364
Müller und Kempf, Photometrische Durchmusterung
364
13 .D.
Sternzeit
I
II
III
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
8°3582
I 7 k 22 m
338 o
3 2?2
2987
3181
310O
4484
9.4362
9.4694
2 3337
17 25
19.5
ig.O
18.0
18.8
18.82
49.6
9 -oi 73
9.0643
0.3633
+ 0.91
5-84
19 3354
17 28
20.4
18.5
18.5
19.0
19.10
33-1
9.0297
9.0442
0.3834
-f- 0.96
5-89
16 3218
17 30
20.5
20.0
18.1
19-3
19.48
36.0
9.0461
9.0643
0.3633
-b 0.91
5-84
16 3256
17 33
21.5
20.0
20.4
19.6
20.38
36.4
9.0838
9.1026
0.3250
4- 0.81
5-74
17 3334
17 34
20.5
19.9
18.0
19-5
19.48
34-6
9.0461
9.0625
0.3651
4- 0.91
5-84
6 3566
17 37
17-5
17-5
17.1
18.2
I 7-58
46.3
8.9601
8.9979
0.4297
4- 1.07
6.00
n 3156
17 38
28.0
28.4
27.6
30.1
28.52
41.7
9-3579
9-3854
8 3582
17 42
33 -i
32.0
33 -o
31.2
32.32
43-9
9.4562
9.4883
Mittel aus den Vergleichsternbeobachtungen: 9.4164; 9.4297; 9.4368.
Zur Reduction benutzt: 9.4276.
Zone 59g. 1892 August 23
#
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 42
und Nr. 44. Luft:
3 -
1°° 43 5 1
19“ O m
28? 9
2 7?6
2685
2587
27818
4587
9 - 3 I 94
9-3557
10 4604
19 5
30.0
26.6
29.6
26.0
28.05
52.0
9.3446
9-3995
17 4370
19 8
33-3
32.4
324
30.2
32.08
38.3
9-4503
9.4719
0.1223
— 0.31
6.17
15 4220
19 IO
32.1
30.8
29.8
29.2
30.48
40.5
9.4104
9-4357
0.0861
— 0.22
6.26
15 4227
19 12
2 1.6
2 I .O
24.O
20.4
21-75
40.6
9-1377
9.1632
0.1864
+ 0.47
6-95
14 4389
19 i 4
14-3
12.0
16.6
13-5
14.10
41.6
8-7734
8.8007
0.5489
4 - i -37
7-85
19 4484
19 16
26.0
26.3
24-5
24-3
25.28
36.4
9.2610
9.2798
0.0698
+ 0.17
6.65
17 4378
19 18
19.9
19-3
2 1.6
19-3
20.02
38.4
9.0689
9.0906
0.2590
4- 0.65
7 -i 3
10 4351
19 21
25.0
24.6
26.7
24.7
25-25
44.1
9.2600
9.2925
10 4604
19 23
28.6
28.3
2 6.8
28.1
27-95
50.0
9 - 34 i 8
9.3900
15 4201
19 29
13-4
13.0
16.5
15-5
14.60
38.8
8.8030
8.8254
0.5242
4 - 1.31
7-79
12 4383
19 3 i
15-7
15.6
16.7
134
15-35
41.0
8.8456
8.8718
0.4778
4 - 1-19
7.67
l6 4315
19 33
24.4
24-3
22.7
2 1.4
23.20
37-8
9.1909
9.2117
0.1379
4-0.34
6.82
12 4405
19 35
13.2
1 2.6
13-5
11.6
12.72
41.4
8.6855
8.7125
0.6371
4 - i -59
8.07
12 4419
19 37
20.1
16.7
18.5
17.7
18.25
41.0
8.9915
9.0177
0.3319
4- 0.83
7 - 3 i
10 4351
19 39
254
24.4
24.2
25-3
24.82
43 -o
9.2460
9.2761
10 4604
19 4 i
2 8.8
27.7
28.7
26.5
27.92
48.2
9.3410
9-3839
Mittel aus den Vergleichsternbeobachtungen: 9.3776; 9.3413; 9.3300. Zur Reduction benutzt: 9.3496.
Zone 600. 1892 August 23
.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 44 und Nr. 46. Luft:
3 -
io°46o4
I 9 ll 49 tn
2780
2480
2686
2588
25885
4783
9.2790
9 - 3 I 94
9 5 111
19 57
21.3
16.4
2 1.4
19-3
19.60
54-2
9-0513
9.1146
9 4984
20 1
14.6
11.6
16.6
11.6
13.60
49.2
8.7427
8.7885
0.4247
4- 1.06
7.60
8 4792
20 4
14-3
11.7
16.O
13-9
13.98
49-5
8.7662
8.8129
0.4003
4- 1.00
7-54
7 4829
20 6
16.3
16.1
17.8
16.6
16.70
5 i -5
8.9169
8.9700
0.2432
4- 0.61
7 -i 5
7 4834
20 8
21.4
20.4
21.4
21.4
21.15
51.0
9.1146
9.1660
0.0472
4- 0.12
6.66
5 4998
20 11
33-3
314
29.6
32.3
3I-65
53-6
9.4398
9.5007
0.2875
— 0.72
5.82
3 4689
20 15
14.7
12.3
13.6
11.7
13.08
54-2
8.7094
8.7727
0.4405
4- 1.10
7.64
10 4604
20 18
27.6
24.2
25.O
22.0
24.70
44-9
9.2421
9.2765
9 5 111
20 20
20.2
19.7
19.8
19-5
1 9.80
5 i -5
9-0597
9.1128
4 4804
20 24
15.6
12.8
13-7
11.6
13.42
5 i -7
8-7313
8.7851
0.4281
4- 1.07
7.61
2 4474
20 30
19.8
16.6
18.7
17.9
18.25
53-9
8.9915
9-0536
0.1596
+ 0.40
6.94
2 4476
20 32
15.0
12.6
16.5
13-9
14.50
53-9
8.7972
8-8593
0.3539
4- 0.88
7.42
3 4672
20 35
11-3
11.6
13.8
12.4
I 2.28
52.3
8.6555
8.7115
0.5017
4 - 1.25
7-79
3 4687
20 37
18.6
17.8
19.7
14.8
17.72
52-3
8.9668
9.0228
0.1904
4- 0.48
7.02
1 4584
20 39
20.1
18.8
18.9
19.4
19.30
53-3
9.0384
9.0981
0.1151
4 - 0.29
6.83
10 4604
20 44
28.7
29.4
27.0
24.9
27.50
43-3
9.3288
9-3595
9 5 111
20 46
l8.8
19.9
20.4
19.4
19.62
48.7
9.0521
9.0964
Mittel aus den Vergleichsternbeobachtungen: 9.2170; 9.1947; 9.2279. Zur Reduction benutzt: 9.2132.
