176
Müller und Kempf, Photometrische Durchmusterung
176
15 . D.
Sternzeit
1
11
in
IV
J
z
log. sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 127. 1887 März 24.
Beobachter: Müller. Photometer: D
Vergleichsterne: Nr. 12 und Nr. 14
Luft: 2-
- 3 -
IO°
8l8
8 1
n m
26? 7
25-4
26? 4
2 696
26828
53-3
9.2923
9-3520
IO
II49
8
13
22.6
20.3
24-5
20.2
2 1.90
47.6
9 -H 34
9.1846
11
975
8
15
26.1
26.8
25.8
24.2
25.72
50.1
9.2749
9-3234
O.0567
— O.14
5-95
14
1088
8
17
17.8
17.6
18.9
17.6
17.98
48.1
8.9791
9.0217
O.2450
4- 0.61
6.70
iö
940
8
18
13.6
12.7
14.6
12.5
13-35
45-9
8.7268
8.7636
0.5031
+■ 1.26
7-35
18
1040
8
20
17.4
15-7
17.2
154
16.42
44.2
8.9025
8-9353
0.3314
+ O.83
6.92
12
968
8
21
27.4
27.7
28.5
29.2
28.20
494
9.3489
9-3953
0.1286
— O.32
5-77
IÖ
957
8
23
17.6
18.5
194
17.9
18.35
46.5
8.9961
9-0344
O.2323
+ 0.58
6.67
IO
818
8
25
26.1
27.6
26.4
26.6
26.68
55 - 1
9-3045
9 - 37 i 6
IO
1149
8
27
22.8
21.0
22.3
20.3
2 1.60
49.0
9.1320
9.1772
12
980
8
29
16.6
15.0
16.5
15.6
I 5-92
504
8.8765
8.9260
0.3407
+ 0.85
6.94
I I
1009
8
30
22.3
21.0
20.6
194
20.82
51.0
9-1015
9.1529
0.1138
-[— 0.28
6-37
i 7
1109
8
3 i
i 3-5
13-4
134
I 3-9
13-55
46.4
8.7396
8.7776
0.4891
+ 1-22
7 - 3 i
H
1136
8
33
16.4
15-7
16.4
154
15.98
48.7
8.8796
8.9239
0.3428
4- 0.86
6-95
16
999
8
34
18.8
18.8
17.7
21.4
19.18
47.0
9-0331
9.0727
0.1940
+ 0.49
6.58
16
1001
8
35
12.4
12.5
12.7
134
12.75
46.9
8.6876
8.7269
0.5398
+ i -35
7-44
IO
818
8
37
25.6
29.8
26.0
24.0
26.35
56.6
9.2945
9.3684
IO
1149
8
39
20.4
19.8
21.0
21.7
20.72
50.2
9-0975
9.1463
Mittel aus den Vergleichsternbeobachtungen: 9.2683; 9.2744; 9.2574. Zur Reduction benutzt: 9.2667.
Zone 128. 1887 März 24.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 14
und Nr. 16. Luft:
3 -
IO°
1149
8 b 43 m
2 3°5
2 6?4
2486
2381
24840
5087
9.2321
9.2825
11
1588
8
45
20.0
22.5
24.O
21.0
2 1.88
44.6
9.1426
9 -I 763
14
1395
8
47
17.0
17.6
19.O
17.9
17.88
46.2
8.9744
9.0119
0.2066
+ 0.52
6.99
18
1324
8
49
12.6
12.6
13.2
10.6
12.25
42.8
8.6534
8.6831
0.5354
+ i -34
7.81
18
1338
8
5 i
13.6
16.1
16.5
13.6
14-95
42.1
8.8232
8.8515
0.3670
+ 0.92
7-39
iö
1273
8
52
17.9
17-5
19-5
17-5
18.10
44.0
8.9846
9.0169
0.2016
+ 0.50
6.97
17
1392
8
54
12.5
12.8
13-9
14.0
13-30
43-8
8.7236
8-7555
0.4630
4- 1.16
7-63
IO
1 262
8
55
12.5
13-9
15.0
12.5
13.48
49-5
8.7351
8.7818
0.4367
+ 1-09
7-56
IO
1149
8
57
23-7
26.5
26.0
25-3
25-38
52.3
9.2642
9.3202
11
1588
8
59
19.8
22.5
22.6
21.0
21.48
45-7
9.1274
9.1637
18
1349
9
1
19.0
19-5
23-5
20.3
20.58
43-7
9.0919
9-1235
0.0950
4- 0.24
6.71
18
1362
9
2
13-5
11.1
12.4
11.6
12.15
43-7
8.6464
8.6780
0.5405
+ 1.35
7.82
16
1298
9
3
24.6
27-5
28.8
27.8
27.18
454
9 - 3 I 94
9-3550
0.1365
— 0.34
6.13
13
1434
9
5
27.2
31.2
33-5
30.0
3048
47-9
9.4104
9.4524
0.2339
— 0.58
5-89
15
1347
9
7
14.9
13.0
14.9
13.2
14.00
46.6
8.7674
8.8060
0.4125
4- 1.03
7-50
11
1344
9
8
19.9
20.1
234
24-5
21.98
50.1
9.1464
9.1949
0.0236
4- 0.06
6-53
IO
1149
9
10
23.8
234
24.2
25.0
24.10
53-9
9.2220
9.2841
11
1588
9
12
20.2
19.0
19-5
19.1
19-45
46.9
9.0449
9.0842
Mittel aus den Vergleichsternbeobachtungen: 9.2294; 9,2420; 9.1841.
Zur Reduction benutzt: 9.2185.
Zone 129. 1887 April 8.
Beobachter: Kempf.
Photometer: Ci. Vergleichsterne: Nr. 17 und Nr.
19. Luft:
2.
11 °
1670
8 h 56 m
i 8°5
2 0?0
2 2?0
1989
tsi
O
• O
O
44 -o
9.0723
9.IO46
11
1984
8
59
19.7
2 1.6
2 1.6
21-5
21.10
4 i -3
9.1126
9-1394
12
1567
9
1
28.9
30.8
30-9
29.4
30.00
44.6
9-3979
9.4316
0.2852
— 0.71
4.80
2
1691
9
3
20.5
I9.O
20.8
20.9
20.30
54 - 1
9.0805
9 -H 34
0.0030
4- 0.01
5-52
IÖ
1510
9
6
22.5
22.5
22.7
23.0
22.68
41.2
9-1723
9.1989
O.0525
— 0.13
5-38
l8
1701
9
8
24.1
25.O
26.4
24.9
25.10
39-2
9 - 255 I
9.2781
O.1317
— 0.33
5.18
l8
1733
9
IO
25-1
26.6
28.5
28.7
27.22
37-9
9.3206
9 - 34 I 5
O.1951
— 0.49
5.02
2
1808
9
11
21.7
23.O
20.6
22.7
22.00
53-3
9.1472
9.2069
0.0605
— 0.15
5-36
I I
1670
9
14
17-5
20.6
20.5
22.4
20.25
45-4
9.0785
9 -II 4 I
