280
Müller und Kempf, Photometrische Durchmusterung
280
B.D.
Stern zeit
1
11
III
IV
J
z
log sin 2 /
corrig.
für Ext.
. Diffi
in log.
Di ff. in
Grössen
Grösse
io°398i
20 h l8 m
2486
2 0?9
2 2?0
20?0
2 1 ?88
4286
9.1426
9 .I 7 I 9
7 3798
20 20
29.8
25-5
20.8
26.5
27-15
50.0
9.3186
9.3668
0.1663
— O.42
6.42
8 3797
20 22
20.0
16.5
l8.8
17-3
18.15
48.7
8.9869
9.0312
0.1693
-j- O.42
7.26
8 3799
20 23
18.2
14.1
16.4
I3.8
15.62
48.8
8.8603
8.9049
0.2956
+ 0-74
7-58
8 3819
20 24
19.1
16.2
14-5
15-2
16.25
48.8
8.8938
8.9384
0.2621
-f- 0.66
7-50
4 3838
20 26
17.8
15.2
17.0
16.O
16.50
53 -o
8.9067
8-9653
0.2352
+ 0.59
7-43
5 3941
20 28
35-7
34 -o
35 -i
33-1
34-48
52.0
9-5058
9.5607
0.3602
— 0.90
5-94
10 3573
20 30
26.0
22.0
21.8
22.7
23.12
48.1
9.1880
9.2306
10 3981
20 31
21.2
19.7
21.4
22.6
21.22
43-2
9-1173
9.1478
Mittel aus den Vergleichsternbeobachtungen : 9.2018; 9.2105; 9.1892. Zur Reduction benutzt: 9.2005.
Zone 388.
1890 September
r 7*
Beobachter: Müller.
Photometer :
D. Vergleichsterne: Nr. 36 und Nr. 38. Luft:
1.
9 ° 34 2 4
i8 h 5o’ n
3787
30? i
3383
3087
32895
4588
9-47 ii
9.5076
10 3573
18 52
24.7
19-5
22.1
20.6
2 1.72
41.8
9.1366
9.1643
5 349 °
18 55
18.7
14.8
16.5
14.9
16.22
49.0
8.8922
8.9374
0.4089
4- 1.02
7.40
9 3471
18 57
17.8
14.2
17.8
l6.2
16.50
45-2
8.9067
8.9418
0.4045
~b 1.01
7-39
9 3485
18 58
23.8
21.3
2O.4
2O.9
2 I.60
45 -o
9.1320
9.1666
0.1797
+ 0.45
6.83
3 3493
19 0
27.7
23.6
25.O
24-5
25.20
5 1 - 1
9.2584
9-3101
0.0362
+ 0.09
6-47
2 3406
19 2
24.0
21.6
25.I
21.7
23.IO
52.9
9 -i 873
9-2455
0.1008
+ 0.25
6.63
0 3786
19 4
14.6
ii -4
1 3-1
1 1-9
12-75
54 -i
8.6876
8.7505
0.5958
+ i -49
7.87
9 3424
19 6
34-4
30.8
32.3
33-6
32.78
47.0
9.4670
9.5066
10 3573
19 8
25.1
22.4
23.0
20.8
22.82
42.3
9-1773
9.2060
5 3521
19 10
22.1
17.4
20.8
19.0
19.82
50.2
9.0605
9.1093
0.2370
+ 0.59
6.97
4 3541
19 11
23.2
19.4
19.4
18.3
20.08
50.9
9 - 07 I 5
9.1226
0.2237
4~ 0.5 6
6-94
8 3511
19 13
17.8
17.0
18.4
16.1
I 7-32
47-3
8.9476
8.9880
0-3583
4- 0.90
7.28
i 3525
19 15
16.2
13.2
16.1
13.6
14.78
54-5
8.8134
8.8780
0.4683
4 -1.17
7-55
i 3526
19 16
23-7
19.7
22.1
19.7
21.30
54-5
g.1204
9.1850
0.1613
4- 0.40
6.78
7 3488
19 20
12.1
9-5
IO.9
9.0
IO.38
48.8
8.5113
8-5559
0.7904
+ 1.98
8.36
9 3424
19 22
36.5
31-5
32.8
3 I-I
32.98
48-5
9 - 47 I 7
9-5154
10 3573
19 24
23-5
20.1
22.6
2 I.9
22.02
43 -o
9.1479
9.1780
Mittel aus den Vergleichsternbeobachtungen: 9.3360; 9.3563; 9.3467.
Zur Reduction benutzt: 9.3463.
Zone 389.
i8go September
17 .
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 36 und Nr. 38. Luft: 1
—2.
io °3573
ig h 2 7 ra
2588
2 2?0
2480
2581
24822
4382
9.2261
9.2566
9 3424
19 31
35-9
29-5
29.9
30.0
31-32
49-3
9-4317
9.4778
14 3374
19 33
19.1
16.5
I 7.6
16.O
17.30
42.8
8.9466
8.9763
0.3865
4 - 0.97
7-35
14 3375
19 35
12.7
9.4
I 2.0
IO.5
ii. 15
42.9
8.5729
8.6028
0.7600
4 - 1-90
8.28
14 3378
19 36
19-3
I 7.O
I9.O
18.4
18.42
42.6
8.9993
9.0286
0.3342
4- 0.84
7.22
15 3327
19 37
28.9
26.4
27-5
26.4
27.30
42.3
9.3230
9 - 35 I 7
0.01 I I
4- 0.03
6.41
14 3387
19 39
15-5
14-5
154
14.5
14.98
43-4
8.8249
8-8559
0.5069
4- 1.27
7-65
14 3397
19 41
18.1
15.2
15-7
154
16.10
43-3
8.8859
8.9167
0.4461
+ 1.12
7-50
17 3401
19 43
18.4
17-5
17.9
16.4
17-55
41.1
8.9587
8.9851
0.3777
4 - o -94
7-32
9 3424
19 45
30.8
28.9
27-5
29.I
29.08
50.8
9-3733
9.4241
10 3573
19 48
29.0
234
25.1
25-5
25-75
44-5
9-2759
9.3093
ii 3315
19 51
21.0
1 7.O
18.4
18.O
18.60
47.1
9.0075
9.0474
0.3154
4- 0.79
7.17
19 3494
19 53
24.0
21.7
23-5
23.6
23.20
39-9
9.1909
9 - 2 I 5 I
0.1477
4- 0.37
6-75
19 35 o 8
19 55
28.0
25.6
24-5
234
25.38
39-8
9.2642
9.2883
0.0745
4- 0.19
6-57
19 3509
19 56
23.2
l 8.3
19.0
I9.O
19.88
39-9
9.0631
9.0873
0.2755
4- 0.69
7.07
16 3347
19 58
18.2
15.8
16.1
I3.6
15.92
42.7
8.8765
8.9060
0.4568
4 - 1.14
7-52
16 3356
19 59
22.0
20.0
21.0
21.5
21.12
42-5
9 -II 34
9.1425
0.2203
+ 0.55
6-93
9 3424
20 1
32.6
29-5
29.0
29.O
30.02
52.6
9.3984
9-4555
10 3573
20 4
25-5
23-5
23.8
23.O
23-95
45-7
9.2169
9-2532
Mittel aus den Vergleichsternbeobachtungen: 9.3672; 9.3667; 9.3544.
Zur Reduction benutzt: 9.3628.
