294
Müller und Kempf, Photometrische Durchmusterung
294
B.D.
Sternzeit
I
II
HI
IV
J
Z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
IO°
1149
31148m
31%
I
VTS
c •
CO
CNJ
3 1°°
3080
30828
5282
94053
9.4609
i 3
11 73
3 51
31.8
U~>
CO
cm
31.2
33 -o
31.12
47-3
9.4267
9.4671
0.0351
4- 0.09
6.18
14
1235
3 53
27.0
25-5
28.4
27.7
27-15
46.9
9.3186
9-3579
0.1443
+ 0.36
6-45
14
1233
4 0
24.2
21.2
24.0
22.6
23.00
46.3
9.1838
9.2216
0.2806
+ 0.70
6.79
1 2
1081
4 2
37-5
35-7
37-5
36.0
36.68
47-4
9-5525
9-5932
0.0910
— 0.23
5-86
12
1084
4 4
45-2
44.0
454
46.0
45-15
47-3
9-7013
9.7417
0.2395
— 0.60
5-49
IO
1071
4 6
22.5
19-5
20.4
19-3
20.42
48.9
9.0854
9-1303
0.3719
+ 0.93
7.02
IO
818
4 9
35-5
33-5
33 -i
34-5
34-15
45-2
9.4985
9-5336
IO
1149
4 u
30.9
27-5
29-3
28.0
28.92
49.6
9.3689
9-4159
Mittel aus den Vergleichsternbeobachtungen: 9.5084; 9.5234; 9.4747.
Zur Reduction benutzt: 9.5022.
Zone 423. 1891 Februar 5
Beobachter:
Müller. Photometer
: D. Vergleichsterne: Nr.
12 und Nr. 14. Luft
: 1.
IO°
1149
4" 14 m
25-5
2 2?0
2389
22? 7
23852
49-3
9.2021
9.2482
IO
818
4 18
30.1
29.0
30.0
32.1
3 °- 3 °
44.6
9.4058
9-4395
17
1203
4 20
23-9
20.5
24-3
20.4
22.28
41.4
9-1576
9.1846
0.1583
4- 0.40
6-49
17
1214
4 22
23.1
19.7
23-9
21.8
22.12
41.1
9-1516
9.1780
0.1649
+ 0.41
6.50
17
1224
4 23
14.2
15.0
16.5
15-7
15-35
4 i -3
8.8456
8.8724
0.4705
4- 1.18
7.27
17
1235
4 25
16.0
14-5
17.7
15.0
15.80
41.8
8.8700
8.8977
0.4452
4 - 1.11
7.20
16
1135
4 27
21.7
21.2
23-9
23.2
22.50
42.5
9-1657
9.1948
0.1481
+ 0.37
6.46
16
1091
4 29
18.4
16.4
20.4
18.2
18.35
41.8
8.9961
Q.0238
0.319!
4- 0.80
6.89
IO
1149
4 3 i
23.6
23-3
26.6
24.8
24.58
47.6
9.2381
9-2793
IO
818
4 33
29.7
27.7
31-3
32.9
3040
43-7
9.4084
9.4400
19
1313
4 37
14-3
12.0
14.9
134
13-65
37-6
8.7458
8.7663
0.5766
+ i -44
7-53
13
H99
4 39
16.0
15.0
16.7
16.5
16.05
43-2
8.8833
8.9138
0.4291
+ 1.07
7.16
13
1200
4 40
12.9
IO.5
14.1
11.8
12.32
43 -i
8.6583
8.6886
0.6543
+ 1.64
7-73
12
1123
4 44
24-5
24.I
24.7
24-3
24.40
43-9
9.2321
9.2642
0.0787
4- 0.20
6.29
I I
I 128
4 48
18.6
17.1
20.9
17-5
18.52
44-2
9.0039
9.0367
0.3062
+ 0.77
6.86
I I
1159
4 5 °
17.7
14.8
16.7
16.2
16.35
44.8
8.8990
8.9331
0.4098
4- 1.02
7.11
14
1283
4 52
22.5
23.O
26.0
234
23.72
41.4
9.2090
9.2360
0.1069
4- 0.27
6.36
IO
H 49
4 54
24-3
22.3
23.8
21.7
23.02
45-6
9.1845
9.2205
IO
8l8
4 56
28.4
30-4
3 i -7
29.8
30.08
42.7
9.4001
9.4296
Mittel aus den Vergleichsternbeobachtungen: 9 - 3439 ; 9-3596; 9.3251. Zur Reduction benutzt: 9.3429.
Zone 424. 1891 Februar 7
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 12 und Nr. 14
. Luft: 1
—2.
IO°
818
4h 27m
34-9
3189
33?6
33 ?o
33-35
4480
9.4804
9 - 5 I 27
IO
1149
4 29
26.0
23.2
24.7
25-3
24.80
47-8
9.2454
9.2872
7
1150
4 32
20.7
17.9
19.0
18.6
19.05
48.6
9.0275
9-0715
0.3045
+ 0.76
6.85
7
1178
4 33
16.0
16.1
17.0
16.5
16.40
48.8
8.9015
8.9461
O.4299
+ 1.07
7.16
6
11 55
4 35
18.3
17.1
17.2
18.3
17.72
49-3
8.9668
9.0129
O.3631
+ 0.91
7.00
6
1160
4 36
21.3
20.3
19-3
21.6
20.62
50.0
9-0935
9 -I 4 I 7
O.2343
4-0.59
6.68
6
1172
4 38
24.1
21.7
23-5
234
23.18
50.0
9.1902
9.2384
O.1376
4- 0.34
6-43
5
1156
4 39
1 5 -1
13.2
14.0
134
13.92
50.9
8.7624
8.8135
O.5625
+ 1.41
7-50
10
818
4 4 i
31.0
29-5
32.3
31.6
31.10
43-3
9.4262
9 - 457 °
IO
1149
4 43
25.1
25.0
26.3
24.0
25.10
46.5
9-2551
9.2934
*) 2
1139
4 46
26.5
26.1
27-3
274
26.82
52.4
9.3087
9-3651
0.0109
+ 0.03
6.12
2
1144
4 47
20.3
17.0
19.8
17.7
18.70
52.0
9.0120
9.0669
0.3091
4-0.77
6.86
2
1171
4 49
15.0
13-9
13-7
i 3-7
14.08
52.8
8.7722
8.8300
0.5460
+ 1.37
7.46
1
1275
4 5 i
20.0
18.5
19-3
21.2
19-75
53-8
9.0576
9 -H 93
0.2567
4- 0.64
6-73
1
1278
4 52
18.0
16.5
18.0
18.1
17-65
53-9
8.9635
9.0256
0.3504
+ 0.88
6-97
4
1181
4 54
18.0
17.0
18.1
174
1 7.62
50.6
8.9620
9.0121
O.3639
4- 0.91
7.00
IO
818
4 56
30.0
30.0
32.3
29.0
30.32
42.7
9.4063
9-4358
IO
1149
4 59
25.2
23-9
23-7
25-1
24.48
45-2
9.2348
9 . 2 ÖQ 9
Mittel aus den
Vergleichsternbeobachtungen
■ 9.4000; 9.3752; 9.3528. Zur Reduction benutzt: 9.3760.
) 2 11 39 - Hellere Componente eines sehr weiten Doppelsterns.
