340
Müller und Kempf, Photometrische Durchmusterung
340
B.D.
Sternzeit
I
II
III
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diif. in
Grössen
Grösse
Zone 539. 1892 März 3.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 16 und Nr. 18. Luft:
2.
11°
1588
6 U 39 111
1 q?8
i6? 4
1986
1786
1 883 5
4280
8.9961
9.0242
IO
1818
6
42
18.4
15.6
19.8
18.8
18.15
47.O
8.9869
9.0265
5
1934
6
48
6.6
4.2
6.9
4.8
5.62
5°-5
7.9818
8.03 16
1.0156
4~ 2-54
9.22
4
1954
6
5i
24.4
21.0
24.9
21.3
22.90
51.0
9.1802
9.2316
0.1844
— O.46
6.22
8
2032
6
53
14.0
12.6
14.9
13.0
13.62
47.1
8-7439
8.7838
0.2634
+ 0.66
7-34
2
1948
6
56
17.2
15.6
16.7
16.3
16.45
52-7
8.9041
8.9616
0.0856
+ 0.21
6.89
5
1950
6
58
12.6
11.6
13.O
12.4
12.40
49-7
8.6638
8.7111
0.3361
-j- O.84
7-52
o
2288
7
1
12.6
10.3
11.6
11.6
11.52
54-4
8.6008
8.6649
0.3823
4~ O.96
7.64
11
1588
7
4
22.0
17.8
20.4
17.9
19.52
4i-3
9.0479
9.0747
IO
1818
7
7
20.0
17-9
19.2
16.8
18.48
44.9
9.0021
9-0365
2
1965
7
10
27.0
26.4
26.6
25.0
26.25
52.0
9.2914
9-3463
0.2991
— 0-75
5-93
8
2057
7
12
14.0
12.0
H-9
12.5
13-35
46.6
8.7268
8-7653
0.2819
+ 0.70
7-38
7
1 97 5
7
15
15-5
11.4
13.8
12.2
13.22
46.8
8.7185
8-7576
0.2896
4- 0.72
7.40
i
2102
7
17
12.8
9-5
12.4
11 -7
11.60
52.6
8.6067
8.6638
0.3834
4- 0.96
7.64
8 2064
7
20
17.0
14.9
17.4
15.2
16.12
45-5
8.8870
8.9228
0.1244
+ 0.31
6-99
0
2312
7
22
12.0
10.0
12.0
9-7
10.92
53-4
8-5550
8.6151
0.4321
+ 1.08
7.76
11
1588
7
25
21.7
18.3
19-5
18.4
19.48
41.2
9.0461
9.0727
IO
1818
7
28
18.9
18.3
19-5
18.6
18.82
43-6
9 -oi 73
9.0487
Mittel aus den
Vergleichsternbeobachtungen: 9.0254; 9.0556; 9.0607. Zur Reduction benutzt: 9.0472.
Zone 540. 1892 März 3.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 22 und Nr. 24. Luft:
2.
9°
2 374
9 1
IO m
2789
2486
2682
25-4
26802
4681
9.2843
9.3216
11
2372
9
12
18.8
17-3
18.O
16.3
1 7.60
49.2
8.9611
9.0069
12
2319
9
15
19.8
16.2
18.3
174
17.92
46.3
8.9762
9.0140
0.1690
4- 0.42
6.82
*) 1 5
2321
9
19
2 1.2
17.8
20.0
18.5
19.38
43-8
9.0418
9.0736
0.1094
+ 0.27
6.67
H
2374
9
20
l6.2
15*1
16.O
H-3
15-40
44.6
8.8483
8.8820
0.3010
4- 0.75
7-15
18
2475
9
24
15-4
13-7
14.6
13.0
14.18
40.8
8.7782
8.8040
0.3790
4- 0.95
7-35
18 2481
9
25
16.4
13.8
16.1
13-9
I5-05
40.8
8.8288
8.8546
0.3284
4- 0.82
7.22
*7
2351
9
27
I4.6
134
14-5
12.7
13.80
41.0
8-7551
8.7813
0.4017
4- 1.00
7.40
9
2374
9
30
29.I
25-7
27.1
25-3
26.80
44.8
9.3081
9.3422
11
2372
9
33
I9.6
17-3
19-5
17-9
18.58
47.0
9.0066
9.0462
18
2488
9
42
I3.6
11.2
14.1
11-5
12.60
39-4
8-6775
8.7009
0.4821
4- 1 • 21
7.61
12
2335
9
44
27.6
26.9
26.6
25.0
26.52
44-7
9.2997
9-3336
0.1506
— 0.38
6.02
J 7
2356
9
46
32.2
28.0
29.4
27.8
29-35
39-8
9.3807
9.4048
0.2218
— 0.55
5.85
12
2338
9
48
18.7
17.6
21.4
18.3
19.OO
44.0
9-0253
9.0576
0.1254
4- 0.31
6.71
16
2266
9
50
28.3
25-7
26.9
26.6
26.88
40.9
9-3105
9-3365
0-1535
— 0.38
6.02
18
2505
9
5 1
I 5-5
12.6
13.8
14.1
14.00
38.7
8.7674
8.7896
0-3934
4- 0.98
7-38
11
2376
9
54
19-3
16.7
18.9
17-3
18.05
45-o
8.9823
9.0169
0.1661
4- 0.42
6.8 2
11
2372
9
55
19.2
17.9
18.9
1 7-5
18.38
45-o
8-9975
9.0321
9
2374
9
57
29-3
26.0
26.4
26.7
27. IO
43-7
9-3i7i
9-3487
Mittel aus den Vergleichsternbeobachtungen: 9.1643; 9.1942; 9.1904.
Zur Reduction benutzt: 9.1830.
*) 1502321 dupl., sehr eng. Als
ein Stern gemessen.
Zone 541. 1892 März 4.
Beobachter:
Kempf.
Photometer:
D. Vergleichsterne: Nr. 8 und Nr. 10. Luft: 2.
9 C
472
5 1
l -y 111
i6?9
16?0
1786
15 ( '4
16848
4883
8.9057
8.9488
11
632
5
29
22.3
19.4
22.1
x 9-5
20.82
42.9
9-1015
9- I 3 I 4
1
667
5
33
20.4
21.7
23-5
21.0
21.65
55-9
9-1339
9.2046
0.2035
— 0.51
6-74
1
673
5
35
20.5
17.7
2I.4
19-5
19.78
55-3
9.0589
9.1269
0.1258
— 0.31
6-94
1
679
5
37
20.2
18.O
2O.4
18.4
19.25
55-4
9.0362
9.1046
0.1035
— 0.26
6.99
2
628
5
39
19.0
17-5
19-5
18.5
18.62
54-5
9.0084
9.0730
0.0719
— 0.18
7.07
1
685
5
41
15.2
12.8
15-5
134
14.22
56.0
8.7806
8.8517
0.1494
4-0.37
7.62
