386
Müller und Kempf, Photometrische Durchmusterung
386
B.l).
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zusatz-Zone
21.
1893 Februar 3.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 10 und Nr. 12. Luft:
2.
11°
632
6 l 37 ”
17?6
1385
i 6?3
1582
15865
4885
8.8620
8.9057
IO
818
6
40
24.6
25.1
24-5
23-5
24.42
44.6
9.2328
9.2665
I 2
598
6
42
36.4
32-3
32.2
3 i -7
33-15
48.4
9-4757
9 - 5 1 9 1
0.4549
— 1.14
5 - 3 1
I
757
6
44
24-5
22.8
23-5
21.5
23.08
59 - 1
9.1866
9-2734
0.2092
— O.52
5-93
1 5
639
6
46
25.8
24.8
27.1
234
25.28
46.4
9.2610
9.2990
0.2348
— 0-59
5-86
i 3
690
6
48
28.9
254
26.1
28.0
27.10
48.2
9 - 3 i 7 i
9.3600
0.2958
-O.74
5 - 7 1
o
798
6
50
28.0
25-3
25.6
25.1
26.OO
59 -i
9.2837
9-3705
0.3063
— O.77
5.68
i 5
665
6
53
33-3
28.3
31.2
30.0
30.70
46.0
9.4161
9 - 453 1
0.3889
— O.97
5-48
11
632
6
56
1 5-7
12.2
15.6
144
14.48
50.5
8.7960
8.8458
io
818
6
58
27.0
24.1
25.8
23-3
25-05
45-9
9-2535
9.2903
7
681
7
1
27-3
24.4
26.3
254
25-85
53-9
9.2790
9 - 341 1
0.2769
— O.69
5-76
IO
621
7
3
28.5
27.8
26.4
27.0
27.42
50.6
9-3265
9.3766
0.3124
— 0.78
5-67
11
646
7
6
27.6
27.0
28.9
27.6
27.78
50.3
9-3369
9.3860
0.3218
— 0.80
5.65
18
743
7
7
31.8
31.0
30.7
32.3
31-45
43-6
94350
9.4664
0.4022
I.OI
5-44
2
800
7
9
29.1
25-7
25-9
26.9
26.90
58.0
9.3m
9 - 39 I 9
0.3277
— 0.82
5-63
7
755
7
11
29.1
25-5
28.2
28.1
27.72
53-4
9-3352
9-3953
0 - 33 11
— 0.83
5.62
11
632
7
13
14.0
13-3
15.6
13-9
14.20
52.6
8.7794
8.8365
IO
818
7
16
23-7
21.5
23-3
25-3
23-45
474
9.1997
9.2404
Mittel aus den
V ergleichsternbeobachtunge
n: 9.0861; 9.0680; 9.0384.
Zur Reduction benutzt: 9.0642
Zusatz-Zone
22.
1893 Februar 3.
Beobachter: Kempf. Photometer: D. Verg
ieichsterne: Nr. 12
und Nr. 14. Luft: 1
— 2.
i o°
1149
7 h
4 i m
2480
20?6
2485
2385
23815
4489
9.1891
9-2235
IO
818
7
43
33-6
26.5
30.6
27.1
29-45
50.1
9-3834
94319
16
672
7
46
37 -o
33 -o
34-6
3 i -5
34.02
49.2
9.4956
9 - 54 H
0.2038
— 0.51
5-58
8
866
7
49
37-4
30.6
36.7
33 -o
3442
55-5
9-5045
9-5734
0.2358
— 0.59
5-50
i 5
759
7
5 i
44.6
39-2
394
38.0
40.30
49.0
9.6215
9.6667
0.3291
0.82
5-27
17
920
7
53
46.0
40.6
44.0
38.0
42.15
46.4
9-6536
9.6916
0-3540
O.89
5.20
14
947
7
55
30.4
25-5
314
28.4
28.92
48.0
9.3689
9.4112
0.0736
O.18
5 - 9 i
13
979
7
57
35-3
3 i -7
38.5
31.0
34-12
46.9
9.4978
9-5371
0.1995
— 0.50
5-59
IO
818
8
0
29.4
25-3
28.5
26.5
27.42
52.0
9-3265
9.3814
IO
1 149
8
2
26.0
22.6
254
23-4
24-35
46.6
9-2305
9.2690
6
1027
8
5
39 -o
364
38.9
35-6
37-48
54-5
9-5685
9 - 633 I
0.2955
— O.74
5-35
14
1041
8
8
36.5
32.5
39 -°
34 -o
35-50
47.6
9-5279
9.5691
0.2315
— O.58
5 - 5 i
0
1239
8
10
35-7
32.8
37 -o
31.0
34-12
59-2
9.4978
9-5851
0.2475
0.62
5-47
19
1186
8
1 2
43-7
38.5
42.0
38.0
40.55
41.9
9.6260
9-6539
0.3163
— O.79
5-30
16
1060
8
15
33-4
32.0
38.5
33-0
34.22
43-9
9.5000
9-5321
0.1945
— O.49
5.60
14
1247
8
*9
37 -o
32.0
35-6
3 i -5
34.02
45 -i
9.4956
9-5304
0.1928
O.48
5 - 6 1
IO
818
8
21
3 i -5
27.0
304
! 27.O
28.98
54-6
9.3706
9-4356
IO
1149
8
23
1 26.0
22.5
26.9
23.2
24.65
48.5
9.2405
9.2842
Mittel aus den Vergleichsternbeobachtungen: 9.3277; 9.3252; 9.3599.
Zur Reduction benutzt: 9.3376.
Zusatz-Zone
23 -
1893 Februar 4.
Beobachter:
Kempf
Photometer
D. Vergleichsterne: Nr. 2 und Nr. 4. Luft: 2.
9 °
47
3 1
o m
26?5
2785
26?5
2483
2 6?20
5383
9.2899
9.3496
IO
168
3
2
18.5
17-5
18.2
16.8
17-75
46.6
8.9682
9.0067
17
55
3
5
53-6
49.9
57-6
46.8
51.98
474
9.7929
9.8336
0.7075
— I.77
4.92
19
79
3
7
37-5
39-5
39-9
35 -o
37-98
45 -o
9-5783
9.6129
0.4868
1.22
5-47
14
111
3
9
39-4
37-5
39-5
36.0
38.10
47.6
9.5806
9.6218
04957
— I.24
5-45
16
76
3
IO
40.0
36-9
43-7
39-5
40.02
46.2
9.6165
9.6540
0.5279
— 1-32
5-37
14
163
3
1 2
32.9
28.6
36.1
32.5
32.52
46.3
9.4609
9.4987
0.3726
— 0.93
5-76
19
185
3
14
30.0
28.2
34-9
35-6
32.18
41.0
9.4528
9.4790
0.3529
— 0.88
5.81
