192
Müller und Kempf, Photometrische Durchmusterung
192
B.D.
Sternzeit
I
II
III
IV
J
Z
log sin 2 ./
corrig. |
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 167
. 1887 October 21.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 2
--3-
10 °435 1
2 1“
57 m
2387
20?4
22?I
20?0
2 1?55
44 -’7
9-1301
9.1640
io 3981
22
2
18.6
17-5
I9.4
17.4
18.22
51-4
8.9901
9.0429
14 4149
22
4
9-7
94
10.2
8.5
945
44.9
8.4307
8.4651
0.6365
+ i-59
8-39
14 4150
22
6
19.2
18.3
20.2
17.7
18.85
45-9
9.0187
9-0555
0.0461
+ 0.12
6.92
14 4158
22
7
19.0
16.3
18.5
17-5
17.82
45-5
8.9715
9.0073
0.0943
+ 0-24
7.04
17 4201
22
8
17.4
16.2
19-5
17.9
17-75
42.8
8.9682
8-9979
0.1037
+ 0.26
7.06
18 4365
22
IO
29.0
25-7
27.6
254
26.92
42.8
9-3117
9.3414
0.2398
— 0.60
6.20
17 4206
22
11
17.1
15-3
18.1
16.4
16.72
43-5
8.9179
8.9491
0.1525
+ 0.38
7.18
10 3981
22
13
18.0
17.0
19-5
17.2
17.92
52-7
8.9762
9-0337
10 4351
22
36
24-5
20.1
21.7
20.4
21.68
48.1
9-1350
9.1776
16 4118
22
39
11.6
10.4
12.0
9-7
10.92
47.8
8.5550
8.5968
0.5048
+ 1.26
8.06
16 4119
22
41
16.3
16.2
18.6
15.6
16.68
47-7
8.9159
8-9574
0.1442
+ 0.36
7.16
12 4209
22
42
12.6
12.3
13.8
114
12.52
51-3
8.6721
8.7245
0.3771
+ 0.94
7-74
13 4259
22
43
15-4
13-3
15-7
14.2
14.65
50.7
8.8059
8.8563
0.2453
+ 0.61
7.41
15 4038
22
45
13.0
13-5
14.6
12.3
13-35
49.1
8.7268
8-7723
0.3293
+ 0.82
7.62
15 4O4O
22
46
21.4
20.3
21.4
19.0
20.52
49-5
9.0895
9.1362
0.0346
— 0.09
6.71
10 3981
22
48
18.0
1 6.4
17.4
17.0
17.20
57-3
8.9417
9.0190
IO 4351
22
50
21.6
21.4
22.7
20.0
21.42
49.6
9-1251
9.1721
Mittel aus den Vergleichsternbeobachtungen: 9.10315; 9.1056; 9.0956. Zur Reduction benutzt: 9.1016.
In der Mitte der Zone eine längere Unterbrechung durch Wolken.
Im Uebrigen scheinen die Messungen
unbedenklich zu sein.
Zone 168. 1887 October 21.
Beobachter : Kempf.
Photometer:
D. Vergleichsterne: Nr. 46 und Nr. 48. Luft:
2.
9° 5 11 1
23
55 m
21?4
2 2?I
2585
2 2?4
22885
44-9
9.1784
9.2 128
9 5277
23
57
23-7
22.0
23-5
23-3
23.12
42.9
9.1880
9.2179
17 4827
O
0
21 . 1
2 1.2
23.1
23.1
22.12
37-8
9-1516
9.1724
0.0030
+ 0.01
6.77
16 4833
O
1
23.6
23.2
24.8
24.2
23-95
38.8
9.2169
9-2393
0.0639
— 0.16
6.60
18 5067
O
3
15-3
I4.O
16.1
14-5
14.98
36.4
8.8249
8.8437
0.3317
+ 0.83
7-59
' ) il 4904
O
5
19.2
21.0
21.8
20.3
20.58
43-8
9.0919
9.1238
0.0516
+ 0.13
6.89
13 5024
O
7
12.0
12.0
14-5
1 1-5
12.50
41-5
8.6707
8.6978
0.4776
+ 1-19
7-95
13 5025
O
8
13.0
I 1*5
13-8
12.0
12.58
41.8
8.6761
8.7038
0.4716
+ 1.18
7-94
9 5111
O
9
20.2
19-5
21.2
20.4
2O.32
45-9
9.0813
9.1181
9 5277
O
11
20.6
21.5
22.7
2 1.1
21.48
43-2
9.1274
9-1579
10 4859
O
14
30.6
32.0
31-9
29.0
30.88
44-3
9.4207
9-4537
0.2783
— 0.70
6.06
14 4916
O
16
17.2
17.1
17-5
17.9
I7.42
41-3
8.9525
8-9793
0.1961
+ 0.49
7-25
19 5048
O
18
1 8.0
174
1 8. i
16.0
I7-38
36.8
8.9505
8.9698
0.2056
+ 0.51
7.27
19 5057
O
19
14-5
14.4
17-5
16.2
I5-65
36.2
8.8620
8.8805
0.2949
+ 0.74
7-50
15 4751
0
21
21.0
22.5
23-9
21.4
22.20
40.4
9.1546
9.1797
0.0043
— 0.01
6-75
15 4760
O
22
23.0
234
234
24.0
23-45
39-8
9.1997
9.2238
0.0484
— 0.12
6.64
9 5111
O
24
21.0
22.9
20.5
21.0
21-35
47.1
9.1224
9.1623
9 5277
O
25
22.0
22.0
23.0
21.5
22.1 2
43-8
9-1516
9 -i 835
Mittel aus den
Vergleichsternbeobachtungen: 9.2154; 9.1380; 9.1729. Zur Reduction benutzt: 9.1754
*) 1104904 dupl. Nur die helle Componente gemessen.
Zone 169. 1887 October 21.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 46 und Nr. 48. Luft: 1
— 2.
9° 5277
o h 3 1 m
20?0
20? 7
2 2? 6
20? 7
2 I ?00
44 ?o
9.1087
9.1410
9 5111
0
33
21-5
19-3
21.7
21.7
2 1.05
47-9
9.1107
9 -I 527
18 5105
0
35
14.4
13-5
13-7
13-5
I 3-78
38.6
8-7539
8.7760
o-3473
+ 0.87
7-63
17 4866
O
37
234
23.0
25-5
24-5
24.IO
39-3
9.2220
9.2452
0.1219
— 0.30
6.46
19 5058
O
38
22.4
20.6
23.1
20.8
2 I.72
38.1
9.1366
9-1579
0.0346
— 0.09
6.67
19 5060
O
40
20.6
17-5
20.2
17-5
18.95
37-5
9.0231
9.0434
0.0799
4- 0.20
6.96
10 4887
O
42
13-3
12.0
13-5
12.4
12.80
46.6
8.6909
8.7295
o -3938
-f - 0.98
7-74
17 4875
O
43
19.2
1 7.0
18.7
17-5
l8.IO
39-4
8.9846
9.0080
0-1153
+ 0.29
7-05
