390
Müller und Kempf, Photometrische Durchmusterung
390
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
; in log.
Diff. in
Grössen
Grösse
Zusatz-Zone 31.
1893 März
27.
Beobachter: Müller.
Photometer:
13. Vergleichsterne: Nr. 20
und Nr. 22. Luft:
2.
9° 22 39
7 h 2Ö ra
1 7?4
i6?i
i 8?5
16?3
1 7?o8
5183
8.9358
8.9882
9 2 374
7 2 «
3 i -5
2 8.8
30.3
28.7
29.82
56.5
9-3932
9.4666
5 2116
7 3 i
50.3
45-7
48.9
45-7
47-65
50.3
9-7373
9.7864
0.6050
— 1 - 5 1
5-05
15 2009
7 3 2
40.2
40.3
38.7
36.6
38.95
41.6
9.5968
9.6241
0.4427
— i.l 1
5-45
9 2188
7 35
35-6
37-5
35-3
34-7
35-78
48.1
9-5338
9-5764
o- 395 o
— O.99
5-57
7 2160
7 37
4 i -5
40.2
42.8
43-6
42.02
50.8
9-6513
9.702 1
0.5207
— 1.30
5.26
7 2181
7 39
28.5
27.0
29.2
29.4
28.52
5 i -5
9-3579
9.41 IO
0.2296
— 0.57
5-99
2 2246
7 4 1
30.6
27.0
29.6
28.7
28.98
55-9
9.3706
9-4413
0.2599
— O.65
5 - 9 1
9 22 39
7 4 2
1 7-3
14.8
15-7
1 5 -i
15-72
49-7
8.8658
8.9131
9 2 374
7 44
29.6
25.8
2 7-5
28.2
27.78
54-6
9-3369
9.4019
13 2183
7 47
34-4
35-6
35 - 1
35-3
35 -io
46.7
9 - 5 I 93
9-5581
0.3767
— 0.94
5.62
14 2228
7 49
37 -o
34-7
35-8
32.0
34-88
47-4
9 - 5 I 46
9-5553
o -3739
— 0.93
5-63
0 2663
7 5 i
34 - 2
30-9
35 -o
32.3
33 -io
61.6
9-4745
9.5766
0 - 395 2
— 0.99
5-57
19 2371
7 53
34-7
33 -o
33-6
30.3
32.90
46.2
9.4699
9-5074
0.3260
— 0.82
5-74
14 2294
7 55
30.6
29.7
32.3
29-5
30.52
49-9
9 - 4 ii 4
9-4593
0.2779
— O.69
5.87
11 2283
7 57
34-4
314
34 -o
33-2
33-25
53-2
9.4781
9-5375
0.3561
— 0.89
5-67
9 2 374
7 59
30.0
26.9
28.7
27.8
28.35
52.8
9-3531
9.4109
9 2239
8 1
16.8
144
16.4
15-3
I 5-72
47-9
8.8658
8.9078
Mittel aus den Vergleichsternbeobachtungen: 9.2274; 9.1575; 9.1594.
Zur Reduction benutzt: 9.1814.
Zusatz-Zone 32.
1893 März 27.
Beobachter: Kempf. Photometer: Ci. Vergleichsterne: Nr. 17 und Nr. 19. Luft: 2
— 3 -
11°1670
8 h 14" 1
20?5
1987
2 2?4
22?2
2 I?20
4 1 89
9 - 1 165
9 -H 44
11 1984
8 16
21.7
21.6
23.6
24-5
22.85
42.3
9 - 1 784
9.2071
10 1746
8 18
14.6
13.6
14.4
14-5
I4.28
42.3
8.7842
8.8129
0.4022
+ 1.01
6.52
16 1662
8 20
14.8
16.4
4-5
1 5-5
I 5-30
35-6
8.8428
8.8605
0.3546
+ 0.89
6.40
18 1882
8 21
12.5
124
1 2-5
13.0
I 2 .ÖO
34-5
8.6775
8.6937
0.5214
+ 1-30
6.81
13 1868
8 23
14.0
13-5
13.2
i 3-9
I 3-65
39 -i
8.7458
8.7687
0.4464
+ 1.12
6.63
9 1921
8 25
14-5
14.5
14.7
13.6
14-32
43-3
8.7866
8.8173
0.3978
+ 0.99
6.50
4 1954
8 27
13-5
15.0
14-5
154
I4.60
48.2
8.8030
8.8459
0.3692
+ 0-92
6-43
11 1670
8 29
21.6
20.0
20.1
20.8
20.62
42-5
9-0935
9.1226
11 1984
8 31
24.6
22.4
25-9
26.4
24.82
41.8
9.2460
9-2737
18 1930
8 33
16.5
16.4
16.5
16.5
16.48
33-8
8.9057
8.9211
0.2940
4- 0.74
6.25
11 1830
8 37
i 5-5
16.0
13.0
1 5-5
15.00
41.6
8.8260
8.8533
0.3618
+ 0.90
6.41
17 1842
8 39
1 5-5
1 5-5
154
15-7
I 5-52
35-2
8.8549
8.8721
0.3430
+ 0.86
6-37
2 I 9 6 5
8 41
18.6
17.4
16.4
16.9
I 7-32
50.1
8.9476
8.9961
0.2190
+ 0.55
6.06
14 1899
8 43
16.4
16.1
i 5-5
15-2
15.80
38.0
8.8700
8.8911
0.3240
+ 0.81
6.32
5 1999
8 46
12.4
* 3-5
11.6
12.4
I 2.48
46.6
8.6693
8.7078
0-5073
+ 1-27
6.78
11 1670
8 48
2 3.5
244
24.6
24.7
24.30
43-5
9.2288
9.2600
11 1984
8 50
25-4
24-5
25.6
25.0
25.12
41.4
9-2558
9.2828
Mittel aus den Vergleichsternbeobachtungen: 9.1758; 9.1981; 9.27x4. Zur Reduction benutzt: 9.2151.
Zusatz-Zone 33.
1893 №ärz 29.
Beobachter: Kempf. Photometer: Ci. Vergleichsterne: Nr. 19
und Nr. 21
. Luft: 1
—2.
11°1984
8 h o m
21?7
21?6
2 I?2
22? 4
2 I ?7 2
4381
9.1366
9.1669
IO 2 II2
8 3
36.0
324
36.O
34-5
34 - 7 2
48.2
9 - 5 11
9-5540
17 2078
8 8
12.4
134
11-5
12.9
12-55
38.1
8.6741
8.6954
0.6982
+ i -75
6.77
8 2226
8 10
1 5 <I
16.6
15.8
15-9
15-85
46.2
8.8727
8.9102
0.4834
4- 1.21
6.23
2 2217
8 12
12.1
12.5
12.4
i 3-5
I 2.62
52.4
8.6788
8.7351
0.6585
+ 1.65
6.67
17 2109
8 15
17.6
16.4
17.6
17-5
I 7.28
38.5
8.9456
8.9675
O.4261
+ 1.07
6.09
12 2090
8 .9
16.5
19.0
174
18.7
I7.9O
43-3
8-9753
9.0060
0.3876
-+0.97
5-99
3 2280
8 21
12.4
14.6
12.5
i3-i
13-15
52.5
8.7140
8.7707
O.6229
+ 1-56
6.58
