296
Müller und Kempf, Photometrische Durchmusterung
296
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
i 5 °
1197
4 h 42™
I 6?2
1580
1 6? I
• O
C\1
! O *
"2
4 i?6
8.8870
8.9143
0.2098
-b 0.52
6-99
i6
1159
4 44
22.0
20.0
2 I.9
21.1
21.25
40.9
9.1185
9-1445
0.0204
— 0.05
6.42
17
I2 77
4 46
14.O
I 1.2
I3.6
12.6
12.85
40.0
8.6943
8.7187
0.4054
+ I.OI
7.48
17
1275
4 48
22.9
2I.9
24.6
22-5
22.98
40.2
9.1831
9.2079
0.0838
0.2 I
6.26
l l
1260
4 51
I2.9
10.0
II4
II.9
11-55
39-0
8.6030
8.6257
0.4984
4 -1.25
7.72
17
1268
4 52
I2.5
I 1.2
I 1.6
11 -5
11.70
38.8
8.6141
8.6365
0.4876
4 - 1.22
7.69
IO
1149
4 54
23-9
2 1.0
22.4
24.4
22.92
45-6
9.1809
9.2169
11
1588
4 57
2O.5
I7.O
18.9
17.i
18.38
50.3
8.9975
9.0466
Mittel aus den
Vergleichsternbeobachtungen: 9.1238; 9.1168; 9.1317.
Zur Reduction benutzt: 9.1241.
Zone 428
. i8gi Februar io.
Beobachter : Kempf.
Photometer: D. Vergleichsterne: Nr. 14 und Nr. 16. Luft: 2—3.
ii°
1588
5h x m
2483
2183
2389
C •
22?80
4989
9.1766
9.2245
IO
1149
5 3
30.5
23.6
25.0
23-5
25.65
44.9
9.2727
9 - 307 I
l 9
1623
5 6
19.7
I4.9
16.O
15-3
16.48
39-8
8.9057
8.9298
0.3591
4- 0.90
7-37
17
1505
5 8
15.2
I3.6
16.O
15-5
15.08
41.i
8.8305
8.8569
0.4320
4- 1.08
7-55
17
1518
5 10
25-5
23.6
254
22.4
24.22
41.8
9.2261
9-2538
0.0351
-f- 0.09
6.56
16
1396
5 13
19-3
I 7.O
17.O
16.4
I7.42
42.0
8-9525
8.9806
0.3083
4 - 0.77
7.24
15
1494
5 15
17.6
15.6
17.O
154
16.4O
42.8
8.9015
8.9312
0.3577
+ 0.89
7-36
15
1504
5 17
15.O
I3.O
14.O
15.0
I4.25
42.9
8.7824
8.8123
0.4766
4 - 1.19
7.66
IO
1149
5 19
29.O
25.O
27.4
25.6
26.75
43-9
9.3066
9-3387
11
1588
5 22
26.4
2 1.0
24.O
22.5
23.48
47.6
9.2007
9.2419
11
1467
5 25
16.8
15.O
16.O
15-5
15.82
45-7
8.8711
8.9074
0.3815
+ 0.95
7.42
IO
1458
5 26
19.4
17-5
20.5
18.5
18.98
46.3
9.0244
9.0622
0.2267
+ 0.57
7.04
12
1469
5 28
33-5
32.6
33-5
34-0
33-40
44.8
9.4815
9 - 5 I 56
0.2267
— 0.57
5-90
13
1572
5 30
20.6
17-5
18.0
18.5
18.65
43-3
9.0098
9.0406
0.2483
4- 0.62
7.09
14
1600
5 32
23.0
20.9
23-5
234
22.70
42.9
9-1730
9.2029
0.0860
4- 0.22
6.69
l6
1433
5 34
22.0
18.i
21.8
20.5
20.60
40.7
9.0927
9.1184
0.1705
4 - 0.43
6.90
IO
1149
5 38
28.5
28.6
29.0
27-5
28.40
42.9
9-3545
9-3844
11
1588
5 40
24.8
21.6
24.0
234
23-45
45-9
9.1997
9-2365
Mittel aus den Vergleichsternbeobachtungen: 9.2658; 9.2903; 9.3105.
Zur Reduction benutzt: 9.2889.
Zone 429
1891 Februar io.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18. Luft: 2
— 3 -
11°
1588
5 h 43 ™
2185
1789
i 7?l
17?i
18840
4587
8.9984
9-0347
IO
1818
5 46
18.6
17.i
16.9
16.9
17-38
52.9
8-9505
9.0087
2
1685
5 50
15-5
14.4
14.8
14.1
14.70
53-7
8.8088
8.8701
0.1754
+ 0.44
7.12
3
1708
5 51
16.5
154
16.4
15.0
15.82
53-2
8.8711
8.9305
0.1150
+ 0.29
6-97
3
1723
5 52
18.2
17.7
16.6
16.i
17-15
53-3
8-9393
8.9990
0.0465
+ 0.12
6.80
3
1715
5 54
31.0
27.6
28.9
28.0
28.88
52.6
9-3679
9.4250
0.3795
— 0.95
5-73
3
1719
5 56
27.4
23.0
25-3
22.0
24.42
52.5
9.2328
9.2895
0.2440
— 0.61
6.07
3
1724
5 57
13-5
114
12.5
1 1-9
12.32
52.4
8.6583
8.7147
0.3308
4- 0.83
7-51
3
1 725
5 58
18.7
17.9
19-5
17-3
18.35
52-4
8.9961
9-0525
0.0070
— 0.02
6.66
11
1588
6 0
19.7
18.0
19.O
18.0
18.68
44-3
9.0111
9.0441
IO
1818
6 3
19.0
174
19-3
17-3
18.25
50.9
8*99 5
9.0426
.4
1751
6 5
16.9
154
15.0
14.2
15-38
50.8
8.8472
8.8979
0
-p*
0
+ 0.37
7-05
6
1729
6 7
25-4
23-3
24.2
22.2
23.78
49.4
9.2111
9-2575
0.2 120
— 0.53
6.15
*) 5
1742
6 9
21.8
19.6
20.8
21.4
20.90
50.1
9.1047
9 -I 532
O.IO77
— 0.27
6.41
7
1773
6 11
17.4
14.7
16.5
15.2
15-95
47-4
8.8781
8.9188
O.I267
4- 0.32
7.00
9
1733
6 14
14.8
12.7
12.5
12.0
13.00
46.1
8.7042
8.7415
O.304O
4~ 0.76
7-44
2
1720
6 16
16.6
13-5
15.2
14.2
14.88
52.6
8.8192
8.8763
O.1692
4- 0.42
7.10
0
2026
6 17
13-9
14.2
13-7
13.2
13-75
54-0
8.7520
8.8145
O.231O
4- 0.58
7.26
11
1588
6 20
22.1
19-3
20.5
20.0
20.48
43-0
9.0879
9.1180
IO
1818
6 22
20.0
16.9
17-3
17.8
18.00
48.8
8.9800
9.0246
Mittel aus den Vergleichsternbeobachtungen: 9.0217; 9.0434; 9.0713.
Zur Reduction benutzt : 9.044:;
*) 5 ° 1742.
Die Nähe von a Canis minoris stört sehr.
