303
Zone o° bis -f- 20° Declination.
303
B.D.
Stern zeit
I
II
III
IV l
/
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 445. 1891 April 3.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 14 und Nr. 16
Luft: 1-
—2.
10°
1149
8 h 1 7 m
2Ö?0
2 2?4
25?6
2384
24835
4880
9-2305
9.2728
11
1588
8 19
22.0
20.4
22.3
21.8
2 1.62
42.8
9 - i 3 2 8
9.1625
14
1395
8 22
I9.4
15-5
18.0
16.6
I 7-38
43-5
8-9505
8.9817
0.202 I
+ O.51
6.98
IO
1262
8 24
12.5
II.7
I 2.0
I I.I
I 1.82
46.4
8.6228
8.6608
O.5230
+ I- 3 I
7.78
11
1344
8 26
23.O
23.0
24.O
23.2
23-30
45-8
9.1944
9.2309
O.O47I
0.12
6-35
13
1434
8 28
33-4
32.3
31-3
30.9
31.98
44.0
9.4479
9.4802
O.2964
— O.74
5-73
15
1347
8 29
15-3
12.8
13.2
13-3
I 3-65
42.5
8.7458
8-7749
O.4089
-}- 1.02
7-49
16
1298
8 31
27.7
234
25.0
25.6
25.42
41.8
9.2654
9.2931
O.IO93
— 0.27
6.20
IO
1149
8 33
24.6
22.0
23.0
21.7
22.82
49.6
9- 1 773
9.2243
11
1588
8 35
2 I. I
18.8
20.4
20.4
20.l8
43-8
9.0756
9 -l °75
18
i 3 2 4
8 39
H.7
9-3
12.4
9.9
10.82
41.7
8.5471
8.5746
O.6092
+ 1-52
7-99
18
1338
8 40
14.7
* 3-7
15.8
13-3
I4.38
40.7
8.7901
8.8158
O.3680
-4-0.92
7-39
18
1349
8 41
23.6
21.0
21.3
20.4
21.58
4 i -3
9 - : 3 12
9 -! 58 o
O.O258
+ 0.06
6-53
18
1362
8 43
1 1-5
10.7
11.8
10.7
11.18
41-5
8.5752
8.6023
O.5815
+ I -45
7.92
17
1392
8 46
1 1-7
9-5
12.0
10.1
10.82
42.9
8.5471
8.5770
O.6068
+ I- 5 2
7-99
16
1273
8 47
17.6
13.8
16.5
15.6
15.88
43-4
8.8743
8.9053
O.2785
+ 0.70
7.17
IO
1149
8 49
24.7
21.8
2 1.8
22.9
22.80
5 i -4
9.1766
9.2294
11
1588
8 52
20.5
21.3
19-5
19.0
20.08
45 - 1
9-0715
9.1063
Mittel aus den Vergleichsternbeobachtungen: 9.2177; 9.1659; 9.1678. Zur Reduction benutzt: 9.1838.
Zone 446. 1891 April 4.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 14 und Nr. 16.
Luft: 1-
—2.
IO°
1149
8 h 2 6 m
2883
2487
2583
2587
2 6?oo
4888
9.2837
9.3283
11
1588
8 29
25-3
20.9
23.8
22.7
23.18
43-4
9.1902
9.2212
1 7
1447
8 3 1
20.6
17.2
21.0
19.8
19.65
39-8
9-°534
9-0775
0.1899
+ 0.47
6.94
18
1423
8 33
16.3
14.2
16.9
14.6
15-50
39-8
8.8538
8.8779
0.3895
+ 0.97
7-44
19
1559
8 34
15.6
14.0
17.0
14-3
15.22
38.5
8.8383
8.8602
O.4072
-f- 1.02
7-49
12
1361
8 36
26.1
22.1
25-5
24.2
24.48
45-5
9.2348
9.2706
O.OO32
— 0.01
6.46
11
1408
8 37
19.8
16.5
20.6
17.0
18.48
45-4
9.0021
9-0377
O.2297
+ 0.57
7.04
IO
1370
8 39
19-3
17-3
19-3
16.8
18.18
46.6
8.9883
9.0269
O.2405
-b 0.60
7.07
IO
1149
8 41
26.0
22.9
27-5
25-9
25.58
50.4
9.2705
9.3200
11
1588
8 43
23.0
21.9
22.3
21.9
22.28
44-4
9 - 1 57 6
9.1908
IO
1335
8 45
29-5
27.9
29.0
27.7
28.52
'48.3
9-3579
9.4011
0.1337
— 0.33
6.14
16
1326
8 47
22.3
19.6
22.6
21.4
21.48
43-3
9.1274
9- i 582
O.IO92
+ 0.27
6.74
16
1352
8 48
17-5
i 5-7
18.2
16.0
16.85
42.7
8.9244
8-9539
0.3135
+ 0.78
7-25
16
1354
8 50
33-6
30.2
3 1 -!
33-3
32.05
42.8
9.4496
9-4793
0.21 19
— 0.53
5-94
15
1412
8 5 i
18.4
i 5-5
l8.I
16.8
17.20
43-4
8.9417
8.9727
O.2947
+ 0.74
7.21
15
1416
8 53
21.4
18.2
20.8
19.0
19.85
43-8
9.0618
9-0937
0.1737
+ 0.43
6.90
IO
1149
8 55
27.9
25.1
25-3
26.9
26.30
52.1
9.2929
9.3482
11
IS88
8 57
23-4
21.0
i 23.0
22.0
22.35
1 45-5
9.1602
9.1960
Mittel aus den Vergleichsternbeobachtungen: 9.2748; 9.2554; 9.2721. Zur Reduction benutzt: 9.2674.
Zone 447. 1891 April 4.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18. Luft:
1—2.
11 {
3 1588
9 11 O m
| 22?5
20?4
2480
2 I?I
2 2?00
4587
9.1472
9* 1 835
IO
1818
9 3
23.6
22.5
25.6
23-5
23.80
42.6
9.2118
9.2411
5
1857
9 5
32.6
3 i -5
33-0
31.0
32.02
49-3
9.4489
9.4950
O.2793
— 0.70
5 - 9 8
9
1843
9 6
24.I
23-5
28.0
24.9
25.12
45-5
9-2558
9.2916
0.0759
— 0.19
6.49
9
i860
9 8
l6.6
15-3
16.4
154
15.92
45 -o
8.8765
8.9111
O.3O46
-4- 0.76
7-44
9
1892
9 IO
I9.9
16.5
19.6
18.7
l8.68
44-9
9.0111
9-0455
0.1702
+ 0.43
7 -i 1
3
1913
9 11
i 9-5
16.0
19.7
I9.4
18.65
50.9
9.0098
9.0609
0.1548
+ 0.39
7.07
*)3
1933
9 14
16.1
154
16.1
154
15-75
5 KO
8.8674
8.9188
O.2969
+ 0.74
7.42
11
1588
9 i 7
24-5
20.9
24.O
2 1.4
22.70
47-3
9 - I 73 °
9-2134
38*
