130
Müller und Kempf, Photometrische Durchmusterung
130
B.D.
Sternzeit
I
II
III
IV
J
z
1 log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 11.
1886 October 20
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft:
1.
io° 3981
2 P
9 m
I 6?2
i 5°7
1780
1584
i6?o8
4680
8.8849
8.9219
10 4351
2 1
11
21-4
19.6
22.0
18.5
20.38
42.2
9.0838
9 -II 23
9 4526
21
15
23.O
20.3
234
22.9
22.40
44.1
9.1620
9*1945
0.1485
— 0.37
6-43
2 4164
2 1
16
17-5
17.7
18.6
15.6
17-35
51*1
8.9491
9.0008
0.0452
-f- O.I I
6.91
2 4175
21
18
20.3
20.4
22.6
20.0
20.82
5 ii
9*1015
9 -I 532
0.1072
— 0.27
6-53
7 4477
21
19
27.4
234
24.7
22.4
24.48
45-8
9.2348
9 - 27 I 3
0.2253
— 0.56
6.24
0 4515
2 1
21
13-3
12.4
I2.3
12.4
12.60
53-3
8.6775
8-7373
0.3087
+ 0.77
7-57
2 4179
2 1
24
14.5
12.4
16.O
14.0
14.22
51-4
8.7806
8.8334
0.2126
+ 0.53
7-33
10 3981
21
26
16.6
15-5
l8.6
16.3
16.75
47.6
8.9194
8.9606
10 4351
2 1
28
21.4
20.5
22.5
20.4
21.20
42.9
9-1165
9.1464
9 4551
2 1
30
17-5
17.7
18.4
18.9
18.12
44-5
8-9855
9.0189
0.0271
+ 0.07
6.87
3 4356
21
32
13-4
13-7
I4.6
13-5
13.80
50.3
8-7551
8.8043
0.2417
4- 0.60
7.40
1 4310
2 1
34
21.0
20.6
23.6
18.6
20.95
52.5
9.1067
9.1634
0.1174
— 0.29
6.51
4 4486
2 1
37
19-5
18.4
20.5
20.6
19-75
49.9
9.0576
9-1055
0.0595
— 0.15
6.65
9 4579
2 1
39
19.8
17-5
18.5
18.3
18.52
45 -o
9.0039
9-0385
0.0075
+ 0.02
6.82
10 3981
2 1
41
16.4
16.4
l8.8
15.6
16.80
49.1
8.9219
8.9674
10 4351
21
43
22.6
20.3
23-7
20.2
21.70
43-7
9 -I 358
9.1674
Mittel aus den Vergleichsternbeobachtungen: 9.0171; 9.0535; 9.0674.
Zur Reduction benutzt: 9.0460.
Zone 12.
1886 October 20
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 42
und Nr. 44. Luft:
2 — 3 -
i °°435 i
2 I 11
51“
2 6?6
2385
2789
2 9?o
26875
4484
9.3066
9-3398
10 4604
2 I
54
33 -o
29.0
33 -o
26.5
30.38
42.2
9.4079
9.4364
2 4311
21
57
25.0
22.5
29.0
27-5
26.00
5 ii
9.2837
9-3354
0.0358
4- 0.09
6-57
9 4735
21
59
29.4
29.2
33-8
30.1
30.62
44.2
9.4140
9.4468
0.0756
— 0.19
6.29
3 4514
22
2
16.1
12.5
154
15.0
14-75
50.4
8.8117
8.8612
0.5100
4-1.27
7-75
*) 8 4625
22
5
15.8
13.2
15-9
14.0
14.72
45 -o
8.8100
8.8446
0.5266
4 -1*32
7.80
2 4319
22
8
1 7-1
16.5
21.5
19-5
18.65
51.8
9.0098
9.0640
0.3072
+ 0.77
7-25
6 4776
22
IO
19.0
19.0
21.2
17.7
19.22
47-3
9.0349
9-0753
0.2959
4-0.74
7.22
10 4351
22
14
27.0
234
24.0
28.0
25.60
46.2
9.2711
9.3086
10 4604
22
17
27.4
28.5
32.9
30.1
29.72
42.9
9-3905
9.4204
4 4639
22
21
14-5
13-1
16.5
14-5
14.65
49-7
8.8059
8.8532
0.5180
4 -1-30
00
9 4769
22
24
19.4
19.0
19.6
20.5
19.62
45-0
9.0521
9.0867
0.2845
4-0.71
7.19
8 4651
22
28
18.8
20.4
23.8
194
20.60
45-9
9.0927
9.1295
0.2417
4- 0.60
7.08
**)6 4802
22
30
34-9
32.6
39 -o
31.6
34-52
48.0
9.5067
9.5490
0.1778
— 0.44
6.04
9 4786
22
33
22.6
21.1
27.7
22.5
23.48
45-3
9.2007
9.2360
0.1352
4-0.34
6.82
0 4714
22
36
22.0
19-5
22.4
19-5
20.85
54 -i
9.1027
9.1656
0.2056
+ 0.51
6.99
10 4351
22
39
1 24-5
25.2
29.6
26.0
26.32
48.6
9-2935
9-3375
10 4604
22
41
28.2
1 27.2
30.0
27.9
28.32
44.0
9-3523
9.3846
Mittel aus den Vergleichsternbeobachtungen: 9.3881; 9.3645; 9.3611.
Zur Reduction benutzt: 9.3712.
*) 8°4625 dupl., als ein
Stern gemessen. Unsicher.
**j 6 4802.
Die röthliche Farbe erschwert die Messungen.
Zone 13
. 1886 October 20
#
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 48 und Nr. 2. Luft: 1
—2
9 ° 5 2 77
o ll 47 m
1980
1985
2I?6
i8?4
19862
458 o
I 9-0521
9.0867
9 47
0
50
25.I
23.6
24.6
234
24.18
43 -i
9.2247
9-2550
*)8 19
0
53
24.4
26.9
29.6
254
26.58
45-2
1 9 - 30 I 5
9.3366
0.1742
— 0.44
6.08
3 26
0
55
13-5
16.3
14.6
13-7
14.52
49-7
8.7984
8.8457
0.3167
4-0.79
7-31
7 27
0
57
21.2
24.6
27.7
23.0
24.12
45-8
9.2227
9.2592
0.0968
— 0.24
6.28
1 28
0
59
17-5
13.0
13.6
14.7
14.70
52.1
8.8088
8.8641
0.2983
+ 0.75
7.27
9 21
1
1
18.6
19.8
23-5
20.4
20.58
44.0
9.0919
9.1242
0.0382
4- O.io
6.62
9 22
1
3
134
1 2.8
13.6
13.6
13-35
44.0
8.7268
8-7591
04033
+ I.OI
7-53
9 5277
1
5
17.2
16.7
20.0
17.6
17.88
46.2
8.9744
9.0119
