209
Zone o° bis -|- 20° Declination.
209
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 210. 1888 Mai 18.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 32
und Nr. 34. Luft: 2.
i i°278o
13 47 m
2585
2385
2480
2 2?4
23885
4483
9-2135
9.2465
9 3 2 °3
13 49
25-3
22.2
24.O
21.5
23-25
52.6
9.1927
9.2498
i5 2925
13 53
16.2
l6.1
16.9
I4.7
15.98
43 -i
8.8796
8.9099
0.2870
+ O.72
7-52
17 2926
13 55
26.0
24-3
24.6
24.O
24.72
41.2
9.2428
9.2694
0.0725
— O.18
6.6 2
13 3024
13 57
26.0
26.5
26.O
23.2
25.42
44-7
9.2654
9.2993
0.1024
— O.26
6-54
16 2840
13 58
25-5
254
27.6
23-5
25-50
42.1
9.2680
9.2963
0.0994
—-O.25
6.55
19 3036
14 0
27-5
23.O
24.3
22.2
24.25
39-8
9.2271
9.2512
0.0543
— O.14
6.66
*)i 2 2918
14 2
19-3
18.4
194
18.3
18.85
45-3
9.0187
9-0540
0.1429
+ O.36
7.16
11 2780
14 4
24.4
20.4
2O.5
21.5
21.70
43-2
9 -I 358
9.1663
9 3203
14 6
22.4
20.1
22.9
19.1
21.12
50.7
9 -II 34
9.1638
14 2969
14 8
36.0
34-7
33 -o
35-8
34.88
43 -o
9.5146
9-5447
0.3478
— 0.87
5-93
13 3°47
14 10
18.4
16.0
16.9
16.5
16.95
44.2
8.9294
8.9622
0.2347
+ o -59
7-39
13 3049
14 11
13.6
12.9
14.2
i 3 -i
13-45
44.0
8-7332
8.7655
0.4314
+ 1.08
7.88
18 3104
14 12
13-4
12.6
15-7
14.6
14.08
39-8
8.7722
8.7963
0.4006
+ 1.00
7.80
18 3108
14 13
19.6
20.9
20.0
20.0
20.12
40.1
9-0731
9.0977
0.0992
4-0.25
7-05
11 2903
14 14
18.5
19.0
18.9
1 7-1
18.38
45-8
8-9975
9.0340
0.1629
4- 0.41
7.21
11 2780
14 16
24-3
23.0
24-5
21.1
23.22
42.5
9.1916
9.2207
9 3203
14 18
21.7
20.4
18.7
2 1.1
20.48
49.4
9.0879
9- I 343
Mittel aus den Vergleichsternbeobachtungen: 9.2482; 9.1650; 9.1775.
Zur Reduction benutzt: 9.1969.
*) i2° 2918 dupl. Gemessen als ein Stern.
Zone 211. 1888 Mai 18.
Beobachter: Müller.
Photometer :
D. Vergleichsterne: Nr. 32 und Nr. 34. Luft:
2.
9°3203
I 4 h 24 m
ig?6
i8? 5
1985
i 8?5
19802
4889
9.0262
9.0711
11 2780
14 26
234
21.4
21.5
20.7
21-75
42.1
9- 1 3 7 7
9.1660
5 3072
14 28
31-3
30-5
294
27.7
29.72
48.9
9-3905
9-4354
0.3330
— O.83
5-97
i 3125
14 29
21.4
19.7
21.7
20.7
20.88
53-3
9- io 39
9.1636
0.0612
— O.I5
6.65
0 3401
14 31
17.0
14.6
1 7.2
16.0
16.20
54-4
8.8912
8-9553
0.1471
4 - 0.37
7.17
i 3131
14 33
21.4
19.0
2 1.4
19.9
20.42
52.5
9.0854
9.1421
0.0397
0.10
6.70
2 3004
14 35
14-5
13-9
144
13.0
13-95
51.6
8.7643
8.8178
0.2846
4- 0.71
7-51
5 3io8
14 36
17.4
15-7
17.1
14.7
16.22
49.2
8.8922
8.9380
0.1644
+ 0.41
7.21
11 2780
14 38
20.4
2 1 .4
21.3
19-3
20.60
41.7
9.0927
9.1202
* 9 3203
14 41
18.0
17.7
18.4
16.6
17.68
47-3
8.9649
9-0053
9 3 116
14 42
234
21.0
21.4
19-5
21.32
45-6
9.1212
9- 1 5 7 2
0.0548
— 0.14
6.66
*)3 3104
14 45
12.3
114
13-3
11.0
12.00
50.6
8.6358
8.6859
0.4165
4-1.04
7.84
5 3117
14 46
14.6
15-3
15-3
15-7
15.22
49-3
8.8383
8.8844
0.2 180
4-0.55
7-35
4 3 ° 9 6
14 48
28.3
29.6
28.4
27.8
28.52
49-7
9-3579
9.4052
O.3028
— 0.76
6.04
i 3 1 5 1
14 49
114
10.6
13.2
1 1-3
11.62
53-2
8.6082
8.6676
O.4348
+ 1.09
7.89
i 3154
14 50
15.8
15.0
14.6
1 5-5
15.22
53-2
8.8383
8.8977
O.2047
4- 0.51
7 - 3 1
11 2780
14 52
21.4
20.4
24-3
21.7
21.95
41.4
9- 1 45 3
9-1723
9 3203
14 54
20.6
18.9
194
18.6
19.38
46.2
9.0418
9-0793
Mittel aus den Vergleichsternbeobachtungen: 9.1186; 9.0627; 9.1258.
Zur Reduction benutzt: 9.1024.
*) 3°3io4 dupl.
Gemessen die hellere,
südlich folgende Componente.
Zone 212. 1888
Mai 27.
Beobachter:
Müller.
Photometer :
D. Vergleichsterne: Nr. 32 und Nr. 34. Lpft:
2.
1 l° 2780
I 4 h 2 I m
2 6?3
2i?o
2583
2380
23890
4283
9.2152
9.2439
9 3203
14 24
21.6
194
22.7
19-3
20.75
48.9
9.0987
9.1436
10 2971
14 27
22.6
20.7
22.4
19-3
21.25
46.9
9.1185
9 -I 578
O.O275
+ 0.07
6.87
17 2982
14 28
25-3
23-5
27.O
24.8
25-15
40.3
9.2568
9.2817
O.O964
— 0.24
6.56
13 3089
H 3 °
17.2
15-2
17.6
14.4
16.10
43-9
8.8859
8.9180
O.2673
4- 0.67
7-47
*)i 3 3091
14 32
21.4
18.7
2O.4
18.6
19.78
43 - 1
9.0589
9.0892
O.O961
+ 0.24
7.04
19 3072
14 34
18.1
16.0
18.4
154
16.98
37-7
8.9309
8.9515
O.2338
+ 0.58
7-38
11 2947
14 35
! 134
12.1
14-3
11.2
12.75
44.9
8.6876
8.7220
O.4633
4-1.16
7.96
11 2780
14 37
23.5
21.6
25.2
22.6
23.22
41.7
9.1916
g.2191
