363
Zone o° bis -j- 20 0 Declination.
363
B.D.
Sternzeit
I
II
m 1
IV
J
z
log sin 2 J
corrig.
für Ext-
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 596. 1892 Juni 16.
Beobachter: Müller. Photometer: Cu. Vergleichsterne: Nr. 33
und Nr. 37. Luft: 1-
—2.
7°3023
16 h 1 4 m 1
i8?6
i5?6
i 5 ?6
i6?4
i6? 55
4582
8.9093
8.9444
8 3582
16 18
16.6
15.2
15.2
15.8
15-70
48.6
8.8647
8.9087
15 2911
l6 2 1
26.1
25.8
26.0
26.5
26.10
37-4
9.2868
9.3070
0.3767
-0.94
3-78
*)i 5 291 1
l6 22
13-7
14-3
12.3
13.6
13.48
37-5
8.7351
8-7554
0.1749
+ 0.44
3-81
4 3069
l6 24
23.8
22.4
22.6
24.1
23.22
48-3
9.1916
9.2348
0.3045
— 0.76
3 - 9 6
16 2849
l6 2Ó
22.7
23-3
22.5
22.6
22.78
36.9
9-1759
9-1954
0.2651
— 0.66
4.06
19 3086
l6 28
22.6
23.6
22.6
25.6
23.60
33 -i
9.2049
9.2194
0.2891
— 0.72
4.00
7 3023
l6 31
17-5
17.4
15.8
17.8
17.12
45-8
8.9378
8-9743
8 3582
16 33
15-5
16.9
154
16.8
16.15
47-3
8.8886
8.9290
9 3298
l6 36
31.0
3 5 -o
30.1
304
31.62
43 -o
9-4391
9.4692
0.5389
— 1-35
3-37
*)i2 3252
l6 39
24-5
25.0
23-9
254
24.70
41.1
9.2421
9.2685
0.3382
— 0.85
2.52
4 3489
l6 42
36.0
36.7
35.8
38.9
36.85
49.2
9-5559
9.6017
0.6714
— 1.68
3-04
*) 4 3489
l6 44
20.1
18.0
17-5
17.6
18.30
49.2
8.9938
9.0396
0.1093
— 0.27
3.10
2 3403
l6 46
21.3
18.9
20.8
21.4
20.60
51.0
9.0927
9 -I 44 I
0.2 138
— 0.53
4.19
8 3582
l6 48
15-3
14.6
154
15.8
15.28
46.2
8.8417
8.8792
7 3023
l6 50
16.9
16.6
15-9
16.6
16.50
46.9
8.9067
8.9460
Mittel aus den Vergleichsternbeobachtungen: 8.9266; 8.9516; 8.9126.
Zur Reduction benutzt: 8.9303
*) Mit Blende 4 beobachtet.
Zone 597. 1892 Juni 24.
Beobachter : Kempf.
Photometer :
Cu. Vergleichsterne: Nr. 33 und Nr. 37. Luft:
2.
7 ° 3 02 3
l6 h 20 m
15-9
i 5 ?8
1584
i6?o
I 5”78
45°4
8.8689
8.9045
8 3582
16 23
13-5
14.4
13-7
14.0
13.90
48.1
8.7612
8.8038
15 2911
16 25
21.9
23.6
2 1.1
23-3
22.48
37-6
9-!650
9 -I 855
0.3244
— 0.81
3-91
4 3069
16 27
22.0
21.0
20.5
22.0
21.38
48.4
9-1235
9.1669
0.3058
— 0.76
3 - 9 6
16 2849
16 29
20.0
22.5
20.0
20.4
20.72
37 -i
9-0975
9.1172
0.2561
— 0.64
4.08
19 3086
16 31
21.8
22.2
2 1.8
23.6
22.35
33 -i
9.1602
9.1747
0.3136
— 0.78
3-94
*)ig 3086
16 33
10.7
11.6
II 4
I 1.0
11.18
33 -i
8.5752
8.5897
0.2714
-f- 0.68
4-05
7 3023
16 36
15-4
16.1
14-3
15.6
15-35
46.1
8.8456
8.8829
8 3582
16 38
13-1
154
14.4
14.6
14.38
46.9
8.7901
8.8294
9 3298
16 41
30.5
29.0
28.6
29.4
29.38
43 -o
9-3815
9.4116
0.5505
— 1.38
3-34
*) 9 3298
16 43
14.6
15.0
15.0
1 5-1
14.92
42.9
8.8214
8.8513
0.0098
+ 0.02
3-39
*) 12 3252
16 45
21.6
23.6
21.0
22.8
22.25
40.8
9-1565
9.1823
0.32 I 2
— 0.80
2-57
4 3489
16 47
33 -i
33 -o
33-5
334
33-25
48.9
9.4781
9-5230
O.6619
-1.65
3-07
2 3403
16 49
21.0
20.0
19-5
22.4
20.72
50.9
9-0975
9.1486
O.2875
— 0.72
4.00
8 3582
16 50
14-5
14.6
12.1
14-5
13.92
46.1
8.7624
8.7997
7 3023
16 52
16.0
16.5
16.0
17-5
16.50
47.0
8.9067
8.9463
Mittel aus den Vergleichsternbeobachtungen: 8.8542; 8.8561; 8.8730.
Zur Reduction benutzt: 8.8611
*) Mit Blende 4 beobachtet.
Zone 598. 1892 Juni 24.
Beobachter: Kempf.
Photometer: Ci. Vergleichsterne: Nr. 35
und Nr. 37. Luft: 2
— 3 -
11 0 3 15 6
17h jül
26? 5
2880
2689
3i?i
28812
4185
9-3467
9-3738
8 3582
17 3
31.0
3°-9
31-5
30.6
31.00
45-3
9-4237
9.4590
10 3165
17 5
25-9
25-5
23.1
23.6
24.52
41.7
9.2362
9.2637
O.1639
-4- 0.41
5-34
1 3408
17 8
15.6
14.0
15.O
15.0
14.90
51-1
8.8203
8.8720
0.5556
+ 1-39
6.32
18 3351
17 IO
2 6.6
29.1
28.0
28.5
28.05
34-2
9-3447
9.3606
O.067O
+ 0.17
5.10
16 3174
17 13
17.4
17-3
1 7.0
18.4
I 7-52
36.0
8-9573
8-9755
O.452I
+ 1.13
6.06
4 3422
17 15
36.0
37-9
384
38.3
37.68
48.2
9-5724
9 - 6 I 53
O.1877
— 0.47
4.46
0 3697
17 18
21.4
18.5
19-3
21.0
20.05
52.0
9.0702
9 -I 25 I
O.3O25
+ 0.76
5-69
ii 3156
17 20
29-5
28.6
26.6
30.1
28.70
41.4
9.3629
9.3899
