292
Müller und Kempf, Photometrische Durchmusterung
292
B.D.
Sternzeit
1
II
III
IV
J
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
3 °
1488
6 h IO ra
3587
33-5
338 o
3385
33892
4984
9-4933
9-5397
0.1260
— O.32
6.15
IO
1149
6 13
33 -o
32.4
33-9
31-5
32.70
42.0
9.4652
94933
11
1588
6 17
28.5
23-9
26.7
26.4
26.38
43-2
9.2954
9-3259
8
1543
6 19
37-4
36.0
38.8
32.6
36.20
44-3
9.5426
9-5756
0.1619
— 0.40
6.07
8
1562
6 21
27-5
24.2
254
25.1
25-55
44-3
9.2696
9.3026
0.1 I I I
+ 0.28
6-75
8
1568
6 23
20.8
18.1
19.2
18.5
I 9 -I 5
43-8
9.0319
9.0638
0.3499
+ 0.87
7-34
7
1539
6 25
27.6
24.4
27.6
26.7
26.58
45 -o
9-3015
9 - 336 i
0.0776
+ 0-19
6.66
7
1544
6 27
26.6
24.6
254
25.1
25.42
45 - 2
9.2654
9-3005
0.1132
+ 0.28
6-75
5
1513
6 30
23-5
21.7
24.0
22.4
22.90
47-7
9.1802
9.2217
0.1920
+ 0.48
6-95
IO
1149
6 33
36.5
34-5
35 -o
34-5
35-12
42.0
9-5197
9-5478
11
1588
6 35
29.4
24.6
27-3
23-9
26.30
42.2
9.2929
9 - 32 I 4
Mittel aus den Vergleichsternbeobachtungen : 9.3970; 9.4096; 9.4346.
Zur Reduction benutzt: 9.4137.
Zone 418
. 1891 Januar 22.
Beobachter: Müller.
Photometer :
CiL Vergleichsterne: Nr.
7 und Nr.
9. Luft:
2.
8°
455
3 b 6 m
1787
I 7 ?2
1784
1885
17870
448 o
8.9658
8.9981
8
652
3 14
16.2
15-5
15.6
16.2
15.88
44.8
8.8743
8.9084
18
243
3 18
26.1
25-4
25-7
254
25-65
38.0
9.2727
9.2938
0.3891
— 0.97
4-03
2
317
3 20
24.7
24.2
23.2
24.6
24.18
53 -i
9.2247
9.2837
O.3790
— o -95
4-05
2
422
3 22
28.5
29.4
30.2
30-5
29.65
504
9.3887
9.4382
0-5335
— i -33
3-67
*)3
419
3 26
39-3
40.6
39-6
40.9
40.10
49.1
9.6179
9.6634
0.7587
— 1.90
2.68
8
455
3 28
15*1
15-4
16.2
16.3
15-75
44.4
8.8674
8.9006
8
652
3 30
14-5
14.6
16.3
16.2
15.40
44.1
8.8483
8.8808
8
5 ”
3 32
29.0
28.6
28.4
28.9
28.72
43-9
9-3635
9-3956
0.4909
— 1.23
3-77
*) 8
5 “
3 34
21.6
22.3
22.7
23.2
22 45
43-9
9.1639
9.1960
0.2913
— 0.73
3-85
*j I 5
612
3 36
22.8
22.3
22.1
21.4
22.15
37-7
9.1528
9-1734
0.2687
— 0.67
3-91
i 5
612
3 37
26.5
29.7
26.0
27.9
27.52
37-7
9.3294
9-3500
0.4453
— 1.11
3-89
i 7
712
3 40
26.1
22.4
22.8
24.8
24.02
35-8
9.2193
9.2372
0.3325
— 0.83
4.17
18
640
3 43
28.7
26.8
28.2
29-3
28.25
34-3
9-3503
9.3663
0.4616
— i • 1 5
3.85
8
652
3 45
15-3
14.6
15.6
14.9
15. 10
43-6
8.8316
8.8630
8
455
3 48
15-7
15-2
154
14.8
15.28
45-3
8.8417
8.8770
Mittel aus den Vergleichsternbeobachtungen: 8.9533; 8.8907; 8.8700.
Zur Reduction benutzt: 8.9047
*) Mit Blende 3 beobachtet.
Zone 41g. 1891 Januar 22
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 12 und Nr. 14.
Luft: X-
-2.
IO°
818
4 h 6 ra
3785
4580
3584
3988
39842
4584
9.6056
9.6412
IO
1 149
4 ii
33 -i
29-5
31.2
30.6
31.10
49.6
9.4262
9-4732
11
975
4 14
38.5
34-8
35-5
37-3
36.52
45-3
9.5492
9-5845
0.02 I I
— 0.05
6.04
11
1009
4 16
29.9
29.0
30.2
30.7
29-95
45-5
9.3966
9.4324
0.13 IO
+ 0.33
6.42
12
980
4 18
24.2
20.5
21.7
22.0
22.10
44.2
9.1509
9 -i 837
0.3797
+ 0.95
7.04
I 2
968
4 19
38.0
36.5
36.8
41.2
38.12
43-8
9.5810
9.6129
0.0495
— 0.12
5-97
14
1088
4 21
27.0
24.4
2Ò.4
25.6
25-85
42.4
9.2790
9-3079
0-2555
+ 0.64
6-73
14
1136
4 23
24.6
22.9
234
24.1
23-75
42.5
9.2101
9.2392
0.3242
+ 0.81
6.90
IO
818
4 26
40.5
38.5
39 -°
394
39-35
44.1
9.6043
9.6368
IO
1149
4 29
34 -o
32.0
33-5
31.0
32.62
47.8
94633
9 - 505 I
16
940
4 31
18.8
14-5
16.6
15-7
16.40
39-2
8.9015
8.9245
0.6389
+ 1.60
7.69
16
957
4 34
26.8
25-5
27-5
26.6
26.60
394
9.3021
9-3255
0.2379
+ 0.59
6.68
16
999
4 35
27.7
23-5
27-5
25.6
26.08
39-7
9.2862
9 - 3 101
0.2533
+ 0.63
6.72
16
1001
4 37
18.3
16.4
17-5
18.4
17-65
39-5
8.9635
8.9870
0.5764
+ 1-44
7-53
17
1109
4 38
20.4
19.4
20.5
20.0
20.08
38.5
9 -o 7 i 5
9-0934
0.4700
+ 1.18
7.27
18
1040
4 40
21.9
21.8
24.0
23-5
22.80
364
9.1766
9-1954
0.3680
+ 0.92
7.01
IO
818
4 43
41.6
40.5
38.7
41.7
40.62
43-2
9.6272
9-6577
IO
1149
4 45
33 -o
29.7
31-5
30.6
31.20
46.3
9.4287
9.4665
Mittel aus den Vergleichsternbeobachtunge
n: 9 - 557 2 j 9-5710; 9.5621. Zur Reduction benutzt: 9.5634.
