204
Müller und Kempf, Photometrische Durchmusterung
204
B.D.
Sternzeit
I
II
III
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone IQ7
1888 Februar 26.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 18 und Nr. 20. Luft:
3 -
IO°
1818
io*» 27™
2 2?0
2482
2384
2586
23?8o
4884
9.2118
9-2552
9
2239
10 30
19-5
19-5
22.7
19.1
20.20
44-5
9.0764
9.1098
IO
1837
10 33
33 -o
324
35 -i
32.1
33-15
48.9
9-4757
9.5206
0-3585
— 0.90
6.05
IO
1840
10 34
27.I
24.0
24.6
21.6
24.32
49.0
9.2295
9.2747
0.1126
— 0.28
6.67
19
2053
10 36
22.1
19.7
25.0
2 1.0
21.95
40.7
9-1453
9.1 710
0.0089
0.02
6-93
19
2069
10 38
2 1.3
22.4
22.4
2 1.8
21.98
40.5
9.1464
9 -I 7 I 7
O.OO96
0.02
6-93
11
1892
10 40
23-5
23.6
23-5
23-7
23-58
48.2
9.2042
9.2471
0.0850
— 0.2 I
6-74
11
1894
IO 41
16.8
13-5
17.4
15.0
15.68
48.1
8.8636
8.9062
0.2559
+ O.64
7-59
IO
1818
IO 42
24.4
22.3
25-5
26.9
24.78
50.0
9.2447
9.2929
9
2239
10 45
17-5
17-3
21.1
I9.I
18.75
45-3
9.0142
9.0495
i 5
1862
10 49
I4.O
11.7
12.6
12.5
12.70
45-9
8.6842
8.72 10
O.441 I
+ I.IO
8.05
i 3
1972
10 51
37-5
34 -o
36-9
33-6
35-50
47-5
9-5279
9.5688
O.4067
1.02
5-93
IO
1864
10 53
37-6
39-5
374
38.0
38.12
49.9
9.5810
9.6289
0.4668
— I.I7
5.78
19
2095
10 54
21.4
23-5
22.5
20.4
21.95
42.3
9-1453
9.1740
0.0119
— O.O3
6.92
12
1904
10 56
32.6
31.0
29-5
30.6
30.92
48.1
9.4217
9-4643
0.3022
O.76
6.19
15
1901
10 57
134
12.6
144
12.0
13.10
45-4
8.7107
8.7463
0.4158
+ 1.04
7-99
13
1994
10 59
23.0
21.4
24.9
23.0
23.08
47.8
9.1866
9.2284
0.0663
— 0.17
6.78
IO
1818
11 1
20.5
22.6
24.0
2 2.0
22.28
52.2
9 -I 576
9.2132
9
2239
ii 3
20.8
17.0
19.4
17.8
18.75
46.4
9.0142
9.0522
Mittel aus den
Vergleichsternbeobachtungen
: 9.1825; 9.1712; 9.1327. Zur Reduction benutzt: 9.1621
Zone 198
1888 Februar 27.
Beobachter: Müller.
Photometer :
D. Vergleichsterne: Nr. 8 und Nr.
10. Luft:
2.
9 °
.472
6 h 6 m
* O
CO
1580
I 5 ( -5
i4?6
1582 2
5284
8.8383
8.8947
11
632
6 8
20.3
19.7
23.6
18.6
20-55
45-7
9.0907
9.1270
13
661
6 IO
12.7
12.9
13-5
11.8
12.72
45-4
8.6855
8.72 11
O.2746
+ 0.69
7-94
13
665
6 12
26.6
25.6
26.3
2 - 5-5
26.OO
45-3
9.2837
9.3190
0.3233
— 0.81
6.44
11
592
6 13
134
12.6
144
11.4
12.95
47-3
8.7009
8.7413
O.2544
—f- 0.64
7.89
i6
579
6 14
18.6
16.5
18.1
16.4
17.40
43-3
8.9515
8.9823
0.0134
+ 0.03
7.28
18
624
6 l6
26.1
26.3
27.0
23-4
25.70
41-5
9-2743
9.3014
0.3057
— 0.76
6-49
18
629
6 17
19.2
17-5
19-5
16.1
18.08
41.8
8.9837
9.0114
O.OI57
— 0.04
7.21
9
472
6 19
16.0
14.2
16.6
13.6
15.10
54 -o
8.8316
8.8941
11
632
6 20
20.6
19.6
20.8
18.2
19.80
46.8
9-0597
9.0988
14
687
6 23
21.6
18.6
20.8
20.7
20.42
46.0
9.0854
9.1224
O.1267
-0.32
6-93
13
Ó67
6 24
13.6
13-7
13.8
12.4
I 3-38
46.8
8.7287
8.7678
0.2279
+ 0.57
7.82
i6
586
6 2Ó
33-0
32.8
32.2
32.0
32.50
43-9
9.4604
9.4925
0.4968
— 1.24
6.01
11
601
6 27
19-3
16.4
20.3
17.4
18.35
48.9
8.9961
9.0410
O.0453
0.1 I
7.14
11
604
6 28
23-5
21.3
21.2
20.2
21-55
48.2
9-1301
9.1730
O.I 773
— 0.44
6.81
12
584
6 30
134
11.6
12.7
11. 6
12.32
47-7
8.6583
8.6998
O.2959
4 - 0.74
7-99
9
472
6 32
16.2
13-7
15-5
14.0
14.85
55-6
8.8175
8.8868
11
632
6 34
20.4
174
20.0
18.6
19.IO
48.2
9.0297
9.0726
Mittel aus den Vergleichsternbeobachtungen: 9.0109; 8.9964; 8.9797. Zur Reduction benutzt: 8.9957.
Zone igg. 1888 Februar 27.
Beobachter: Kempf.
Photometer:
D. Vei
gleichsterne: Nr. 10 und Nr. 12. Luft:
2.
ii° 632
5h 37m
2 I?2
19?8
20?4
i9?6
20?2 5
4885
9.0785
9.1222
IO
818
6 39
34-5
384
31.6
36.0
35-12
44-5
9 - 5 I 97
9-5531
IO
688
6 42
21.5
18.5
20.9
20.2
20.28
46.9
9.0797
9.1190
O.2312
+ O.58
7-03
11
702
6 43
16.8
16.0
17.O
17.0
16.70
46.5
8.9169
8.9552
0.3950
+ O.99
7-44
11
7°4
6 45
17.1
15-5
17.4
15.2
16.30
45-9
8.8964
8.9332
0.4170
+ 1.04
7-49
14
825
6 47
18.4
19-3
19.O
19.1
18.95
43-5
9.0231
9-0543
O.2959
+ 0-74
7.19
13
803
6 48
18.5
15-5
I 7.2
16.0
16.80
44.1
8.9219
8.9544
0.3958
+ O.99
7-44
19
847
6 49
2 1 .4
20.9
22.0
23.0
21.82
39-2
9.1404
9.1634
O.1868
+ 0.47
6.92
11
632
6 51
23.8
19.4
2I.4
21.1
21.42
50.0
9-1251
9-1733
