200
Müller und Kempf, Photometrische Durchmusterung
200
B.l).
Sternzeit
I
II
III
IV
/
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 187.
1887 November 17.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 1
—2.
io°4004
23k j 5 m
2485
2485
2484
2I?3
23?68
46?6
9.2076
9.2462
9 5 i 11
23 18
20.9
19.7
19.6
16.7
19.22
43 -o
9.0349
9.0650
ii 4583
23 23
24.6
22.5
23-7
2 I.4
23-05
47.0
9.1856
9.2252
0.0715
— 0.18
6.36
ii 4596
23 25
14.2
12.4
14.4
12.7
13.42
46.7
8.7313
8.7701
0.3836
+ 0.96
7-50
10 4570
23 26
14.4
14.0
134
12.2
i 3 - 5 o
48.3
8.7364
8.7796
0.3741
+ 0.94
7.48
17 4606
23 29
22.0
19.0
19.4
I7.7
19.52
41.7
9.0479
9-0754
0.0783
0.20
6-74
19 4740
23 31
I7.4
15-3
17-5
16.4
16.65
40.5
8.9144
8-9397
0.2 I4O
+ 0.54
7.08
14 4637
23 32
2O.4
18.5
20.6
20.6
20.02
44.8
9.0689
9.1030
O.O5O7
4- 0.13
6.67
10 4604
23 34
24.2
23.8
25.6
24-3
24.48
48.2
9.2348
9.2777
9 5111
23 36
19-5
19.0
18.0
18.2
18.68
43-8
9.0111
9.0430
ii 4613
23 39
14.4
13-7
15-3
14.2
14.40
48.5
8-7913
8.8350
O.3187
+ 0.80
7-34
19 4748
23 41
15.0
13-9
14.7
14.2
14-45
4 i -5
8-7943
8.82 14
0.3323
+ 0.83
7-37
19 4754
23 42
27.6
29.4
27.6
26.6
27.80
41.0
9-3375
9-3637
0.2100
— 0.53
6.01
18 4845
23 44
12.6
13.0
13-9
12.1
12.90
41-3
8.6976
8.7244
O.4293
4- 1.07
7.61
14 4647
23 47
14.7
12.8
13.0
13.2
13.42
46.2
8.7313
8.7688
0.3849
+ 0.96
7-50
9 4872
23 49
16.6
16.2
16.6
I4.7
16.02
50.2
8.8817
8-9305
O.2232
+ 0.56
7.10
14 4668
23 50
24.2
25.6
25.6
25-3
25.18
46.1
9-2577
9.2950
O.I 4 I 3
— 0.35
6.19
10 4604
23 52
22.6
23-7
23-5
22.4
23-05
50.1
9.1856
9.2341
9 5111
23 54
18.2
19-3
18.2
20.0
18.92
44.8
9.0218
9-0559
Mittel aus den Vergleichsternbeobachtungen : 9.1556; 9.1604; 9.1450. Zur Reduction benutzt: 9.1537.
Zone
H
00
00
1887 November 17.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft:
—2.
1o°4604
O k 6 m
2 6?4
2389
29?o
2485
25895
5187
9.2822
9.3360
9 5 111
O 8
24.4
20.6
234
21.8
22.55
45-8
9 -i 675
9.2040
15 46 i 7
0 IO
18.0
20.5
20.5
19-5
19.62
43-4
9.0521
9.0831
O.2088
+ 0.52
7.06
19 4897
0 12
20.3
17.6
21.5
20.7
20.02
40.3
9.0689
9.0938
O.I981
+ 0.50
7.04
13 4892
0 14
14.6
12.2
12.4
12.5
12.92
45-6
8.6989
8-7349
0.5570
+ i -39
7-93
13 4896
0 15
22.2
22.9
24-5
25.0
23-65
45-7
9.2066
9.2429
0.0490
+ 0.12
6.66
13 4898
0 16
19.0
18.1
21.5
18.2
19.20
45-4
9.0340
9.0696
0.2223
+ 0.56
7.10
14 4772
0 18
19.0
19.1
20.5
20.1
19.68
44-7
9-0547
9.0886
O.2033
+ 0.51
7-°5
10 4604
0 20
29-5
29.0
30.0
27.0
28.88
53-4
9-3679
9.4280
9 5111
0 22
22.8
21.5
22.8
23.0
22.52
46.9
9.1664
9.2057
14 4786
0 25
20.7
21.5
21.0
19.9
20.78
45 -i
9.0999
9-1347
O.I572
+ 0.39
6-93
14 4790
0 26
20.0
19.6
19-5
21.4
20.12
45-4
9-0731
9.1087
O.1832
~f— O.46
7.00
15 4639
0 28
22.3
18.5
20.0
19-5
20.08
44-7
9-0715
9.1054
O.1865
+ 0.47
7.01
16 4724
0 29
17-5
16.0
17.0
18.2
17.18
43-6
8.9407
8.9721
O.3198
-f- 0.80
7-34
17 4746
0 30
27-5
28.0
27.9
27.2
27.65
42.9
9-3332
9-3631
O.O712
— 0.18
6.36
11 4804
0 32
20.3
19.1
18.5
18.4
19.08
48.3
9.0288
9.0720
0.219g
+ 0.55
7.09
10 4604
0 34
27-5
27.8
25-5
28.1
27.22
55 -i
9.3206
9-3877
9 5111
0 36
22.4
24.0
21.6
20.0
22.00
48.2
9.1472
9.1901
Mittel aus den Vergleichsternbeobachtungen: 9.2700; 9.3169; 9.2889.
Zur Reduction benutzt: 9.2919.
Zone 189
1887 December
7 -
Beobachter:
Müller
Photometer
D. Vergleichsterne: Nr. 4
und Nr. 6. Luft: 3
IO° 168
O u 42 m
1984
1 6?5
ig?o
i6?8
17?9 2
4189
8.9762
9.OO41
8 385
O 44
26.0
25-4
27-3
234
25-52
47.8
9.2686
9.3104
2 270
O 47
27-5
26.4
29.0
24.6
26.88
50.6
9-3105
9.3606
O.2087
— 0.52
6.16
6 275
O 48
16.4
14.6
15-8
14-3
15.28
46.7
8.8417
8.8805
O.27 14
+ 0.68
7-36
9 235
O 50
16.0
15.2
16.6
17-3
16.28
43-9
8.8954
8-9275
O.2244
+ 0.56
7.24
8 292
O 52
20.7
18.9
19.8
18.5
19.48
45-6
9.0461
9.082 1
O.0698
+ 0.17
6.85
i 347
0 54
26.0
24.4
25.0
23-5
24.72
52.4
9.2428
9.2992
0.1473
— 0.37
6.31
5 274
O 56
17-5
17.2
18.5
18.0
17.80
48.4
8.9706
9.0141
O.I378
+ 0.34
7.02
