304
Müller und Kempf, Photometrische Durchmusterung
304
B.D.
Sternzeit
I
II
III
IV
J
Z
log sin 2 J
corrig.
für Ext.
> Diff.
in log.
Diff. in
Grössen
Grösse
i o° 1818
9 h 1 9 m
2 4°5
20?5
23-5
2381
22890
4382
9.1802
9.2 107
4 1945
9 21 1
22.5
20.5
22.6
21.8
21.85
50.0
9-1415
9.1897
0.0260
-1- 0.07
6-75
9 1921
9 23
26.1
22.6
27.0
23.6
24.82
45-5
9.2460
9.2818
0.0661
— 0.1 7
6.51
1 2056
9 25
16.5
13.0
14.6
15.0
14.78
53 -i
8.8134
8.8724
0.3433
+ 0.86
7-54
6 1919
9 27
17.0
I4.7
16.4
16.1
16.05
48.3
8.8833
8.9264
0.2893
+ O.72
7.40
6 1923
9 29
19.6
I 7.6
20.8
18.4
19.10
48.4
9.0297
9 - 073 I
0.1426
+ O.36
7.04
6 1900
9 30
15.0
I2.4
14.0
12.3
1342
48.8
8-7313
8-7759
0.4398
+ I.IO
7.78
11 1588
9 33
23.8
22.0
23-5
23.1
23.10
49.0
9-1873
9-2325
10 1818
9 35
23.6
20.5
24.0
23-5
22.90
44.2
9.1802
9.2130
Mittel aus den Vergleichsternbeobaclitungen: 9.2x23; 9.2121; 9.2227. Zur Reduction benutzt: 9.2157.
*) 3° *933 dupl. Gemessen nur die belle, nördlich vorangehende Componente.
Zone 448. 1891 April 23.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 18 und Nr. 20. Luft: 1
—2.
10 0 1818
lO h 23 111
2 2?3
20?7
2384
2 2?I
CM
c •
CM
CM
4880
9-1516
9-1939
9 22 39
IO 25
18.O
16.9
I 8.2
I 7.O
17-52
44.2
8.9573
8.9901
4 2081
IO 27
27.7
25.0
26.4
27-5
26.65
5 i -7
9-3036
9-3574
0.2804
O.7O
6.25
3 2099
10 30
15-9
15-3
16.4
I 7.2
16.20
53-5
8.8912
8-9517
0.1253
+ 0.31
7.26
3 2124
IO 31
17-3
15-2
17.7
I 7.6
16.95
53 -i
8.9294
8.9884
0.0886
+ 0.22
7.17
2 21 12
10 33
20.0
19.1
22.3
I9.7
20.28
54-5
9.0797
9 -H 43
0.0673
— 0.17
6.78
I 2210
10 35
12.6
1 1-3
13-7
I 1.6
12.30
55-7
8.6569
8.7267
0.3503
+ 0.88
7-83
O 2449
10 37
31.0
30.8
33 -i
32.5
31-85
56.5
9.4448
9.5182
0.441 2
— I.IO
5-85
10 1818
10 39
20.7
20.0
21.8
2 1.8
21.08
49-7
9.1118
9 -i 59 i
9 2239
10 41
17.2
16.4
18.6
18.2
17.60
45 -o
8.9611
8-9957
9 2093
10 43
26.4
24.6
25.6
25-3
25.48
48.2
9.2674
9-3103
0.2333
— 0.58
6-37
9 2099
10 45
i 3 -1
11.8
13-1
12.4
12.60
48.6
8-6775
8.7215
0.3555
+ 0.89
7.84
7 2066
10 47
29.0
29.7
31.0
31.0
30.18
50.0
9.4027
9.4509
0.3739
— 0.93
6.02
7 2068
10 48
22.0
18.5
21.6
20.1
20.55
50-4
9.0907
9.1402
0.0632
— 0.16
6.79
6 2087
10 50
24.6
234
254
26.8
25-05
5 i -9
9-2535
9.3080
0.2310
— 0.58
6-37
2 2138
IO 52
13-5
12.1
134
14-3
13-32
54-8
8.7249
8.7907
0.2863
+ 0.72
7.67
10 1818
10 53
21.1
20.0
22.6
20.8
21.12
51.2
9 -i 134
9 -i 655
9 2239
10 55
17-3
15-5
174
16.9
16.78
45-8
8.9209
8-9574
Mittel aus den Vergleichsternbeobaclitungen: 9.0920; 9.0774; 9.0615. Zur Reduction benutzt: 9.0770.
Zone 44g. .1891 April 24.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 18 und Nr. 20. Luft:
2.
10 0 18 18
IO 1 ’ 28’”
2 2?6
1987
20?6
2 0?0
20872
48?5
9-0975
9.1412
9 2239
10 30
I9.4
16.6
17.6
I 6.2
17-45
44.4
8-9539
8.9871
2 2145
IO 33
26.5
25-5
26.2
25.O
25.80
53-9
9.2774
9-3395
0.2576
— 0.64
6.31
O 2477
10 35
20-7
i 9-5
19.0
l8.6
19-45
54-9
9.0449
9.1112
0.0293
— 0.07
6.88
1 2267
10 37
I9.6
18.0
ig.O
19.6
19.05
54-2
9.0275
9.0908
0.0089
— 0.02
6-93
1 2271
10 38
I 7.6
15.0
16.4
15-5
16.12
54-4
8.8870
8.9511
0.1308
+ 0.33
7.28
2 2173
10 39
I9.O
16.8
18.2
18.0
18.00
53 -i
8.9800
9.0390
0.0429
+ 0.1 I
7.06
2 2l68
10 40
13-9
1 2.0
12.6
12.3
12.70
53-3
8.6842
8-7439
0.3380
+ 0.85
7.80
10 1818
10 42
23-4
18.6
22.0
20.5
2 I . I 2
50.0
9 -i 134
9.1616
9 2239
10 44
20.1
15.6
l8.8
17.0
17.88
45 -i
8.9744
9.0092
9 2133
10 46
20.0
17-5
194
17.9
18.70
47-5
9.0120
9.0529
0.0290
+ 0.07
7.02
8 2172
10 47
18.7
154
l 8.3
16.0
17.IO
49.2
8.9368
8.9826
0.0993
+ 0.25
7.20
3 2144
10 49
19.6
17-5
19.2
18.5
18.70
54 -i
9.0120
9.0749
0.0070
+ 0.02
6-97
4 2139
10 55
27.7
24.0
25.O
23.0
24.92
53 -o
9.2493
9-3079
0.2260
— 0-57
6.38
6 2120
10 56
23-9
21.2
23-5
24.4
23-25
5 i -7
9.1927
9.2465
0.1646
— O.41
6-54
8 2199
10 58
19.0
15.0
18.6
15-5
I 7.O2
49.0
8.9329
8.9781
0.1038
+ 0.26
7.21
10 1818
11 0
24.0
194
21.6
20.0
21.25
52.0
9.1185
9-1734
9 2239
11 2
22.0
16.6
18.0
15-5
l8.02
46.3
8.9809
9.0187
Mittel aus den Vergleichsternbeobachtungen: 9.0642; 9.0854; 9.0960. Zur Reduction benutzt: 9.0819
