20*
158
159
Zone o° eis -j- 20 ° Declination.
159
B.D.
Sternzeit
1
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
ii°
1588
8 h 2Ó m
25?o
2 i?i
24-5
2589
2 4? 12
43°3
9.2227
9-2535
IO
1818
8 28
22.5
21.4
23-7
24-5
23.02
41.9
9.1845
9.21 24
4
1751
8 3 1
22.5
20.0
21.0
20.4
20.98
49.4
9.1079
9-1543
0.0678
+ 0.17
6.85
7
1773
8 32
20.0
19.7
23.2
21.4
21.08
46.4
9.1118
9.1498
0.0723
■4-O.18
6.86
6
1729
8 34
29.8
31.0
33-5
28.5
30.70
48.1
9.4161
9-4587
0.2366
— 0-59
6.09
2
1720
8 35
ig.O
19.0
21.0
19.0
19.50
51-9
9.0470
9-1015
0.1206
4-0.30
6.98
o
2026
8 37
i8.2
15-5
18.3
15-5
16.88
53-3
8.9259
8.9857
0.2364
+ O.59
7.27
9
1733
8 3^
18.3
16.5
16.6
15-9
16.82
45-2
8.9229
8.9580
0.2641
4- 0.66
7-34
5
1742
8 40
25.8
234
26.6
2 9-5
26.32
48.8
9-2935
9 - 338 i
0.1160
— 0.29
6-39
11
1588
8 43
23-4
24-3
24-5
23-7
23.98
44.4
9.2179
9-2511
IO
1818
8 45
23.6
22.4
26.7
21.1
2345
42.0
9.1997
9.2278
Mittel aus den Vergleichsternbeobachtungen: 9093 8 ; 9 - 2 3 2 9 ; 9 - 2 395 -
Zur Reduction benutzt: 9.2221.
Zone 85
1887 Februar n.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 14 und Nr. 16. Luft: 1
—2.
IO°
1149
4 ll 37 m
20?3
20? 7
20?3
20?6
20848
4780
9.0879
9-1275
11
1588
4 40
18.5
18.4
20.6
17.4
18.72
52.2
9.0129
9.0685
i6
1396
4 43
I4.6
13.2
14-3
I4.4
14.12
45-3
8.7746
8.8099
0-3151
4-0.79
7.26
i 7
I 5°5
4 44
I 1.6
11.7
12.7
12.3
12.08
43-8
8.6415
8.6734
0.4516
+ 1.13
7.60
11
1467
4 46
13-5
13.2
15.0
13.0
13.68
49-5
8.7477
8.7944
0.3306
4- 0.83
7-30
. ig
1623
4 50
12.6
114
13-9
12.4
12.58
41-5
8.6761
8.7032
0.4218
+ 1-05
7-52
13
1572
4 53
13-7
14.8
16.0
I3.6
14.52
47.0
8.7984
8.8380
0.2870
4- 0.72
7.19
17
1518
4 54
18.0
18.2
20.0
18.4
18.65
43-5
9.0098
9.0410
0.0840
4- 0.21
6.68
10
1149
4 56
24.2
20.5
22.4
22.6
22.42
45-4
9.1627
9.1983
11
1588
4 59
18.6
18.6
20.6
I9.7
19.38
50.0
9.0418
9.0900
15
1494
5 i
14.4
13.2
15-3
13-3
14.05
44.2
8.7704
8.8032
0.3218
4- 0.80
7.27
15
1504
5 2
15.6
134
13.2
12.4
13-65
44-3
8.7458
8.7788
0.3462
4- 0.87
7-34
H
1600
5 4
18.0
17.7
19.7
16.7
18.02
45-5
8.9809
9.0167
0.1083
4- 0.27
6.74
IO
1458
5 6
16.2
15-3
17.0
15-3
15-95
48.2
8.8781
8.9210
0.2040
4- 0.51
6.98
1 2
1469
5 7
26.5
24.7
29.4
25.6
26.55
46.8
9.3006
9-3397
0.2147
— 0.54
5-93
16
1433
5 8
16.6
15.8
17-3
15.6
16.32
43-3
8.8974
8.9282
0.1968
4- 0.49
6.96
11
1588
5 n
18.9
19.4
18.3
18.7
18.82
48.7
9-0173
9.0616
IO
1149
5 13
24.2
22.2
22.0
22.2
22.65
44.2
9.1712
9.2040
Mittel aus den Vergleichsternbeobachtungen: 9.0980; 9.1442; 9.1328.
Zur Reduction benutzt: 9.1250.
Zone 86.
1887 Februar 13
Beobachter : Kempf.
Photometer :
D. Vergleichsterne: Nr. 8 und Nr. io. Luft:
1.
9 °
472
5 h o™
O
C •
I 7 ?2
i 8?7
i6?6
17838
46 ?i
8-9505
8.9878
a
11
632
5 4
22.4
21.6
26.5
22.0
23.12
41.8
9.1880
9-2157
12
473
5 7
35-2
31.0
32.1
2 8.6
31.72
45-7
9.4416
9.4779
0.3917
— 0.98
6.27
12
477
5 8
2 7-3
22.5
23-5
24.1
24-35
45-3
9-2305
9.2658
0.1796
— 0.45
6.80
18
484
5 10
22.0
20.6
22.4
21.5
21.62
40.1
9.1328
9-1574
0.0712
— 0.18
7.07
5 12
18.8
15.0
20.9
174
18.02
38.8
8.9809
9.0033
0.0829
4- 0.2i
7.46
) *9
5 o 7 1
5 13
10.4
8.0
11.0
7-5
9.22
38.9
8.4095
8.4320
0.6542
+ 1.64
8.89
IO
444
5 15
22.4
18.2
22.5
20.0
20.78
47.2
9.0999
9.1400
0.0538
— 0.13
7.12
14
565
5 17
15.8
14.0
15-3
14-5
14.90
44.1
8.8203
8.8528
0-2334
4- 0.58
7-83
9
472
5 19
18.1
17.0
18.1
17.0
17-55
47.6
8.9587
8.9999
11
632
5 21
18.0
20.0
22.8
23-5
21.08
42.4
9.1118
9.1407
16
450
5 24
16.5
17.0
17.7
16.8
17.00
43 -i
8.9319
8.9622
0.1240
+ 0.31
7-56
»7
564
5 26
21.5
21.0
24-5
22.0
22.25
42.1
9-1565
9.1848
0.0986
— 0.25
7.00
**)n
487
5 27
22.5
19.2
20.4
19.8
20.48
47.8
9.0879
9.1297
0.0435
O.I I
7.14
16
458
5 29
18.4
174
18.5
17.2
17.88
43-4
8.9744
9.0054
0.0808
4- 0.20
7-45
13
568
5 30
21-5
18.5
19.8
17.4
19.30
46.0
9.0384
9-0754
0.0108
4- 0.03
7.28
17
575
5 32
25-5
26.0
30.0
27.0
27.12
42.6
9-3177
9 - 347 °
0.2608
— 0.65
6.60
9
472
5 34
16.0
18.7
19.0
17.0
17.68
49.0
8.964g
9.0101
11
632
5 37
21.8
-20. 1
24.0
20.5
21.60
43-3
9.1320
9.1628
Mittel aus den Vergleichsternbeobachtungen
: 9.1018; 9.0703; 9.0864. Zur Reduction benutzt: 9.0862.
*) 19 0 537 dupl. Zuerst die nördlich vorangehende Componente gemessen.
**) 11 487 dupl. Gemessen die hellere Componente.
i i
t I
m