, Photometrische Durchmusterung
180
B.D.
Sternzeit
I
II
III
IV
J
0
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
,
Zone 137. 1887 April 10.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 20 und Nr. 22. Luft: 1
—2.
9 °
2374
ll h
Ol
00
3
33°5
3886
3885
3585
36852
4688
9.5492
9-5883
9
2239
12
0
18.0
16.7
18.6
16.1
17-35
51.6
8.9491
9.0026
17
2156
12
2
15.2
14.0
16.4
15-2
15.20
43-7
8.8372
8.8688
0.4287
+ 1.07
7-63
11
2134
12
4
13.6
15-9
144
14-5
14.60
48.6
8.8030
8.8470
0.4505
4 -1.13
7.69
11
2136
12
5
15-7
15.6
17.0
15.6
15.98
49.2
8.8796
8.9254
0.3721
+ 0.93
7-49
16
2059
12
6
12.4
13.0
14.6
13-5
I 3-38
444
8.7287
8.7619
0.5356
4- 1-34
7.90
IO
2100
12
8
17.0
17.4
1 7-5
16.6
17.12
49-5
8.9378
8.9845
0.3130
4-0.78
7-34
12
2138
12
10
15.0
1 5-5
16.0
154
1548
48.1
8.8527
8.8953
0.4022
4- 1.01
7-57
9
2239
12
11
17.0
17.0
19.0
17.8
17.70
52.9
8.9658
9.0240
9
2374
12
13
36.1
37 *o
404
37-5
37-75
48.1
9.5738
9.6164
16
2077
12
15
23-9
21-5
24.0
24.0
23-35
44.8
9.1962
9.2303
0.0672
4-0.17
6-73
13
2206
12
16
14.1
16.1
15.0
15-9
15.28
474
8.8417
8.8824
0.4151
4- 1.04
7.60
15
2167
12
18
15.0
16.1
17-5
15-3
15.98
45-5
8.8796
8.9154
0.3821
4- 0.96
7-52
19
2307
12
20
18.5
18.9
21.1
19.0
19.38
42.6
9.0418
9.0711
0.2264
4-0.57
7- I 3
IO
2116
12
22
1 7 - 1
17-3
16.7
18.0
17.28
50.6
8.9456
8-9957
0.3018
+ 0.75
7 - 3 i
14
2217
12
23
21.2
25-5
28.4
25.2
25.08
47-2
9-2545
9.2946
0.0029
4- 0.01
6-57
9
2239
12
25
15-9
16.0
18.0
16.4
16.58
54-5
8.9108
8-9754
9
2374
12
27
31.6
33 -o
37-7
40.4
35-68
49-4
9 . 53 I 7
9-5781
Mittel aus den Vergleichsternbeobachtungen: 9.2955; 9.3202; 9.2767.
Zur Reduction benutzt: 9.2975.
Zone 138. 1887 April 11.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 20 und Nr. 22. Luft:
I.
9 °
2239
i 4
3 ° m
iö?o
1488
1583
1680
15852
4886
8.8549
8.8989
9
2374
11
32
29.4
304
29.7
27.7
29.30
45 -o
9-3793
9 - 4 I 39
13
2128
11
34
17.8
17.6
19-3
174
18.02
46.1
8.9809
9.0182
0.1308
4-0.33
6.89
13
2131
11
35
16.6
15.6
17.O
15-7
16.22
45-6
8.8922
8.9282
0.2208
4-0.55
7.n
13
2136
11
36
17.6
16.5
18.O
154
16.88
45-8
8.9259
8.9624
0.1866
4-0.47
7.03
2134
11
37
15-3
1 5-7
16.5
15.6
I 5-78
45-2
8.8689
8.9040
0.2450
4- 0.61
7- 1 7
14
2136
11
39
34.4
32.3
35-8
34-3
34.20
44.8
9.4996
9-5337
0.3847
— 0.96
5.60
l 9
2251
11
40
21.8
21.4
22.4
21.4
2 i -75
40.6
9-1377
9.1632
0.0142
— 0.04
6.52
9
2239
11
42
16.6
1 5-5
18.0
13.6
I 5-92
49.8
8.8765
8.9241
9
2374
11
44
27-3
27.7
27.6
28.8
27.85
45-8
9 - 339 °
9-3755
*9
2254
11
45
18.6
19.0
18.4
17.2
18.30
41.1
8.9938
9.0202
0.1288
4-0.32
6.88
12
2090
11
47
314
28.7
30.5
324
30.75
47-5
9.4174
94583
0.3093
— 0.77
5-79
12
2095
11
48
1 9-5
20.0
21.2
19.8
20.12
47-7
9.0731
9.1146
0.0344
4- 0.09
6.65
12
2105
11
50
16.7
16.0
16.9
15-7
16.32
47. 1
8.8974
8-9373
0.2 I I 7
4-0.53
7.09
13
2164
11
52
21.7
20.8
21.3
20.7
21.12
46.4
9-“34
9-1514
0.0024
-—- 0.0 I
6-55
18
2274
11
53
11.2
10.5
12.6
11.8
11.52
42.3
8.6008
8.6295
0.5195
4 - 1-30
7.86
9
2239
11
55
16.8
144
15-3
14.1
I 5 -I 5
5 1 - 1
8.8344
8.8861
9
2374
11
56
29-3
28.4
28.0
28.2
28.48
46.7
9-3567
9-3955
Mittel aus den Vergleichsternbeobachtungen: 9.1564; 9.1498; 9.1408.
Zur Reduction benutzt: 9.1490
Zone 13g. 1887 April 11.
Beobachter: Kempf.
Photometer:
1). Vergleichsterne: Nr. 20 und Nr.
22. Luft:
I.
9 f
'2374
11 1
l 59 m
33 ?!
37?5
3589
3583
35 ( -45
4689
9.5269
9.5662
9
2239
12
1
20.2
194
22.0
18.5
20.02
5 i -7
9.0689
9.1227
16 2098
12
2
I7.4
1 7-5
20.0
18.2
18.28
42.2
8.9929
9.0214
O.2725
4- 0.68
7.24
18 2338
1 2
5
20.7
20.7
23-9
20.5
21-45
40.8
9-i263
9 .I 52 I
0.1418
4-0.35
6.91
18
2345
12
6
17-5
19.6
20.0
19-3
I9.IO
40.6
9.0297
9-0552
0.2387
+ 0.60
7.16
18
2352
12
7
12.9
14.1
13.8
13.0
1345
40.6
8.7332
8.7587
0.5352
4 - 1.34
7.90
13
22 37
12
8
18.2
18.0
17.6
17-5
I 7.82
45-5
8 - 97 1 5
9.0073
0.2866
4~ 0.72
7.28
15
2192
12
10
24.6
27.0
24.0
25-9
2548
43-2
9.2642
9.2947
0.0008
0.00
6.56
9
2239
12
12
17.4
16.6
18.5
16.0
17.12
53 -o
8.9378
8.9964
