252
Müller und Kempf, Photometrische Durchmusterung
252
B.D.
Sternzeit j
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log. 1
Diff. in
Grössen
Grösse
9 °
472
3 h 6 m
i6?8
I5?2
i6?7
1589
16? 15
4381
8.8886
8.9189
11
632
3 8
20.5
19.9
21.4
20.2
20.50
44-4
9.0887
9.1219
o
721
3 10
14.9
15.6
15.6
15.0
15.28
53-7
8.8417
8.9030
0.1156
+ O.29
7-54
5
614
3 12
27.0
23-7
27.0
25.0
25.68
48.0
9.2737
9.3160
0.2974
— O.74
6.51
5
613
3 13
18.9
17.9
19-3
16.6
18.18
47-9
8.9883
9.0303
0.0117
— O.03
7.22
5
631
3 15
34 -o
33-6
34 -o
31-5
33-28
48.1
9-4787
9 - 52 I 3
O.5027
— 1.26
5-99
9
558
3 17
22.0
19.4
21.8
21.0
21.05
44.6
g.i 107
9.1444
O.1258
— O.31
6.94
9
562
3 18
27.0
26.9
26.5
26.2
26.65
44.0
9.3036
9-3359
0 . 3 I 73
— O.79
6.46
8
672
3 19
23.8
22.0
23-9
21.8
22.88
44.9
9-1795
9.2139
0.1953
— O.49
6.76
9
472
3 21
17.7
l6.0
17-5
14.8
16.50
42.8
8.9067
8.9364
11
632
3 23
21.1
I9.2
19.6
19-3
19.80
43-3
9-0597
9.0905
Mittel aus den
Vergleichsternbeobachtungen : 9.0219
; 9.0204; 9.0134. Zur Reduction benutzt: 9.0186.
Zone 318
. 1889 Januar 13.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 2 und Nr. 4.
Luft: 1—
-2.
9 °
47
4 40™
3083
2880
2984
2Ó?4
28852
45°6
9-3579
9-3939
IO
168
1 42
19.8
i8.2
18.6
ig.6
19.05
41.7
9.0275
9-0550
15
69
1 46
2 1.0
I9.4
21.2
18.8
20.10
40-3
9.0723
9.0972
0.1339
+ O.33
7.02
i 5
73
1 47
19.8
i8.2
19.9
18.2
19.02
40.3
9.0262
9-0511
0.1800
+ 0.45
7.14
IO
57
I 49
I 7.0
I4.6
18.0
15-3
16.22
44-7
8.8922
8.9261
0.3050
+ O.76
7-45
12
47
I 51
16.7
16.O
17.4
16.2
16.58
43-6
8.9108
8.9422
0.2889
4~ O.72
7.41
18
67
i 53
21.4
21-5
22.0
20.5
21-35
37-4
9.1224
9.1426
0.0885
+ 0.22
6.91
i 7
67
1 55
I9.9
19.0
2 2.0
20.4
20.32
38.3
9.0813
9.1029
0.1282
+ 0.32
7.01
9
47
i 57
29.I
28.7
29-3
28.8
28.98
46.9
9.3706
9.4099
IO
168
i 59
19.7
20.5
20.5
17.8
19.62
42.3
9.0521
9.0808
15
74
2 2
20.8
20.0
21-3
17.8
19.98
41-3
9.0673
9.0941
O.137O
+ 0.34
7-03
i 3
69
2 3
12.5
II .9
12.8
11.6
12.20
43-5
8.6499
8.6811
0.5500
+ 1-38
8.07
13
73
2 5
12.6
10.0
13.0
12.0
11.90
43 -i
8.6286
8.6589
0.5722
+ i -43
8.12
12
57
2 7
24.8
23.8
25-5
24-3
24.60
44.2
9.2388
9.2716
O.O405
— 0.10
6-59
12
59
2 9
24.9
24.0
26.3
24.0
24.80
44-5
9-2454
9.2788
O.O477
— 0.12
6-57
l 9
83
2 11
13-3
10.5
11.8
11.6
11.80
38.2
8.6214
8.6428
O.5883
4 ~ i -47
8.16
9
47
2 13
29.2
27.0
28.2
27.2
27.90
48.3
9.3404
9-3836
IO
168
2 16
19.6
17-5
20.6
19.0
19.18
43-2
9-0331
9.0636
Mittel aus den Vergleichsternbeobachtungen
: 9.2245
; 9 - 2453 ; 9-2236.
Zur Reduction benutzt: 9.2311
Zone 319. 1889 Januar 13.
Beobachter : Müller.
Photometer :
D. Vergleichsterne: Nr. 2
und Nr. 4.
Luft: I-
—2.
i o°
168
21138m
19?6
1985
2185
2 o?o
20815
4486
9.0744
! 9.1081
9
47
2 41
29.0
28.8
29-3
29.0
29.02
5 1.1
9 - 37 I 7
9-4234
i 4
76
2 43
30.8
314
31.8
30-9
31.22
46.0
9.4292
9.4662
0.2228
— 0.56
6.13
IO
65
2 45
17.9
17.0
1 7.6
15-9
1 7.10
49-5
8.9368
8-9835
O.2599
4- 0.65
7-34
IO
70
2 47
15-4
13.6
15.6
13-3
14.48
49-4
8.7960
8.8424
O.4OIO
4 - 1.00
7.69
i 5
106
2 49
24-5
23.0
23.6
21.8
23.22
44.6
9.1916
9-2253
O.Ol8l
+ 0.05
6-74
12
87
2 51
15-3
134
15-3
13-9
14.48
47.6
8.7960
8.8372
O.4062
4- 1.02
7.71
18
IOI
2 53
28.9
27.1
28.8
26.4
27.80
42.1
9-3375
9-3658
0.1224
— 0.31
6.38
9
47
2 55
28.3
28.1
27.0
26.2
27.40
52.7
9-3259
9-3834
IO
168
2 57
19.8
18.5
19-5
17-3
18.78
46.2
9 -OI 55
9.0530
18
103
2 59
14.0
13-5
14.8
12.5
1340
43-3
8.7489
8.7797
O.4637
-f- i. 16
7.85
17
105
3 i
13.0
12.6
15.0
12.0
I 3 -I 5
43-6
8.7140
8-7454
O.4980
+ 1.25
7-94
17
106
3 3
12.5
10.6
13.2
11.7
I 2.00
44.2
8.6358
8.6686
O.5748
4 - i -44
8.13
i 4
11 7
3 5
18.8
18.2
18.0
18.8
18.45
47-4
9.0007
9.0414
1 0.2020
+ 0.51
7.20
11
106
3 7
21.0
18.9
19.9
19.0
I9.7O
49.1
9-0555
9.1010
O.I424
4- 0.36
7-05
12
104
3 9
15-2
13-9
16.3
12.4
1445
48.5
8-7943
8.8380
O.4O54
4 - 1.01
7.70
9
47
3 u
28.2
28.7
26.3
29-5
28.18
54.6
9-3483
9-4133
IO
168
3 14
20.0
19.0
19-5
18.6
19.28
47-8
9-0375
9-0793
Mittel aus den Vergleichsternbeobachtungen: 9.2658; 9.2182; 9.2463.
Zur Reduction benutzt: 9.2434.
