382
Müller und Kempf, Photometrische Durchmusterung
382
B.D.
Stenv/eit
I
II
III
IV
J
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zusatz-Zone n.
1893 Januar
17 .
Beobachter: Müller.
Photometer:
Gl. Vergleichsterne: Nr. i
und Nr.
3. Luft:
3 -
IO°
8
2 h o ,n
1485
1480
1487
1485
14842
4788
8.7925
8.8343
11
96
2 2
15.2
15.6
15-7
15.0
I 5-38
44.1
8.8472
8.8797
IO
5004
2 7
17-3
14.8
13.6
17.2
I 5-72
50.7
8.8658
8.9162
0.0722
— O.18
5-54
6
5216
2 8
9-7
9-5
11.0
9.2
9-85
53-9
8.4664
8.5285
0-3155
+ 0-79
6.51
8
5164
2 10
9.8
9.4
94
9.8
9.60
5 i -7
8.4442
8.4980
0.3460
4- 0.87
6-59
7
5121
2 12
12.2
10.9
12.2
12.2
11.88
52.3
8.6272
8.6832
0.1608
4- 0.40
6.12
7
27
2 14
IO.I
12.4
10.6
IO.9
11.00
5 i -4
8.561 2
8.6140
0.2300
-4 0.58
6.30
o
28
2 16
I 1.0
10.0
9-5
94
9.98
57-4
8.4776
8-5554
0.2886
4- 0.72
6.44
IO
8
2 18
14.6
i 4-5
14.2
14.7
14-50
49-7
8.7972
8.8445
11
96
2 21
15-3
14.0
14.6
16.3
I 5-05
45-6
8.8288
8.8648
IO
25
2 23
10.6
1 1-3
11.7
10.3
10.98
49.4
8.5596
8.6060
0.2380
4- 0.60
6.32
7
36
2 25
11.7
14.9
15-4
13-5
13.88
52 -i
8.760O
8.8153
0.0287
-4 0.07
5-79
I 2
25
2 27
8.7
10.3
9.6
9-5
9-52
47-3
8.4370
8-4774
0.3666
4- 0.92
6.64
I
57
2 29
11 -4
10.8
10.8
10.8
10.95
57-7
8-5573
8.6366
0.2074
4- 0.52
6.24
i 5
59
2 32
9.4
9-4
11 -4
10.0
10.05
45 -o
8.4836
8.5182
0.3258
4" 0.81
6-53
18
5 i
2 34
9.4
8.9
94
9.0
9.18
42.2
8.4057
8.4342
0.4098
4- 1.02
6.74
IO
8
2 36
13.0
13-7
13-5
13-5
13-42
5 i -7
8-7313
8.7851
11
96
2 38
15-2
15-4
14-3
14.4
14.82
47.2
8.8157
8.8558
Mittel aus den Vergleichsternbeobachtungen: 8.8570; 8.8547. 8.8204.
Zur Reduction benutzt: 8.8440.
Zusatz-Zone 12.
1893 Januar
17 -
Beobachter: Kempf.
Photometer:
Ci. Vergleichsterne: Nr.
und Nr.
7. Luft:
3 -
IO°
252
2 ll 47 m
n?6
n?6
n?6
0
• 0
1 1 ?3 8
4388
8.5903
8.6222
8
455
2 51
20.5
20.6
21.0
20.1
20.55
43-9
9.O9O7
9.1228
i
347
2 54
11.2
10.5
9-5
9.9
10.28
52.8
8.5O3O
8.5609
0.282 1
4- 0.71
6.28
11
261
3 0
10.5
10.0
8-5
8.9
9.48
42.7
8-4334
8.4629
0.3801
-4- 0.95
6.52
2
3 i 1
3 4
10.6
9-5
12.0
8.6
10.18
51.8
8.4947
8.5489
0.2941
4-0.74
6.31
I 2
271
3 7
10.5
10.5
11.4
9.8
10-55
41.8
8.5254
8.5531
0.2899
+ 0.72
6.29
17
307
3 u
9.6
10.4
8.9
10.5
9-85
37-5
8.4664
8.4867
0.3563
+ 0.89
6.46
7
324
3 14
9.0
10.4
8.9
94
9.42
47.1
8.4279
8.4678
0-3752
4- 0.94
6.51
IO
252
3 17
9-5
10.0
10.6
10.5
10.15
45-8
8.4922
8.5287
8
455
3 21
20.5
20.0
19-5
21.5
20.38
44.2
9.0838
9.1166
18
277
3 25
13.2
I3.O
13.2
12.5
12.98
36.9
8.7029
8.7224
0.1206
-4 0.30
5-87
7
347
3 28
12.3
12.6
12.9
12.6
12.60
47-3
8.6775
8.7179
0.1251
4- 0.31
5-88
14
357
3 31
12.5
11-5
12.9
12.5
12-35
41.1
8.6604
8.6868
O.1562
+ 0.39
5-96
l 9
340
3 34
11.7
12.8
13.0
1 1-5
12.25
36.6
8-6534
8.6724
0.1706
4 - 0.43
6.00
19
365
3 36
8.6
1 1-5
9.6
9.6
9.82
35-7
84637
8.4815
0.3615
4- 0.90
6-47
J 7
380
3 40
10.0
10.0
10.4
94
9-95
38.1
8-4750
8.4963
0.3467
-4 0.87
6.44
IO
252
3 44
10.5
10.5
10.5
10.5
10.50
48.2
8.5213
8.5642
8
455
3 47
22.0
20.0
19-5
18.5
20.00
45-2
9.0681
9.1032
Mittel aus den Vergleichsternbeobachtungen: 8.8725; 8.8227; 8.8337.
Zur Reduction benutzt: 8.8430.
Zusatz-Zone 13.
1893 Januar
17 ■
Beobachter:
Müller.
Photometer:
Ci. Vergleichsterne: Nr.
7 und Nr.
9. Luft:
3-
8°
455
31152m
2380
20?4
20?8
1985
20892
4585
9-io55
9-I4I3
8
652
3 55
24.4
23-5
24.0
23.6
23.88
43-5
9.2145
9-2457
7
450
3 57
10.8
13-3
11.8
i 3 -i
12.25
46.4
8-6534
8.6914
O.4962
4 - 1-24
6.24
3
410
3 59
10.0
9-3
1 1-3
8.8
9-85
50.2
8.4664
8.5152
0.6724
—J— 1.68
6.68
IO
401
4 2
13.6
13-3
12.7
13-3
13.22
44.1
8.7185
8.7510
O.4366
-4 1-09
6.09
4
485
4 3
I I.I
10.5
11.9
10.6
I 1.02
49-5
8.5628
8.6095
0.5781
4 - i -45
6-45
3
420
4 5
13.6
13-7
13.6
14.9
13-95
50.5
8.7643
8.8141
0.3735
4- 0.93
5-93
i
534
4 7
12.8
12.5
12.0
1 2.4
12.42
52.8
8.6652
8.7230
O.4646
-4 1 . 1 6
6.16
