Zone o° bis 20° Declination.
191
190
191
Grösse
6.87
6.23
6.42
7.62
6.2g
6.63
6.51
7.04
6.87
7.21
6.47
6.18
6.79
7.21
7.16
7.72
6.46
7.80
7.04
743
7-35
6-54
6-37
7-39
6-95
7.22
7.02
7.86
6.51
B.D.
Sternzeit
I
II
111
IV
/
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
i o° 43 51
2 2 11 7" 1
2387
2486
2585
2685
25808
45o
9-2545
9.2903
11 3996
22 IO
24.0
22.5
24-3
23.2
23-50
50.4
9.2014
9.2509
0.0518
— O.13
6.67
18 4252
22 12
17.8
15-5
16.6
16.5
1 6.60
44.4
8.9118
8.9450
0.2541
4- 0.64
7-44
G 4115
22 14
22.0
19.2
18.5
19.6
19.82
45-5
9.0605
9.0963
0.1028
4 0.26
7.06
16 4029
22 l6
15-4
13-9
16.5
16.5
I5-58
46.4
8.8581
8.8961
0.3030
+ 0.76
7-56
4 4175
22 l8
23.1
20.0
21.0
22.6
21.68
43-8
9-1350
9.1669
0.0322
4 0.08
6.88
19 4177
22 19
16.5
15-5
17.0
I4.O
15-75
44.0
8.8674
8.8997
0.2994
+ 0.75
7-55
10 3981
22 2 1
20.5
19.1
20.2
19.2
19-75
53-7
9.0576
9.11 89
10 4351
22 24
21.9
23.0
23.5
24.8
23-3°
1 47-o
9.1944
9.2340
Mittel aus den
Vergleichsternbeobachtungen: 9.1943; 9.2266; 9.1764.
Zur Reduction benutzt: 9.1991
Zone 165
. 1887 October 13.
Beobachter : Möller.
Photometer :
D. Vergleiehsterne: Nr. 42 und Nr.
44. Lu ft :
2.
IO ° 435 i
22 1 * 27" 1
2 I?4
2 0? 3
19?6
i 8?7
20?00
4782
9.0681
9.1082
10 4604
22 29
26.6
234
25.2
24.1
24.82
43-4
9.2460
9.2770
14 4393
22 31
2 7-5
22.4
2 6.8
23-5
25-05
44-5
9-2535
9.2869
0.1160
— 0.29
6.19
13 4491
22 32
9.0
7.8
10.0
8.3
8.78
44.8
8-3673
8.4014
O.7695
4 i-9 2
8.40
13 4487
22 34
18.0
17.4
17-3
16.4
17.28
45-5
8.9456
8.9814
O.1895
+ 0.47
6-95
12 4437
22 35
13.0
10.5
12.4
I 1.0
11.72
46.6
8.6156
8.6542
O.5167
4 1-29
7-77
17 4382
22 37
22.4
21.7
21.7
20.0
21.45
42.4
9.1263
9-I552
O.OI57
4 0.04
6.52
19 4489
22 39.
12.4
11-5
12.7
I 1.0
11.90
40.6
8.6286
8.6541
O.5168
4-1-29
7-77
10 4351
2 2 40
19.8
18.2
19.2
18.5
18.92
48.5
9.0218
9 -o 655
10 4604
22 42
24.4
25.0
22.6
21.2
23-30
44.1
9.1944
9.2269
19 4490
22 44
13-5
11*9
13*1
IO.5
12.25
41-3
8.6534
8.6802
O.4907
4-1-23
7.71
19 4494
22 45
10.7
9.6
10.6
9.6
10.12
41.1
8.4896
8.5160
O.6549
4 1-64
8.12
19 4501
22 47
15-5
14-5
16.5
16.3
15-7°
40.6
8.8647
8.8902
O.2807
+ 0.70
7.18
13 45o6
22 49
13.0
11. 6
12.6
12-5
I 2.42
47.0
8.6652
8.7048
O.4661
4- 1.17
7-65
ii 4368
22 51
16.4
154
18.4
16.4
16.65
48.3
8.9144
8.9576
O.2133
4-0.53
7.01
17 4401
22 53
22.6
18.6
22.2
2 1.6
21.25
43-4
9.1185
9-1495
0.02 14
4- 0.05
6-53
10 4351
22 55
21.0
18.5
21.3
18.4
19.80
50.2
9-0597
9.1085
10 4604
22 57
21.8
24.7
24.8
23.O
23-58
45-i
9.2042
9.2390
Mittel aus den Vergleichsternbeobachtungen : 9.1926; 9.1462; 9.1738.
Zur Reduction benutzt: 9.1709.
Zone 166
1887 October 21.
Beobachter : Kempf.
Photometer: D. Vergleichsterne: Nr. 40 und Nr. 42. Luft: 2
— 3 -
io 0 3g8i
21 h 1O™
20? 2
21?4
20?0
20?4
20850
4680
9.0887
9-1257
10 4351
21 12
23-5
244
25.6
24.4
24.48
42.2
9.2348
9-2633
ii 4019
21 15
24.2
29-5
27.4
24.0
26.28
44-7
9.2923
9.3262
O.1278
— 0.32
6.48
14 4074
21 17
14.4
12.8
16.0
13-9
14.28
41.4
8.7842
8.8112
O.3872
+ 0.97
7-77
18 4276
21 20
24-5
26.0
26.9
25.2
25-65
38.5
9.2727
9.2946
O.O962
— 0.24
6.56
19 4195
21 21
16.0
18.0
19.4
16.8
17-55
37-o
8.9587
8.9783
0.2201
+ 0.55
7-35
19 4196
21 23
18.5
16.6
15-9
15.0
16.50
37-2
8.9067
8.9266
O.2718
+ 0.68
7.48
16 4053
2 I 24
16.6
15-7
16.0
13-9
15-55
40.5
8.8565
8.8818
O.3 l66
40.79
7-59 .
10 3981
2 1 27
23-5
17-5
21.5
21.0
20.88
47.6
9.1039
9 -I 45 I
10 4351
21 29
22.5
25-5
26.0
26.0
25.00
42.9
9-2519
9.2818
14 4083
21 32
20.4
20.6
20.8
19-5
20.32
42.6
9.0813
9.1106
O.0878
4 0.22
7.02
14 4096
21 33
19.9
18.0
21.0
18.5
19-35
42.7
9.0406
9.0701
O.I283
40.32
7.12 •
II 4065
21 35
H -5
17.0
15.0
14.0
15.12
46.1
8.8327
8.8700
O.3284
4 0.82
7.62
1 1 4066
21 36
13.6
12.9
14-5
13.0
13-50
46.0
8.7364
8-7734
O.425O
4 1.06
7.86
IO 4126
2 i 38
20.4
22.5
24.4
22.8
22.52
46.4
9.1664
9.2044
O.O060
— 0.02
6.78
16 4086
21 39
19-5
194
20.5
19.6
19-75
41.8
9.0576
9 -o 853
O.II31
4 0.28
7.08
10 3981
21 41
19-5
20.6
20.5
20.8
20.35
49.1
9.0826
9.1281
10 4351
21 43
25.0
24.0
23-5
23.0
23.88
43-7
9-2145
9.2461
Mittel aus den Vergleichsternbeobachtungen: 9.1945; 9- 21 35 > 9*1871. Zur Reduction benutzt: 9.1984.
24*
