236
Müller u^d Kempf, Photometrische Durchmusterung
236
B.D.
Steinzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
9 °
47
i h 38™
3184
2481
2 8?i
2785
27878
4584
9-3369
9-3725
16
11
1 40
25.6
23-5
25.0
23-5
24.40
40.5
9.2321
9-2574
0.0454
4- 0.11
6.63
13
2 7
1 41
16.3
13.6
16.5
14.0
15.10
43 -o
8.8316
8.8617
0.4411
+ 1.10
7.62
15
39
i 43
18.4
18.4
18.0
16.5
17.82
40.9
8.9715
8-9975
0.3053
4- 0.76
7.28
19
38
1 44
22.4
20.4
22.1
18.2
20.78
37-4
9.0999
9.1201
0.1827
4- 0.46
6.98
11
34
1 46
24-3
20.6
23-5
22.4
22.70
44-4
9.1730
9.2062
0.0966
4- 0.24
6.76
IO
25
1 48
27.6
29.1
29.9
28.1
28.68
46.0
9.3623
9-3993
0.0965
— 0.24
6.28
9
5277
i 50
24.0
22.9
24.1
23.8
23.70
50.3
9.2083
9-2574
9
47
i 52
31-9
274
274
26.0
28.18
46.5
9-3483
9.3866
Mittel aus den
Vergleichsternbeobachtungen: 9.2861; 9.3003; 9.3220. Zur Reduction benutzt: 9.3028
Zone 278.
1888 December
5 .
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 8 und Nr. 10. Luft: 2
3 *
9 °
472
3I1 jgm
1588
1483
1584
1387
14880
4288
8.8146
8.8443
11
632
3 20
18.4
15.8
18.9
17.6
17.68
43-5
8.9649
8.9961
2
692
3 22
16.O
14.2
16.6
14.8
15.40
51-5
8.8483
8.9014
0.0070
4- 0.02
7.27
5
649
3 24
15-4
14-3
15-7
15.0
15.10
48.4
8.8316
8.8751
0.0333
4- 0.08
7-33
4
691
3 25
22.5
21-5
22.0
21.4
21.85
49.6
9-1415
9.1885
0.2801
— 0.70
6-55
8
687
3 26
23.6
23-9
22.9
21.8
23-05
45-4
9.1856
9.2212
0.3128
— 0.78
6.47
6
685
3 28
17.4
14.9
15.8
15.0
15-78
46.9
8.8689
8.9082
0.0002
0.00
7-25
6
686
3 29
1 2.7
10.7
11.6
II -3
11.58
46.8
8.6052
8.6443
O.264I
4- 0.66
7.91
11
632
3 30
17-5
16.7
17-5
16.8
17.12
42.9
8.9378
8.9677
9
472
3 32
14.9
12.5
14.8
12.3
13.62
42.7
8-7439
8-7734
i
753
3 34
22.8
23.2
22.0
20.5
22.12
51-5
9 -i 5 i 6
9.2047
O.2963
— 0.74
6.51
i
755
3 36
24.2
23-3
23-3
2 1.0
22.95
51-7
9.1820
9-2358
0.3274
— 0.82
6-43
7
648
3 38
16.5
134
16.2
I3.6
14.92
45-4
8.8214
8.8570
O.O514
+ 0.13
7-38
7
656
3 40
11.2
94
10.7
8.2
9.88
46.2
8.4690
8.5065
O.4OI9
4- i .00
8.25
a^aJ
3 42
94
6.5
8.0
6-3
7-55
46.6
8.2371
8.2757
O.6327
4 - 1.58
8.83
) 0
090^
3 44
15-3
11. 9
16.4
12.8
14.10
46.6
8-7734
8.8120
O.O964
+ 0.24
7-49
5
671
3 45
18.2
17-7
18.7
15.6
17-55
47.6
8.9587
8.9999
O.O915
— 0.23
7.02
11
632
3 46
194
17.7
18.7
17.9
18.42
42.1
8.9993
9.0276
9
472
3 48
15-5
14-3
15.8
134
14-75
42.8
8.8117
8.8414
Mittel aus den
Vergleichsternbeobachtungen: 8.9202; 8.8706; 8.9345.
Zur Reduction benutzt: 8.9084.
*) 6° 696 dupl. Zuerst die vorangehende Componente gemessen.
Zone
279 .
1888 December
5 .
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 10
und Nr. 12. Luft: 2
— 3 -
ii°
632
3 53 m
1 9?8
2185
2I?4
20?5
20880
4189
9.1007
9.1286
IO
818
3 56
31-5
32.3
28.0
32.8
31-15
46.2
9-4275
9.4650
5
899
3 57
20.5
17.2
17.6
17.9
18.30
49.8
8.9938
9.0414
O.2624
4- 0.66
7.11
5
905
3 59
21.9
194
21.5
20.5
20.82
49.9
9 -ioi 5
9.1494
O.1544
+ 0.39
6.84
3
872
4 i
15-1
13-5
15-8
14.0
14.60
51-4
8.8030
8.8558
O.4480
4- 1.12
7-57
3
864
4 2
14.6
13-5
16.0
12.4
14.12
51-4
8.7746
8.8274
O.4764
+ 1.19
7.64
2
947
4 4
24.0
20.0
23.0
21.2
22.05
52.5
9-1491
9.2058
O.O980
4~ 0.25
6.70
2
965
4 6
24.4
20.6
21.0
I9.7
21.42
52.6
9-1251
9.1822
0.12 l6
+ 0.30
6-75
i
1032
4 7
2 8.6
27.8
27.1
27.7
27.80
53 -i
9-3375
9-3965
O.O927
— 0.23
6.22
11
632
4 10
19.0
19.1
19.0
18.4
18.88
41.4
9.0200
9.0470
IO
818
4 12
34-5
37-6
334
34 -i
34-90
45 -o
9 - 5 I 50
9.5496
o
1056
4 13
22.0
24.9
23.1
21-5
22.88
53-8
9-1795
9.2412
O.0626
4-0.16
6.61
6
923
4 15
18.7
20.0
22.0
19.9
20.15
47.6
9.0744
9 -II 56
O.1882
4-0.47
6.92
3
903
4 17
17.2
15.8
16.5
14.0
15.88
50.5
8-8743
8.9241
0-3797
4- 0.95
7.40
4
949
4 19
21.1
21.4
26.5
23-9
23.22
50.2
9.1916
9.2404
O.0634
4-0.16
6.61
3
948
4 20
32.5
32.0
34 -o
32-5
32-75
51.0
9.4664
9 - 5 I 78
0.2 I40
— 0.54
5-91
i
1021
4 22
19.9
20.0
22.0
20.3
20.55
52.7
9.0907
9.1482
•O.I556
+ 0.39
6.84
11
632
4 24
20.6
20.0
20.6
21.3
20.62
41.2
9-0935
9.1201
IO
818
4 25
34-7
32.5
34 -o
32.1
33 - 32 .
44 -i
9-4797
9.5122
Mittel aus den Vergleichsternbeobachtungen: 9.2968; 9.2983; 9.3162.
Zur Reduction benutzt: 9.3038.
