150
Müller und Kempf, Photometrische Durchmusterung
150
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 62
1887 Januar ig.
Beobachter : Kempf.
Photometer:
Cl. Vergleichsterne: Nr. c
und Nr.
[i. Luft:
3 -
8°
652
4 h 5 m
2 i?o
2 3?o
2 7 ?0
2580
2 4?00
43-4
9.2186
9.2496
9
683
4 6
25.2
26.4
27.6
26.0
26.30
43-3
9.2929
9-3237
15
666
4 8
24-5
25-7
28.5
25*5
26.05
37 -o
9-2853
9.3049
0.0188
— O.05
4-95
7
681
4 IO
18.2
18.8
18.7
18.4
18.52
45 -o
9.0039
9-0385
0.2476
+ O.62
5.62
IO
621
4 12
18.0
18.0
18.O
194
18.35
41.8
8.9961
9.0238
O.2623
4“ 0.66
5.66
11
646
4 14
18.5
18.9
21.0
20.1
19.62
41.2
9.0521
9.0787
0.2074
+ 0.52
5-52
8
777
4 16
3 1 - 1
26.0
29.6
30.5
29.30
44.0
9-3793
9.4116
0.1255
— 0.31
4.69
18
743
4 18
22.7
20.5
22.9
22.5
22.15
34 -i
9- 1 528
9 -ì 685
O.I I 76
+ 0.29
5-29
8
652
4 20
23-3
24-5
28.0
24.2
25.00
43-4
9-2519
9.2829
9
683
4 21
24.0
24.4
27.0
26.9
25.58
42.7
9.2705
9.3000
5
745
4 23
42.8
41.0
43-2
39 -°
41.50
47.2
9.6425
9.6826
0.3965
— 0.99
4.01
H
777
4 25
31.0
27.0
28.9
274
28.58
38.6
9-3595
9.3816
0.0955
— 0.24
4.76
2
800
4 28
19.0
19 5
16.5
20.9
18.98
50.2
9.0244
9.0732
0.2 129
+ 0.53
5-53
7
755
4 30
19-3
19.5
18.5
18.9
19.05
44.9
9.0275
9.0619
0.2242
+ 0.56
5.56
13
740
4 32
38.0
36.9
42.8
39-2
39.22
39-3
9.6019
9.6251
0.3390
— 0.85
4-15
16
672
4 34
18.2
15.6
16.7
I 9*5
17.50
35-6
8.9563
8.9740
O.3 12 I
+ 0.78
5.78
8
652
4 36
24.4
23-9
23-7
24-5
24.12
43-7
9.2227
9-2543
9
683
4 38
24.0
24.0
29.0
26.2
25.80
42.4
9.2774
9.3063
Mittel aus den Vergleichsternbeobachtunge
n : 9.2867; 9.2914; 9.2803.
Zur Reduction benutzt: 9.2861
Zone 63
. 1887 Januar ig.
Beobachter: Müller.
Photometer:
Cl. Vergleichsterne: Nr. 13 und Nr. 15. Luft:
3 .
9 °
1064
6 h 46 m
2 I?4
2 5-3
2Ó?8
2 7-4
25822
4480
9.2590
9 - 29 1 3
11
1428
6 51
13-5
14.8
13.O
16.3
14.40
41-3
8 . 79 I 3
8.8181
17
1357
6 53
13-7
14.2
16.5
14.7
14.78
34-8
8.8134
8.8300
O.2408
+ 0.60
5-38
13
1390
6 56
21.0
21.2
20.5
21.6
21.08
39-3
9.1118
9 -I 350
O.0642
— 0.16
4.62
8
1496
6 58
18.3
20.8
20.2
18.6
19.48
44-3
9.0461
9.0791
O.OO83
— 0.02
4.76
2
1397
6 59
l8.6
20.5
18.4
22.4
19.98
50.0
9.0673
9- 11 5 5
O.O447
O.I I
4.67
13
1462
7 2
I9.O
20.7
20.4
20.7
20.20
39-2
9.0764
9.0994
0.0286
— 0.07
4.71
7
1607
7 5
10.6
12.6
I 1 .6
13.i
I I.98
44-7
8.6344
8.6683
O.4025
4- i .01
5-79
9
1064
7 8
24.7
27.1
25-5
27-5
2Ó.20
45-2
9.2899
9-3250
11
1428
7 IO
15.6
154
1 5-7
16.7
I 5-85
41-3
8.8727
8.8995
16
1397
7 12
12.6
14.1
13-1
I 5*7
I3.88
36.3
8.7600
8.7786
O.2922
+ 0.73
5-51
16
1417
7 14
174
16.6
16.8
17.6
I 7.IO
36.0
8.9368
8-9550
O.II58
4- 0.29
5-07
16
1443
7 15
34-3
37-6
35-8
38.1
3645
35-7
9-5478
9-5656
O.4948
— 1.24
3-54
11
1578
7 18
13.8
15-5
15.2
14.2
14.68
40.5
8.8076
8.8329
O.2379
4-0.59
5-37
9
1643
7 23
17.6
194
1 7-3
18.7
18.25
42.9
8.9915
9.0214
O.O494
4-0.12
4.90
9
1660
7 24
24-3
254
22.0
26.8
24.62
43-3
9-2395
9.2703
O.1995
— 0.50
4.28
9
1064
7 26
23-3
25-3
22.5
234
23.62
46.6
9.2056
9.2442
11
1428
7 28
14.0
15.2
144
* 5-9
14.88
41.7
8.8192
8.8467
Mittel aus den Vergleichsternbeobachtungen: 9.0547; 9.1123; 9.0454.
Zur Reduction benutzt: 9.0708.
Zone 64
1887 Januar 28.
Beobachter :
Kempf.
Photometer
D. Vergleichsterne: Nr. 8 und Nr. 10. Luft:
3 -
9 °
472
41139m
20?0
i8?o
1989
i 8? 5
19810
4486
9.0297
9.0634
11
632
4 42
2I.4
23-9
22.5
23-5
22.82
41-3
9- 1 773
9.2041
2
692
4 45
2O.9
19-3
24.1
21.2
21.38
50.6
9 - 1 2 3 5
9 -I 736
O.O307
— 0.08
7.17
5
649
4 48
19-5
20.0
23-7
21.0
21.05
47-3
9.1107
9 -I 5 II
O.O082
— 0.02
7-23
4
691
4 50
25.0
28.4
28.1
29-5
27-75
48.7
9 - 336 i
9.3804
0.2375
— 0.59
6.66
8
687
4 52
28.0
30.5
314
29.6
29.88
44.6
9.3948
9.4285
O.2856
— 0.71
6-54
6
685
4 54
20.3
19-5
20.0
20.0
19-95
46.1
9.0660
9 - 1 °3 3
O.O396
4-0.10
7-35
6
686
4 56
14.6
15.0
15-5
16.0
15.28
46.1
8.8417
8.8790
O.2639
4- 0.66
7.91
9
472
4 59
18.1
17.9
19.4
18.0
18.35
45-9
8.9961
9.0329
11
6 32
5 2
24.0
21.1
234
23.0
22.88
41.7
9- 1 795
9.2070
