378
Müller und Kempf, Photometrische Durchmusterung
378
B.D.
Sternzeit
I
II
III
IV
J
g
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zusatz-Zonen.
Zusatz-Zone i.
1893 Januar 7.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 46 und Nr. 48. Luft:
2.
9 °
5 111
i h 9 ra
2 2?8
1787
20?6
i8?o
19878
5186
9.0589
9 - 1 124
9
5277
1 12
21.9
19.6
19-5
18.7
19.92
46.7
9.0647
9 -i °35
i 3
4971
1 16
34 -o
28.6
30.2
26.5
29.82
49.8
9-3932
9.4408
0.3756
— O.94
5.82
9
5122
1 25
49.1
42.0
44.6
34-6
42.58
53-6
9.6607
9.7216
0.6564
— 1.64
5-12
16 4831
1 27
34-9
30.9
364
30.6
33-20
47-7
9.4769
9.5184
0.4532
— 1-13
5-63
19
5036
1 29
32.9
32.6
344
31-3
32.80
44.2
9-4675
9-5003
0.4351
— 1.09
5-67
9
5170
1 3 i
32.3
32.0
34-5
30.2
32.25
52.3
9-4545
9 - 5 I 05
0.4453
— 1.11
5-65
16 4882
1 33
28.4
28.7
33-8
28.6
29.88
45-8
9.3948
9 . 43 I 3
0.3661
— 0.92
5-84
9
5 i”
1 35
17.6
i 7-3
18.1
17.4
17.60
54-7
8.9611
9.0265
9
5277
1 37
17.4
17-5
20.5
17.7
18.28
48.9
8.9929
9.0378
4
4997
1 40
39 -i
40.6
42.9
39-8
40.60
56.2
9.6269
9.6989
0.6337
-1.58
5.18
11
4993
1 43
37 -o
43-5
44.8
40-5
41-45
50.0
9.6417
9.6899
0.6247
-1.56
5.20
0
4998
1 45
34-4
35-8
40.0
36.5
36.68
59-8
9-5525
9-6433
0.5781
— i -45
5-31
17
4952
1 47
29.2
30.4
33-3
32.6
3 I -38
43-4
9-4332
9.4642
0.3990
— 1.00
5-76
9 5 26 8
1 50
41.6
40.3
43-6
37-9
40.85
50.4
9-6313
9.6808
0.6156
— i -54
5.22
9
5277
1 5 i
17-5
16.9
18.3
18.8
17.88
50.4
8.9744
9.0239
18
5231
1 53
43-8
41.0
41.9
41.1
41-95
41.8
9.6502
9.6779
0.6127
— i -53
5-23
9
5 111
1 57
19.6
16.7
20.4
17.8
18.62
57-6
9.0084
9.0872
Mittel aus den Vergleichsternbeobachtungen: 9.1080; 9.0321; 9.0556. Zur Reduction benutzt: 9.0652.
Zusatz-Zone 2.
1893 Januar
7 -
Beobachter:
fLempf.
Photometer:
Ci. Vergleichsterne: Nr. 3
und Nr. 5. Luft: 2.
11°
96
2 h 9 m
17?o
l8?2
i 8?7
i8? 4
i8?o8
4486
8.9837
9.0174
IO
252
2 12
16.4
15-9
154
154
I 5-78
42.2
8.8689
8.8974
i 5
63
2 16
13-9
15-9
13.6
13-9
14.32
42.9
8.7866
8.8165
0.0998
+ 0.25
6.17
12
57
2 18
12.5
11.0
11-5
12-5
11.88
45-2
8.6272
8.6623
0.2540
+ 0.64
6.56
12
59
2 20
12.1
1 1-5
12.4
14-5
12.62
45-5
8.6788
8.7146
0.2017
+ 0.50
. 6.42
14
76
2 23
1 5 • 1
15.0
16.5
17.2
15-95
43-8
8.8781
8.9100
0.0063
4- 0.02
5-94
18
IOI
2 25
10.5
13.6
14.0
134
12.88
39 -o
8.6963
8.7190
0.1973
+ 0.49
6.41
4
123
2 28
16.0
15*2
16.5
18.0
16.42
52.4
8.9025
8.9589
0.0426
— 0.11
5.81
11
96
2 30
17.4
17.2
17-5
18.5
i 7- 6 5
46-5
8.9635
9.0018
IO
252
2 33
12.8
i 3-7
15-5
14-5
14.12
43 -o
8.7746
8.8047
2
118
2 35
12.0
11.6
12.5
13.0
12.28
54-5
8.6555
8.7201
0.1962
+ 0.49
6.41
18
122
2 38
16.0
13-5
14-5
14-5
14.62
40.0
8.8042
8.8286
0.0877
-r 0.22
6.14
12
119
2 40
ii -5
12.0
13-3
13-5
12.58
44.8
8.6761
8.7102
0.2061
+ O.52
6.44
12
135
2 45
14.5
12.3
14-5
14.6
13.98
45 -i
8.7662
8.8010
0.1153
+ O.29
6.21
H
175
2 48
14.4
14-3
14.9
15.6
14.80
42.6
8.8146
8.8439
0.0724
+ O.18
6.10
6
181
2 49
14-5
13.2
12.6
13-5
13-45
50.3
8-7332
8.7823
0.1340
+ 0-34
6.26
11
96
2 52
18.5
17.4
16.3
17.6
17-45
48.7
8-9539
8.9982
IO
252
2 55
13-7
13-4
12.6
14.9
13-65
44.2
8.7458
8.7786
Mittel aus den Vergleichsternbeobachtungen[: 8.9574; 8.9032; 8.8884. Zur Reduction benutzt: 8.9163.
Zusatz-Zone 3.
1893 Januar
7 -
Beobachter:
Müller.
Photometer:
Ci. Vergleichsterne: Nr.
und Nr.
7. Luft: 2.
IO C
252
3I1 0 m
1487
1480
1388
1380
13888
4485
8.7600
8-7934
8
455
3 3
25-1
24-5
24.6
26.3
25.12
43-9
9-2558
9.2879
1
347
3 5
12.5
13.0
12.1
13-7
12.82
53-4
8.6922
8-7523
0.3003
+ O.75
6.32
11
261
3 6
12.4
15-4
13.6
13-7
I 3-78
43 -i
8-7539
8.7842
0.2684
+ O.67
6.24
2
3 11
3 8
12.9
14.7
14-3
15.2
14.28
52-1
8.7842
8-8395
0.2 131
+ 0-53
6.10
12
271
3 10
14.9
134
14.8
15.0
14.52
42.0
8.7984
8.8265
0.226l
+ 0-57
6.14
