136
Müller und Kempf, Photometrische Durchmusterung
136
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 26
1886 October 30.
Beobachter :
Müller
Photometer
D. Vergleichsterne: Nr.
2 und Nr.
4. Luft :
2.
9 °
47
22 h
5 2 m
2585
2 2?2
24-9
2784
25800
4685
9.2519
9.2902
IO
168
22
55
1 7 -i
14-3
15-5
14.4
15-32
50.2
8.8439
8.8927
6
105
22
57
29.0
22.6
26.2
25.6
25-85
50.5
9.2790
9.3288
O.2730
— 0.68
6.01
4
123
22
59
27-3
24-5
27.2
25.2
26.05
52.2
9-2853
9.3409
0.285 1
— O.71
5 - 9 8
i
149
23
2
11.6
10.3
12.2
10.4
I I.I 2
54-6
8-5705
8.6355
O.4203
+ 1-05
7-74
2
118
23
3
19-5
18.4
21.4
18.6
19.48
54 -o
9.0461
9.1086
0.0528
— O.13
6.56
3
120
23
5
12.6
12.2
13-7
12.4
I2.72
53-4
8.6855
8-7457
O.3101
+ 0.78
7-47
o
149
23
7
H -4
154
15-5
16.2
I 5-38
55-7
8.8472
8.9170
O.1388
+ O.35
7.04
9
47
23
9
23-7
21.2
23.2
21.4
22.38
45-3
9 - 1 6 1 3
9.1966
IO
168
23
11
13-7
13.6
17.6
14.6
14.88
48.5
8.8192
8.8629
6
135
23
13
16.4
15.0
18.8
17.7
16.98
50.4
8.9309
8.9804
O.0754
+ O.19
6.88
5
1 3 1
23
15
24.1
22.4
23.2
21.5
22 . 8 o
50.7
9.1766
9.2270
O.1712
— 0-43
6.26
i
185
23
17
11 -5
10.5
11.6
114
II.25
54-3
8.5805
8.6443
O.4115
+ 1-03
7.72
8
158
23
19
14.0
12.0
15-1
16.1
I4.3O
48.4
8.7854
8.8289
O.2269
+ 0-57
7.26
8
159
23
20
16.9
15-3
16.7
15.2
IÓ .02
48.1
8.8817
8.9243
O.I 3 I 5
+ 0-33
7.02
4
166
23
22
10.5
10.6
114
10.3
IO.7O
51.8
8-5375
8.5917
O.4641
+ 1.16
7-85
9
47
23
24
22.9
22.2
234
21.4
22.48
44.4
9 -% 5 °
9.1982
IO
168
23
27
16.6
15-5
15.6
144
I 5-52
46.9
8.8549
8.8942
Mittel aus den Vergleichsternbeobachtunge
n: 9.0915; 9.0297; 9.0462.
Zur Reduction benutzt: 9.0558.
Zone 27
1886 October 31
Beobachter : Kempf.
Photometer :
D. Vergleichsterne: Nr. 2
und Nr. 4
Luft : 2
- 3 -
9 °
47
23 b
2I m
28?0
29?3
3 °?i
2880
28885
44 %
9-3671
9.4008
IO
168
23
24
18.9
18.0
19.1
17.7
18.42
47.2
8.9993
9.0394
5
141
23
27
19-5
16.5
16.6
18.5
17.78
49.9
8.9696
9.0175
O.2082
+ O.52
7.21
*)o
174
23
30
29.2
274
32.9
29.2
29.68
54-8
9-3895
9-4554
O.2297
— 0-57
6.12
i
203
23
32
17-5
15-3
1 7.0
16.5
16.58
53-9
8.9108
8.9729
O.2528
+ O.63
7-32
4
172
23
35
29.9
31-5
30-5
32.3
3 I -05
50-5
9.4250
9.4748
O.2491
— O.62
6.07
**\ A
23
38
22.7
23-5
23-5
23.1
23.20
51.0
9.1909
9.2423
O.OIÓ6
— 0.04
6.65
) 4
1 7 j
23
39
16.6
16.0
17-3
16.8
16.68
50-9
8.9159
8.9670
O.2587
+ O.65
7-34
7
167
23
42
18.1
17.0
20.1
20.0
18.80
47-5
9.0164
9-0573
O.1684
+ O.42
7-1
9
47
23
45
28.5
29.6
294
28.9
29.10
43-5
9-3739
9.4051
IO
168
23
48
18.1
174
20.9
17.7
18.52
45 -i
9.0039
9.0387
8
173
23
5 i
13-5
12.5
13.0
13-5
13.12
46-3
8.7120
8.7498
0-4759
+ 1.19
7.88
i
212
23
54
25.0
21.8
27.2
22.3
24.08
52-9
9.2213
9-2795
O.0538
— 0.13
6.56
9
132
23
56
21.0
21.7
22.1
21.4
21-55
45-2
9.1301
9- 1 65 2
O.0605
+ O.15
6.84
8
177
23
58
14.7
14-5
16.5
13-9
14.90
45-3
8.8203
8.8556
O.3701
+ o -93
7.62
4
190
O
1
37-8
37 -°
35-6
40.0
37.60
49.1
9-5709
9.6164
O.3907
— 0.98
5-71
i
221
O
4
27-5
28.4
29-5
30.0
28.85
52.1
9.3671
9.4224
O.1967
— 0-49
6.20
9
47
O
7
27.9
25.6
30.0
304
28.48
42.9
9-3567
9.3866
IO
168
O
9
19.0
17.6
22.4
19-5
19.62
43-6
9.0521
9-0835
Mittel aus den Vergleichsternbeobachtungen: 9.2201 ; 9.2219; 9.2351.
Zur Reduction benutzt: 9.2257.
*) o°
174 dupl. Nur die hellere Componente gemessen
**) 4
175 dupl. Zuerst die vorangehende Componente gemessen.
Zone 28
1886 October 31
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 4
und Nr. 6.
Luft : 2-
- 3 -
io‘
168
O 1
17™
1384
1380
14-5
1584
14808
43 %
8.7722
8.8025
8 385
O
20
22.4
22.3
22.5
2 1.2
22.10
50.1
9.1509
9.1994
8
183
O
22
14-3
1 1-7
134
11.2
12.65
44.4
8.6809
8.7141
0.3080
+ 0-77
7-45
9
138
O
23
19.4
16.7
18.1
17.0
17.80
43-6
8.9706
9.0020
0.0201
+ 0.05
6-73
1
223
O
25
18.3
15-7
17-5
16.0
16.88
51-3
8.9259
8.9783
O.O438
+ 0.11
6.79
6
181
O
27
22.5
21.4
23-5
21.5
22.22
46.8
9-1553
9- I 944
O.I723
— 0.43
6.25
0
210
0
29
16.7
15.0
15.0
154
15-52
52.8
8.8549
8.9128
O.IO93
+ 0.27
6-95
9
142
O
31
134
1 2.2
134
13.2
13-05
44.0
8-7075
8.7398
O.2823
+ 0.71
7-39
