388
Müller und Kempf, Photometrische Durchmusterung
388
B.D.
Steriizeit
I
II
III
IV
J
z
log sin 2 ./
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zusatz-
Zone
26.
1893 Februar 4.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18
Luft: 1-
—2.
O
11°
1588
6 h 1 6 m
l8?2
1 /84
i 7 °i
i6?7
17835
4382
8.9491 '
8.9796
IO
1818
6 18
17.7
17.8
18.0
16.6
I 7-52
49.4
8.9573
9.0037
7
1607
6 21
28.1
27.0
26.4
26.0
26.88
45-6
9-3105
9-3465
0.3637
— O.91
5-77
16
1397
6 22
30.2
32.2
30.1
29.2
30.42
37 -i
9.4089
9.4286
0.4458
— 1.11
5-57
11
1578
6 24
29-3
28.6
3°-4
30.1
29.60
42.0
9-3874
9-4155
O.4327
— 1.08
5.60
2
1691
6 26
33-7
34-5
33-4
29.7
32.82
51-9
9.4680
9-5225
0-5397
— 1-35
5-33
IÓ
1510
6 28
32.1
29.4
29.8
30.9
30-55
38.1
9.4122
9-4335
0.4507
—1.13
5-55
2
1808
6 30
32-5
32-9
31.0
29.6
3 1 * 5 °
52.8
9.4362
9.4940
O.5112
— 1.28
5-40
I I
1588
6 33
18.4
18.0
18.7
16.4
17.88
42.3
8.9744
9.0031
IO
1818
6 35
18.4
15-9
16.6
15-7
16.65
47.6
8.9144
8.9556
i 7
1731
6 37
30-7
29.0
28.8
28.4
29.22
38.0
9-3771
9.3982
O.4154
— 1.04
5.64
13
1831
6 39
34-6
32-5
34 -o
33-4
33 -Ó 2
42.1
9.4865
9.5148
0.5320
— 1-33
5-35
8
2053
6 42
34-5
35-3
35-4
32.4
34-40
48.8
9.5040
9.5486
0.5658
—1.41
5-27
13
1912
6 44
31-7
29.4
31-1
29.2
30.35
43-9
9.4071
9.4392
O.4564
—1.14
5-54
12
1941
6 47
31.0
32.0
32.6
31.8
31-85
47-3
9.4448
9.4852
O.5024
— 1.26
542
15
1945
6 48
33 -o
33 -o
33-3
31.6
32.72
44.0
9-4657
9.4980
0.5152
— 1.29
5-39
11
1588
6 51
18.7
15-7
18.7
17-3
1 7.60
41.6
8.9611
8.9884
IO
1818
6 54
19.1
16.0
17.0
15-7
16.95
45-9
8.9294
8.9662
Mittel aus den Vergleichsternbeobachtungen
: 8.9917; 8.9793; 8.9773.
Zur Reduction benutzt: 8.9828.
Zusatz-Zone 27.
1893 März
23 *
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 24
und Nr. 26. Luft:
3 -
11°
2372
gh 33 m
20?3
1980
19-5
1984
19855
4780
9.0492
9.0888
11
2440
9 36
27-3
25.2
27.4
23.2
25.78
51-5
9.2768
9.3299
6 2384
9 39
40.0
41.2
41.7
38.4
40.32
48.3
9.6219
9.6650
0-4575
—1.14
5-33
0
2761
9 43
32.3
304
31.0
28.7
30.60
54-8
94135
9-4793
O.27 18
— 0.68
5-79
14 2367
9 45
32.1
31-5
33-2
31-5
32.08
42.1
9-4503
9.4786
O.271 1
— 0.68
5-79
2
2409
9 48
32.2
35-4
31.6
31.8
32.75
52.8
9.4664
9.5242
O.3167
— 0.79
5.68
3
2504
9 52
36.O
35-7
34-2
32.0
3448
52.3
9-5058
9.5618
0.3543
— 0.89
5.58
19
2459
9 56
34-6
32.6
34-5
30.0
32.92
37-6
9.4704
9.4909
0.2834
— 0.71
5.76
11
2372
9 59
20.6
17.6
18.8
18.3
18.82
44-7
9 -OI 73
9.0512
11
2440
10 2
26.8
25-5
26.4
24.6
25.82
48.6
9.2780
9.3220
17
2374
10 5
28.3
26.6
30.1
26.1
27.78
38.7
9-3369
9-3591
O.15 16
— 0.38
6.09
4
2556
10 17
31-3
30.5
33 -o
31-7
31.62
52.2
9-4391
9.4947
0.2872
— 0.72
5-75
15
2436
IO 20
40.3
40.7
39-4
39-7
40.02
42.9
9.6165
9.6464
0.4389
I.IO
5-37
17
2504
IO 22
33-7
31.6
33 -o
33-4
32.92
43 -o
9.4704
9-5005
0.2930
— 0.73
5-74
17
2533
10 25
43 -o
38.6
41.7
44.0
41.82
44.1
9.6479
9.6804
O.4729
— 1.1S
5-29
14
2549
10 28
33-7
29.7
30-4
28.8
30.65
46.4
• 9.4148
9.4528
0.2453
— 0.61
5-86
11
2372
10 30
19.9
18.4
19.7
20.9
19.72
42.5
9.0563
9.0854
11
2440
10 33
28.0
27-3
27-5
27-5
2 7-58
45-7
9*3311
9.3674
Mittel aus den Vergleichsternbeobachtungen: 9.2094; 9.1866; 9.2264. Zur Reduction benutzt: 9.2075
Zusatz-Zone 28.
1893 März
24.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 20 und Nr.
22. Luft:
2.
9 (
'2239
7 h 24 m
20?6
! 20?6
2 2?4
20?5
2 I ?0 2
r 1 0-
5 1 - 5
9.1095
9.1626
9
2374
7 30
35-4
33-2
32.9
33-5
33-75
56.3
9.4895
9.5620
5
2116
7 32
53-5
50.0
48.8
50.0
50-58
50.2
9-7758
9.8246
0.5035
— 1.26
5-30
15
2009
7 36
44.8
43-6
43-6
43 -i
43-78
41-3
9.6801
9.7069
0.3858
— 0.96
5.60
9
2188
7 39
41-5
39 - 6
42-5
40.0
40.90
47.8
9.6321
9-6739
0.3528
— 0.88
5-68
7
2160
7 42
51-8
47-3
46.5
47.1
48.18
50.4
9.7446
9.7941
0.4730
— 1.18
5.38
7
2181
7 45
36.7
37-4
34-5
34-5
35-78
51.0
9.5338
9-5852
0.2641
— 0.66
5-90
2
2246
7 48
35-4
34-4
; 35-5
34 -o
34.82
55-3
9 - 5 I 32
9.5812
0.2601
— 0.65
5-91
