138
Müller und Kempf, Photometrische Durchmusterung
138
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 31.
1886
November i
Beobachter: Kempf. Photometer: D
Vergleichsterne: Nr. 40 und Nr. 42. Luft: 2
— 3 -
IO°
3981
2l“
22 ra
20?9
1985
2385
2I?0
21822
4782
9-1173
9-1574
IO
4351
2 I
25
23-5
25.0
24.7
24.O
24.30
42.8
9.2288
9-2585
15
3721
21
28
15-9
15.0
* 7-5
15-1
15-88
46.2
8.8743
8.9118
0.2946
+ 0.74
7-54
3887
21
30
15-9
14.6
16.0
15.0
I 5-38
44.4
8.8472
8.8804
0.3260
4- 0.82
7.62
16
3775
21
32
20.4
19.0
24.0
19.4
20.70
45-6
9.0967
9 -I 327
0.0737
4-0.18
6.98
11
3775
21
34
19.0
18.0
18.5
18.4
18.48
5°-6
9.0021
9.0522
0.1542
+ 0.39
7- I 9
14 3829
21
36
22.6
22.9
24.0
22.4
22.98
47.6
9.1831
9.2243
0.0179
— 0.04
6.76
14
3830
21
38
18.9
18.6
20.5
17.8
18.95
47-9
9 - 023 1
9.0651
0.1413
4-0.35
7-15
IO
3981
21
40
19.8
21.3
23-5
20.0
21.15
49.0
9.1146
9.1598
IO
4351
21
42
22.0
23-5
23-9
21.0
22.60
43-7
9- l6 93
9.2009
14 3831
21
45
15.8
15-4
16.0
15.0
15-55
49.0
8.8565
8.9017
0.3047
4-0.76
7-56
19
3949
21
47
13.0
13-1
1 1-5
12.0
12.40
44-5
8.6638
8.6972
0.5092
4 -1-27
8.07
11
3778
21
49
20.5
21.6
20.4
21.0
20.88
51-9
9.1039
9 -Ì 584
0.0480
4- 0.12
6.92
18 3998
21
52
1 5-1
15.2
17-5
15.0
15-70
46.1
8.8647
8.9020
0.3044
4-0.76
7-56
IO
3839
2 I
54
18.2
17-5
15.6
16.0
16.82
53-6
8.9229
8.9838
0.2226
4-0.56
7-36
15
3743
21
56
15-7
15.0
17.2
16.5
16.10
48.9
8.8859
8.9308
0.2756
4- 0.69
7-49
IO
3981
22
1
20.9
21.5
23-5
20.0
21.48
51-3
9- I2 74
9.1798
IO
4351
22
3
22.8
23-5
27-5
25.6
24.85
45-2
9.2470
9.2821
Mittel aus den Vergleichsternbeobachtungen: 9.2080; 9.1803; 9.2310. Zur Reduction benutzt: 9.2064.
Zone 32.
1886 November i.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 2
— 3 -
IO°
4351
2 2^
9 m
2I?4
ig?o
2 I ?2
20? 2
2 o ?45
4588
9.0867
9.1232
IO
398 i
22
11
17.4
17-3
18.7
16.8
1 7-55
52.5
8.9587
9.0154
12
4225
22
14
1 3-7
12.0
13.6
1 1-5
12.70
48.0
8.6842
8.7265
0.3359
4- 0.84
7.64
12
4226
22
15
11-7
14-3
13-3
13-7
13-25
48.0
8.7204
8.7627
0.2997
+ 0.75
7-55
12
4229
22
16
15-4
12.4
13-5
15-4
14.18
47.6
8.7782
8.8194
0.2430
4- 0.61
7.41
IO
4180
22
18
14.6
14.0
16.3
15-2
15.02
50.0
8.8271
8-8753
0.1871
+ 0.47
7.27
15
4047
22
20
12.4
11.4
12.6
12.0
12.10
45-7
8.6429
8.6792
0.3832
4- 0.96
7.76
I 6
4150
22
22
13.6
13-7
15-5
14.6
I 4-35
45-4
8.7884
8.8240
0.2384
4- 0.60
7.40
IO
398 i
22
24
16.3
16.8
18.6
17.4
17.28
54 -i
8.9456
9.0085
IO
4351
22
27
20.0
18.0
20.8
19.4
19-55
47-4
9.0492
9.0899
16
4153
22
29
24-3
22.5
21.5
20.7
22.25
46.1
9- 1 5 65
9.1938
0.1314
— 0.33
6.47
IO
4189
22
3 1
21.4
21.3
21.2
21.8
21.42
51-5
9-1251
9.1782
0.1158
— 0.29
6.51
IO
4192
22
32
12.3
1 1-3
11.2
11.1
11.48
51-5
8.5978
8.6509
0.4115
4 -1-03
7-83
11
4153
22
34
13-5
12.8
13.2
13.0
13.12
50.4
8.7120
8.7615
0.3009
4-0.75
7-55
16 4162
22
36
16.7
14.0
16.3
14.0
15-25
46.6
8.8400
8.8786
0.1838
-f- 0.46
7.26
18
4402
22
38
I 5 - 1
15.6
15-7
15-4
1 5-45
45 -i
8.8511
8.8859
0.1765
4-0.44
7.24
IO
398 i
22
40
18.5
17. 1
20.2
15.8
1 7 - 9 °
56.2
8-9753
9-°473
IO
4351
22
42
21.8
17.4
19.4
19.2
I 9-45
48.9
9.0449
9.0898
Mittel aus den Vergleichsternbeobachtungen: 9.0693; 9.0492; 9.0686. Zur Reduction benutzt: 9.0624.
Zone 33. 1886 November
I.
Beobachter: Kempf.
Photometer: 1 ). Vergleichsterne: Nr. 42 und Nr. 44
Luft: 2-
- 3 -
io c
’4351
2 2
'46™
2485
2185
2684
2382
23890
4983
9.2152
9.2613
IO
4604
22
49
26.9
26.4
29.I
25.8
27.05
44-5
9 - 3 I 56
9.3490
*)i 5
4251
22
52
14.0
14.0
15-7
14.1
14-45
45 -i
8-7943
8.8291
O.4771
4 - 1.19
7.67
14
4419
22
54
13.0
IO.I
13.2
11-5
ii -95
46.2
8.6322
8.6697
O.6365
4 - i -59
8.07
12
4465
22
56
14-5
14.7
14.O
13-3
14.12.
48.0
8.7746
8.8169
0.4893
-f- 1-22
7.70
15
4257
22
58
14.4
13.6
16.O
13.0
14.25
45-4
8.7824
8.8180
0.4882
4- 1-22
7.70
11
4389
23
0
12.6
13-4
15.O
14.6
13.90
49-3
8.7612
8.8073
0.4989
4 -1-25
7-73
14
4433
23
2
17.6
16.5
20.5
16.9
17.88
47.0
8.9744
9.0140
O.2922
4 - 0.73
7.21
IO
4351
23
5
23.0
23.0
24-5
25.0
23.88
51-4
9.2145
9.2673
IO
4604
23
9
23.6
24.7
28.3
27.8
26.10
46.0
9.2868
9-3238
