358
Müller und Kempf, Photometrische Durchmusterung
358
B.D.
Sternzeit
I
II
III
IV
J
z
logsin 2 /
corrig.
für Ext.
Riff,
in log.
Diff. in
Grössen
Grösse
ig°2966
13 1 ’ 2 i m
2585
2380
2387
2285
23868
4080
9.2076
9.2320
0.1551
— 0.39
6.41
19 2972
13 23
15.8
13-7
l6.I
12.8
14.60
41.1
8.8030
8.8294
0.2475
+ 0.6 2
7.42
16 2789
13 24
19.8
21.4
22.7
194
20.82
42.7
9 *ioi 5
9.131°
0.0541
0.14
6.66
16 2790
13 26
14-3
1 3-7
16.9
14-3
14.80
42.8
8.8146
8.8443
0.2326
-4- 0.58
7-38
11 2780
13 28
21.5
20.0
2 2.0
194
20.72
45-9
9-0975
9*1343
9 3 2 °3
13 30
16.6
19.0
18.7
174
17.92
55 -o
8.9762
9.0429
10 2853
13 32
18.3
154
l6.2
16.0
16.48
47-4
8.9057
8.9464
0.1305
4 - 0.33
7-13
11 2800
13 34
13-7
11.7
I 2.4
11.7
12.38
46.6
8.6624
8.7009
0.3760
+ 0.94
7-74
11 2801
13 36
14.9
12.7
I4.4
13.0
13-75
46.0
8.7520
8.7890
0.2879
4- 0.72
7-5 2
12 2838
13 37
16.1
14.9
15.6
14.6
I 5-30
45-4
8.8428
8.8784
0.1985
+ 0.50
7-30
13 2953
13 39
17-3
13-5
15.8
15-7
I 5-58
44.2
8.8581
8.8909
0.1860
+ 0.47
7.27
13 2946
13 41
12.1
10.2
13-9
11*3
11.88
43-5
8.6272
8.6584
0.4185
4 - 1.05
7.85
11 2780
13 43
21.3
21.4
22.0
20.1
21.20
44-7
9-1165
9.1504
9 3203
13 45
17.6
17.2
I 9.8
17-3
17.98
53-2
8.9791
9.0385
Mittel aus den Vergleichsternbeobachtungen
: 9.0476; 9.0886; 9.0944.
Zu,r Reduction benutzt: 9.0769.
Zone 584. 1892 Mai 3.
Beobachter: Kempf.
Photometer :
Cu. Vergleichsterne: Nr. 27 und Nr. 33. Luft
3-
11° 2485
14 11 4 m
n ?5
1185
io?4
1185
I I?2 2
4582
8.5782
8.6133
7 3023
14 9
12.5
12.8
13-5
134
I 3-05
48.5
8.7075
8.7512
4 2669
14 12
22.1
23-5
20.5
22.5
22.15
51-3
9.1528
9.2052
0.5109
— 1.28
3-58
*) 4 2669
14 14
11-7
ii -4
11-4
11-5
11.50
51-4
8-5993
8.6521
0.0422
4- 0.11
3.62
11 2529
14 15
28.0
29-5
29.6
28.4
28.88
43-8
9-3679
9.3998
0.7055
— 1.76
3.10
O 3076
14 17
23-5
21.0
21.9
22.1
22.12
53-4
9 -i 5 i 6
9*2117
0.5174
— 1.29
3-57
19 2725
14 19
31-5
32.6
29.0
30.9
31.00
34 -o
9.4237
9-4393
0.7450
— 1.86
3.00
11 2485
14 22
n.7
1 1-4
10.4
11-5
II.25
46.8
8.5805
8.6196
7 3023
14 23
12.5
134
13.0
13.0
12.98
47-5
8.7029
8.7438
17 2768
.14 26
13.0
13.i
14-3
14.4
13.7O
35-5
8.7489
8.7664
0.0721
— 0.18
4.68
14 2770
14 28
17-5
18.0
18.6
19.1
18.3O
38.2
8.9938
9.0152
0.3209
— 0.80
4.06
11 2821
14 30
18.3
17-5
18.0
17.9
17.92
43-2
8.9762
9.0067
0.3124
— 0.78
4.08
6 3088
14 33
32.5
32.8
30.0
32.7
32.00
47.6
9.4484
9.4896
0.7953
— i -99
2.87
*)6 3088
14 35
15-4
154
154
15-9
I 5-52
47-4
8.8549
8.8956
0.2013
— 0.50
3.01
**)6 3088
14 38
30.6
30.0
294
28.7
29.65
47-3
9.3887
9.4291
0.7348
— 1.84
2.60
7 3023
14 41
13-4
14.6
13.0
14.0
13-75
46.3
8.7520
8.7898
11 2485
14 43
10.6
12.5
11.6
11 .5
ii -55
48.9
8.6030
8.6479
Mittel aus den Vergleichsternbeobachtungen: 8.6823; 8.6817; 8.7188. Zur Reduction benutzt: 8.6943.
*) Mit Blende 4 beobachtet.
**) Mit Blende 3 beobachtet.
Zone 585.
1892 Mai 5.
Beobachter:
Müller.
Photometer:
D. Vergleichsterne: Nr. 32
und Nr. 34. Luft:
3*
O
CO
CM
O
13 11 i6 m
O
O •
<N
CM
1986
2 2?3
1985
20885
4780
9.1027
9.1423
9 3203
13 19
18.4
17.7
194
17.4
18.20
56.4
8.9892
9.062 1
16 2797
13 22
24.1
23-3
2 6.6
22.3
24.08
43 - 6
9.2213
9.2527
0.1448
— 0.36
6-44
16 2799
13 24
21.3
19.O
2 1.6
18.7
20.15
43-5
9.0744
9.1056
0.0023
4- 0.01
6.81
17 2880
13 25
21.6
18.9
22.1
19.7
20.58
42.5
9.0919
9.12 10
0.0131
— 0.03
6-77
18 3044
13 27
27.4
244
27-3
23.6
25.68
42.1
9-2737
9.3020
0.1941
— 0.49
6.31
16 2807
13 29
26.3
25.6
27.8
25-7
26.35
43-3
9-2945
9-3252
0.2173
— 0.54
6.26
15 2890
J 3 33
18.7
18.9
I9.6
18.5
18.92
43-8
9.0218
9-0536
0.0543
4-0.14
6-94
11 2780
13 35
20.8
20.6
23.O
21.3
2 1.42
45-3 ■
9-1251
9.1604
9 3203
13 37
17.4
174
2O.4
18.9
18.52
54 -i
9.0039
'9.0668
Mittel aus
den Vergleichsternbeobachtungen: 9
1022; 9.1136. Zur Reduction benutzt:
9.1079.
Wegen Wolkenbildung
musste
die Zone abgebrochen werden.
