166
Müller und Kempf, Photometrische Durchmusterung
166
B.D.
Sternzeit
1 j
II
TU
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 102. 1887 März 1.
Beobachter: Kempf. Photometer: D
Vergleichsterne: Nr. 16 und Nr. 18
Luft: 2-
"" 3 *
IO°
1818
6 h 16 m
1985
2 i?o
22?5
21?6
2I?I5
4986
9.1146
9.1616
11
1588
6 20
23-5
21.3
23-9
22.6
22.82
42.9
9-1773
9.2072
16
1612
6 22
29.0
27.0
29.8
25.0
27.70
40.0
9-3346
9 - 359 °
0.1768
— 0.44
6.24
i 7
1744
6 23
14.1
13.6
16.5
13.0
14.30
39-7
8.7854
8.8093
O.3729
+ 0.93
7.61
15
1734
6 25
15-4
15-5
14.0
15-3
15-05
41.2
8.8288
8-8554
O.3268
4- 0.82
7-50
12
1748
6 27
14.0
13-3
14-3
144
14.OO
43-4
8.7674
8.7984
O.3838
+ 0.96
7.64
12
1754
6 28
18.0
18.7
19.6
18.0
1848
43-7
9.0066
9.0382
O.1440
+ 0.36
7.04
!9
igi 1
6 30
26.4
22.1
26.1
24-5
24.78
37-3
9.2447
9.2647
O
ö
00
— 0.21
64^
11
1588
6 32
21.4
20.8
24.0
234
22.40
42.3
9.1620
9.1907
IO
1818
6 34
22.9
194
21.1
18.9
20.58
47-7
9.0919
9-1334
14
1831
6 36
21.0
23.0
25.0
23.0
23.00
42.0
9.1838
9.2119
0.0297
— 0.07
6.61
x 7
1778
6 38
15-4
15-5
17.1
154
I 5-85
38.9
8.8727
8.8952
0.2870
4-0.72
7.40
15
1775
6 39
234
23.2
25.6
22.6
23.70
41.1
9.2083
9-2347
0.0525
— 0.13
6-55
IO
1746
6 41
25.0
27.0
26.0
25-9
25.98
45-5
9.2831
9.3189
0.1367
— 0.34
6-34
16
1657
6 43
16.0
16.0
16.4
14-5
I 5-72
39-3
8.8658
8.8890
0.2932
+ 0.73
7.41
16
1659
6 44
17.0
i 5-5
15.0
14.1
15.40
38.7
8.8483
8.8705
0.3117
4- 0.78
7.46
11
1588
6 46
25.0
22.0
23-9
23-7
23.65
41.8
9.2066
9-2343
IO
1818
6 48
20.6
20.9
23.0
21-5
21.50
46.4
9.1282
9.1662
3
1724
6 52
14-5
15.6
14.0
15.0
14.78
49.4
8.8134
8.8598
0.3224
4- 0.81
7-49
3
i 7 2 5
6 53
20.5
18.7
21-5
22.2
20.72
49-5
9-0975
9.1442
0.0380
4-0.10
6.78
Mittel aus den Vergleich,Sternbeobachtungen: 9.1844; 9.1621; 9.2002. Zur Reduction benutzt: 9.1822.
Zone 103. 1887 März 1.
Beobachter:
Müller.
Photometer:
D. Vergleichsterne: Nr. 18 und Nr. 20. Luft:
3 -
IO°
1818
7 h o m
i8?o
1584
1984
i 5°7
1 7?I2
4585
8.9378
8.9736
9
2239
7 3
13.0
12-5
13.6
12.3
12.85
53-8
8.6943
8.7560
6
2030
7 5
21.3
20.0
21.0
19.7
20.50
50.1
9.0887
9.1372
0.2655
— 0.66
6.29
5
2049
7 7
18.6
17-3
2 1.0
16.3
18.30
51.0
8.9938
9.0452
0.1735
— 0.43
6.52
0
2379
7 8
17.0
14.8
16.7
154
15.98
55-3
8.8796
8.9476
0.0759
— 0.19
6.76
1
2163
7 10
14.7
1 1-9
13.0
11.8
12.85
54-7
8.6943
8-7597
0.1 120
4- 0.28
7-23
9
2047
7 11
12.0
12.3
134
11.7
12-35
47.1
8.6604
8.7003
0.1714
-b 0.43
7-38
3
2056
7 i 4
12.6
114
12.8
10.3
11.78
52.7
8.6199
8.6774
0.1943
4- 0.49
7-44
3
2057
7 15
14.6
12.4
15-3
12.6
I 3-72
52.7
8.7501
8.8076
0.0641
4-0.16
7-1
IO
1818
7 i 7
16.3
19.0
16.4
16.3
1 7.00
44-2
8.9319
8.9647
9
2239
7 19
134
12.5
12.5
12.4
12.70
52.0
8.6842
8.7391
2
2072
721
12.9
12.4
13-5
12.3
12.78
53-4
8.6896
8.7498
0.12 19
4- 0.30
7-25
2
2073
7 23
10.7
10.7
12.4
1 1-5
11.32
52.4
8.5858
8.6422
O.2295
+ 0.57
7-52
7
2036
7 25
154
17-5
16.6
16.0
16.38
47-8
8.9005
8.9423
O.0706
— 0.18
6.77
8
2134
7 26
16.9
15-7
17.7
15-3
16.40
46.8
8.9015
8.9406
O.0689
— 0.17
6.78
5
2074
7 28
18.2
16.4
18.6
19.2
18.10
49-3
8.9846
9.0307
0.1590
— 0.40
6-55
IO
1818
7 30
18.8
17.6
17.4
17.6
I 7-85
43-5
8.9730
9.0042
9
2239
7 32
12.5
14.0
14-5
134
13.60
50.6
8.7427
8.7928
Mittelaus den Vergleichsternbeobachtungen: 8.8648; 8.8519; 8.8985.
Zur Reduction benutzt: 8.8717.
Zone 104. 1887 März 1.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 18 und Nr.
20. Luft
3 -
9
3 2239
7 h 35 m
I l6?0
1581
i 8°5
16°6
16855
5083
8.9093
8.9585
IO
1818
7 37
20.7
21.0
23-5
22.2
21.85
43 -i
9 -I 4 I 5
9.1718
4
2081
7 39
24.0
25.6
26.1
26.8
25.62
50.0
9.2717
9.3199
0.2679
— 0.67
6.28
3
2099
7 4 i
16.9
18.5
18.0
17.0
1 7.60
5 i -5
8.9611
9.0142
0.0378
4- 0.09
7.04
2
2112
7 42
20.0
18.6
22.8
18.9
20.08
52.5
9-0715
9.1282
0.0762
•— 0.19
6.76
1
2210
7 44
11.0
13-9
14.8
13-5
13-30
53-3
8.7236
8.7834
0.2686
+ 0.67
7.62
9
2093
7 45
22.3
234
26.5
22.5
23.68
44-7
9.2076
9.2415
0.1895
— 0.47
6.48
9
2099
7 47
13.6
12.3
14.0
134
I3-32
! 45.0
8.7249
8-7595
0.2925
+ 0.73
7.68
