290
Müller und Kempf, Photometrische Durchmusterung
290
B.D.
Sternzeit
I
II
III
IV
/
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
i 7°3687
20 h 2 Ó m
i 6 ?i
1385
J 5°3
1480
14872
4089
8.8100
8.8360
0.4146
+ 1.04
7.88
17 3691
20 27
14.8
12.3
14-5
13-5
13.78
40.9
8.7539
8.7799
0.4707
4~ 1.18
8.02
17 3701
20 29
19.4
16.6
17.9
15-7
1740
41.1
8-9515
8.9779
0.2727
-f- 0.68
7 - 5 2 '
10 3573
20 31
26.0
25-5
26.5
24.0
25-50
48.2
9.2680
9.3109
10 3981
20 33
23-5
22.0
22.6
23-5
22.90
43-3
9.1802
9.2 110
15 3537
20 36
21.4
20.3
21.1
18.6
20.35
44.0
9.0826
9 -i 149
0.1357
+ 0-34
7.18
14 3615
20 38
21.1
16.6
18.5
174
18.40
44.6
8.9984
9.0321
0.2185
+ 0.55
7-39
13 3713
20 39
15.8
14-5
16.0
14-5
15.20
45-8
8.8372
8.8737
0.3769
+ 0.94
7.78
16 3593
20 41
14.0
11.0
12.5
10.5
12.00
43-2
8.6358
8.6663
0.5843
+ 1-46
8.30
19 3762
20 43
18.4
16.7
17.2
15-5
16.95
40.9
8.9294
8-9554
0.2952
+ 0-74
7.58
10 3633
20 44
25.6
22.7
25-5
22.4
24.05
48.6
9.2203
9.2643
0.0137
— 0.03
6.81
10 3573
20 46
25.0
234
24.6
23-5
24.12
49.8
9.2227
9.2703
10 3981
20 48
25.6
21.6
21.7
19.2
22.02
44-3
9.1479
9.1809
Mittel aus den Vergleichsternbeobachtungen: 9.2652; 9.2610; 9.2256.
Zur Reduction benutzt: 9.2506
Zone
413 .
1890 November 7
9
Beobachter: Müller.
Photometer :
I). Ver
gleichsterne: Nr. 38 und Nr. 40. Luft:
2.
io° 3981
20 h 50 m
2I?7
20?4
20?5
i 9?4
20850
4484
9.0887
9.1219
10 3573
20 52
234
22.0
22.8
20.1
22.08
50.5
9.1502
9.2000
10 3873
20 54
16.1
I4.2
15-9
14-5
15.18
46.1
8.8361
8.8734
0.2652
4- 0.66
7-50
11 3802
20 56
29.6
26.3
27.6
25.6
27.28
45-8
9.3224
9-3589
0.2203
— 0.55
6.29
13 3988
20 57
17-5
2O.7
174
194
i 8.75
43-9
9.0142
9.0463
0.0923
4- 0.23
7.07
13 3985
20 59
13-7
IO.I
12.5
10.4
11.68
43-7
8.6126
8.6442
0.4944
4 ~ 1.24
8.08
14 3896
21 0
21.8
18.8
21.9
19.7
20.55
42.8
9.0907
9.1204
0.0182
+ 0.05
6.89
15 3798
21 2
13.0
13-7
134
12.2
13.08
41.9
8.7094
8-7373
0.4013
+ 1.00
7.84
10 3573
21 4
21.9
18.6
21.8
21.3
20.90
51-9
9.1047
9.1592
10 3981
21 6
20.0
18.2
20.7
20.7
19.90
45-7
9.0639
9.1002
17 3943
21 8
21.1
16.4
17.4
15-2
I 7-52
41.1
8.9573
8.9837
0.1549
+ 0.39
7.23
*)i8 4043
21 10
19-5
16.3
20.5
17.2
18.38
40.2
8.9975
9.0223
0.1163
+ 0.29
7-13
18 4055
21 12
13.0
10.6
11*9
9-3
I 1.20
40.4
8-5767
8.6018
0.5368
+ 1-34
8.18
19 3997
21 13
20.3
15-2
17.9
15-3
17.18
39 -i
8.9407
8.9636
0.1750
+ 0.44
7.28
19 4000
21 16
24.9
2 1 .9
21.3
22.3
22.6o
39-5
9.1693
9.1928
0.0542
— 0.14
6.70
12 3896
21 17
18.9
16.4
17.9
14.0
l6.8o
46.7
8.9219
8.9607
0.1779
+ 0.44
7.28
10 3573
21 19
21.7
19-3
20.7
22.7
21.10
53-7
9.1126
9.1739
10 3981
21 22
22.1
17.8
19.0
18.1
I 9-25
47.1
9.0362
9.0761
Mittel aus den Vergleichsternbeobachtungen: 9.1610; 9.1297; 9.1250. Zur Reduction benutzt: 9.1386.
*) 1804043 dupl. Nur die folgende, hellere Componente gemessen.
Zone
414.
i8go November ig.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 44 und Nr. 46. Luft:
3 -
I0°4004
23 11 36™
31-8
27-5
2 9?9
2785
29818
4884
9-3761
9.4196
9 5111
23 38
26.9
23.6
23.6
24-5
24.65
43-9
9.2405
9.2726
II 4729
23 41
20.4
16.9
18.0
17.6
18.22
45-2
8.9901
9.0252
0.3197
-(- 0.80
7-34
II 4730
23 42
23.1
20.6
22.5
21.4
21.90
45-8
9-1434
9.1799
0.1650
4- 0.41
6-95
16 4665
24 44
16.4
13.6
15.6
14.9
15.12
41-5
8.8327
8.8598
0.4851
4- 1.21
7*75
17 4693
23 45
29-5
27.0
29-5
304
29.10
40.4
9-3739
9.3990
0.0541
— 0.14
6.40
18 4930
23 47
37 -o
35-3
35-6
36.0
35-98
39-3
9.5380
9.5612
0.2 163
— 0.54
6.00
12 4760
23 49
16.6
13.0
144
13.0
14.25
45 -i
8.7824
8.8172
O.5277
+ 1-32
7.86
IO 4604
23 51
30.1
27.0
28.2
28.4
28.42
50.0
9-355 1
94033
9 5111
23 52
27.0
22.6
24-5
25-7
24-95
44-7
9-2503
9.2842
Mittel aus den Vergleichsternbeobachtungen: 9.3461 ; 9.3438. Zur Reduction benutzt: 9.3449.
