140
Müller und Kempf, Photometrische Durchmusterung
140
B.D.
Stemzeit
1 1
n
III
IV
J
z
log sin 2 «/
corrig.
für Ext.
Diff.
in log.
Diff. in
Grossen
Grösse
Zone 36.
1886
November c
I-
Beobachter : Müller.
Photometer :
D. Vergleichsterne: Nr. 48 und Nr.
2. Luft:
3 -
9 °
47
2^ 3 111
2784
24?8
29?4
2583
26872
4785
9-3057
9.3466
9
5277
2 6
23-3
18.4
22.3
19.7
20.92
52.1
9 - 1 °5 5
9.1608
11
5090
2 IO
14.6
13.0
13-7
13.6
13.72
48.6
8.7501
8.7941
0-4543
+ I.I 4
7.66
11
5092
2 11
16.9
14.4
18.7
15.0
16.25
48.8
8.8938
8.9384
0.3100
-j- 0.78
7-30
13
5201
2 13
17.8
16.0
17.7
16.3
16.95
47.0
8.9294
8.9690
O.2794
+ O.70
7.22
i 4
5094
2 15
15.6
14.2
1 5-7
12.7
14-55
46.7
8.8001
8.8389
0.4095
+ 1.02
7-54
19
IO
2 17
17.0
15-9
17.0
15-5
16.35
42.1
8.8990
8.9273
O.3211
+ 0.80
7-32
i6
3
2 19
18.2
14-3
18.2
14.7
16.35
44-3
8.8990
8.9320
O.3164
+ O.79
7-31
9
5277
2 21
20.3
18.5
21.5
18.7
19-75
53-8
9.0576
9-“93
9
47
2 23
27-3
24.1
29.0
25.2
26.40
49.4
9.2960
9.3424
i6
11
2 25
24.6
20.5
22.4
18.3
2145
45-2
9.1263
9.1614
0.0870
+ 0.22
6-74
13
27
2 27
I 2.8
11.1
14-3
12.6
12.70
47.6
8.6842
8.7254
0.5230
+ 1-31
7-83
15
39
2 29
15-7
14-3
17-5
14-5
15-50
45-6
8.8538
8.8898
0.3586
-j- O.9O
7.42
19
38
2 30
19-3
17.8
19-5
17-5
18.52
42.4
9.0039
9.0328
0.2156
+ 0.54
7.06
11
34
2 32
21.4
19.4
21.6
21.4
20.95
49.1
9.1067
9.1522
0.0962
+ O.24
6.76
IO
25
2 34
27.4
24.0
32.0
2 7-5
27.72
50.7
9-3352
9-3856
O.1372
— 0.34
6.18
9
5277
2 36
20.8
18.6
22.3
19.4
20.28
55-7
9.0797
9- I 495
9
47
2 38
29.2
25.0
30-3
24.4
27.22
51.0
9.3206
9.3720
Mittel aus den Vergleichsternbeobachtungen: 9.2537; 9.2309; 9.2607.
Zur Reduction benutzt: 9.2484.
Zone
37 -
1886
November 23.
Beobachter: Keinpf. Photometer: D. Vergleichsterne: Nr. 46 und Nr. 48. Luft: 1-
—2.
9 °
51 1 I
o h i8 m
24?0
2898
2 7?0
2585
26832
4686
9-2935
9-3321
9
5277
0 22
22.3
24-5
27.8
23.1
24.42
43-7
9.2328
9.2644
*) 16 4746
0 25
20.5
16.6
19-5
17.7
18.58
43 -o
9.0066
9.0367
O.2901
+ 0.73
7-49
12
4838
0 27
25.8
27-5
25-5
25.6
26.10
46.6
9.2868
9-3254
O.OO14
0.00
6.76
!9
4949
0 29
29-5
25-3
26.6
28.5
27.48
40.4
9.3282
9-3533
0.0265
— 0.07
6.69
15
4670
0 31
28.0
27.4
28.4
32.0
28.95
44-4
9.3698
9.4030
0.0762
— 0.19
6.57
12
4843
0 32
17-5
16.5
20.0
17-5
17.88
46.6
8-9744
9.0130
O.3138
+ 0.78
7-54
13
4944
0 34
1 7*9
17.0
19-5
19.0
18.35
45-6
8.9961
9.0321
O.2947
+ 0.74
7-50
9
51 1 1
0 37
24.0
25.1
31-5
25-4
26.50
48.3
9.2991
9-3423
9
5277
0 39
25-3
25.6
28.9
27.9
26.92
44-5
9 - 3 ii 7
9-3451
19 4965
0 41
26.5
25.6
27.2
26.4
26.42
41.4
9.2966
9.3236
O.OO32
+ 0.01
6.77
IO
478 i
0 44
26.0
27-3
33-5
30.9
29.42
49.2
9-3825
9.4283
O.IO15
— 0.25
6.51
12
4850
0 46
21.0
21.0
22.4
22.1
21.62
48.1
9 - i 3 2 8
9-1754
O.1514
+ 0.38
7.14
11
4838
0 48
30.0
27.0
33-4
30.5
30.22
48.8
9-4037
9.4483
O.1215
— 0.30
6.46
18
5 OI 4
0 50
35-2
39-6
38.8
42.0
38.90
42.7
9-5959
9.6254
0.2986
— 0.75
6.01
18
5021
0 53
30.6
33 -i
36.0
32.5
33-05
42.9
9-4734
9-5033
O.1765
— 0.44
6.32
9
5m
0 55
24.7
25-3
28.4
28.6
26.75
50.1
9.3066
9-3551
9
5277
0 58
26.3
26.5
26.1
25-3
26.05
45-7
9.2853
9.3216
Mittel aus den Vergleichsternbeobachtunge
n: 9.2983; 9.3437; 9-3383.
Zur Reduction benutzt: 9.3268.
*) 16° 4746 dupl. Die hellere, vorangehende Componente gemessen.
Zone 38.
1886
November 23.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 46 und Nr. 48. Luft: 1
—2.
9 C
’5111
l h g m
21?7
20?0
20? 1
17?6
19885
5186
9.0618
9- 11 5 3
9
5277
1 11
18.0
i8.2
20.6
17.6
18.60
46.6
9.0075
9.0461
19 4982
1 14
14-3
12.0
15-7
12.1
13-52
45 -i
8-7377
8.7725
O.3226
-f- 0.81
7-57
14 4845
1 16
12.3
I 1.0
12.8
11.2
11.82
49.0
8.6228
8.6680
O.4271
+1-07
7-83
13
4974
1 18
26.5
25-4
27.9
26.3
26.52
50.2
9.2997
9-3485
O.2534
— 0.63
6.13
IO
4805
1 23
19.8
I7.6
21.5
17.6
19.12
53-6
9.0306
9.0915
O.OO36
+ 0.01
6.77
13 4983
l 25
16.4
13-5
14.7
14.6
14.80
50.8
8.8146
8.8654
O.2297
+ 0.57
7-33
18 5046
1 26
25-7
23-3
25-4
24.0
24.60
46.6
9.2388
9.2774
0.1823
— 0.46
6.30
9
5 111
1 29
20.7
19.8
19.0
17.4
19.22
54 -o
9.0349
9.0974
