194
Müller und Kempf, Photometrische Durchmusterung
194
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
I)iff. in
Grössen
Grösse
Zone 172
1887 October 25
#
Beobachter: Müller.
Photometer :
D. Vei
gleichsten^ : Nr. 44 und Nr. 46. Luft :
3 -
IO°
^1"
0
0
■xf"
2 3 h
9 m
2587
22?5
2384
21?6
23830
4680
9- I 944
9.2314
9
5111
2 3
12
19.4
l8.6
21.3
: 7-3
I9-I5
42.9
9.0319
9.0618
13
4781
23
14
17.6
15-7
20.4
18.5
18.05
43-4
8.9823
9-OI33
0.1403
+ 0-35
6.89
16 4598
23
16
24.4
22.2
22.6
21.3
22.62
40.2
9.1700
9.1948
0.0412
O.IO
6.44
15
45°5
23
17
16.2
16.2
18.5
1 73
17-05
41-5
8.9344
8.9615
0.1921
—f- 0.48
7.02
19
4793
23
19
22.4
21.5
24.6
21.6
22.52
37-3
9.1664
9:1864
0.0328
— 0.08
6.46
18 4871
23
20
12.5
12.8
I4.6
14.8
13.68
38.3
8-7477
8.7693
0.3843
-f- 0.96
7-50
11
4677
23
21
11*9
10.5
I2.9
10.7
11.50
45-i
8-5993
8.6341
0.5195
+1.30
7.84
IO
4604
23
23
25.1
24.8
24.9
23.0
24-45
47-2
9.2338
9-2739
9
511 1
23
25
20.6
19.0
19-5
18.0
19.28
43-3
9-0375
9.0683
IO
4645
23
26
18.6
18.2
19.1
17.4
18.32
46.4
8.9947
9.0327
0.1209
+ 0.30
6.84
18 4874
23
28
17.6
16.8
18.2
16.5
17.28
39- 1
8.9456
8.9685
0.1851
+ 0.46
7.00
15
4519
23
30
18.3
154
1 7.6
17.6
17.22
42.1
8.9427
8.9710
0.1826
+ 0.46
7.00
19 4809
23
3 1
15.0
14.6
15-2
15-3
15.02
38.1
8.8271
8.8484
0.3052
+ 0.76
7-30
12
47 11
23
33
19.6
19.2
18.9
17.2
18.72
45-3
9.0129
9.0482
0.1054
4- 0.26
6.80
17 4657
23
34
11.8
10.0
12.2
10.0
11.00
40.6
8.5612
8.5867
0.5669
+ 142
7.96
IO
4604
23
36
26.5
2 1.2
24.4
22.2
23-58
48.4
9.2042
9.2477
9
51”
23
38
19.7
I7.4
19.0
18.2
18.58
43-9
9.0066
9.0387
Mittel aus den Vergleichsternbeobachtungen
: 9.1466; 9.1 71 1 ; 9.1432. Zur Reduction benutzt: 9.1536.
Zone 173
. 1887 October 26.
Beobachter: Kempf. Photometer: D
Vergleichsterne: Nr. 38 und Nr. 40
Luft: 2
—3-
IO°
3573
20'
5 2 m
22? 5
2380
2584
22?I
23825
UT
O
• O
u»
9.1927
9.2425
IO
3981
20
55
20.8
I9.7
22.5
20.6
20.90
44.8
9- io 47
9.1388
14
3846
20
57
37-6
38.O
38.2
37-o
37-70
43-i
9.5728
9.603 1
0.4259
— 1.06
5.78
19
3956
20
58
29.2
29.6
29.0
30-5
29.58
38.6
9.3869
9.4090
0.2318
— 0.58
6.26
19
3959
2 I
0
17.0
16.O
1 7-5
15-5
16.50
39-4
8.9067
8.9301
0.2471
-f- 0.62
7.46
18
4014
2 I
2
19.4
I7.O
19-5
18.4
18.58
39-9
9.0066
9.0308
0.1464
+ 0.37
7.21
18
4011
2 I
3
24.2
21.6
23-5
24.0
23-32
40.5
9-195 1
9.2204
0.0432
O.I I
6-73
15
3747
2 I
4
1 7-5
I 7.O
17. 1
16.9
I 7.1 2
42.7
8.9378
8.9673
0.2099
+ 0.52
746
IO
3573
2 I
6
22.5
22.0
23.1
21.1
22.i8
52.1
9- 1 5 39
9.2092
IO
3981
2 I
8
20.0
19.8
20.8
19.4
20.00
45-9
9.0681
9.1049
16
3809
2 I
10
15.0
15.0
14.6
14.1
14.68
42.5
8.8076
8.8367
■0.3405
4-0.85
7.69
IÓ 3812
2 I
12
16.5
17.8
19-5
18.6
18.IO
42.9
8.9846
9.0145
0.1627
4- 041
7-25
15
3762
2 I
13
13-5
13.0
13-1
12.2
12.95
43-8
8.7009
8.7328
0.4444
4 - i.11
7-95
19
3975
21
15
23-5
I9.7
21.5
22.6
2 1.82
40.5
9.1404
9-1657
0.0115
4- 0.03
6.87
13
3981
2 I
17
15-1
I4.9
16.9
I4.4
Ì 5-32
45-5
8.8439
8.8797
0.2975
4- 0.74
7.58
11
3801
2 I
19
14.6
15.0
15-1
T 4-5
14.80
47.6
8.8146
8.8558
0.3214
4- 0.80
7.64
IO
3573
2 I
22
23.0
22.5
21.5
21.5
22.12
54- 1
9-1516
9.2145
IO
3981
2 I
25
1 22.5
2O.4
2 1 .4
20.1
21.10
47-4
9.1126
9-1533
Mittel aus den
Vergleichsternbeobachtungen: 9.1907; 9.1570; 9.1839.
Zur Reduction benutzt: 9.1772.
Zone 174
1887 October 26.
Beobachter: Mùllér. Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 2
- 3 -
IO C
398 1
2 p
29 m
18?7
I 784
i8?3
1784
17895
4788
8.9777
9.0195
IO
4351
2 I
32
19-5
20.4
21.6
20. 1
20.40
43-i
9.0846
9- 1 x 49
14 3948
21
34
12.7
11-5
12.6
10.7
11.88
45-4
8.6272
8.6628
0.4140
-b i -04
7.84
15
386Ó
2 1
37
15.8
15.8
17-3
15-4
16.08
44-3
8.8849
8.9179
0.1589
4- 0.40
7.20
15
3868
21
39
9.6
7-7
9-5
8.5
8.82
45-i
8.3712
8.4060
0.6708
4- 1.68
8.48
16
3902
2 I
41
14.6
13.6
15-5
13-7
14-35
44.2
8.7884
8.8212
0.2556
4-0.64
7-44
17
4009
2 I
43
14.0
13.2
14-3
14.4
13.98
43-2
8.7662
8.7967
0.2801
4-0.70
7-50
IO
3967
21
45
15.0
15.0
16.6
14-5
15.28
49.9
8.8417
8.8896
p
CO
4-0.47
7.27
IO
398 1
21
46
17.6
17.9
19.6
17.4
18.12
49.6
8-9855
9-0325