196
197
Zone o° bis -j- 20° Declination.
197
Pubi, des Astrophys. Obs. zu Potsdam. Bd.IX.
25
Grösse
7-23
6-53
7-57
7-93
7.29
7.42
6.60
6.82
7.28
7-57
5.66
8.19
7.48
7.88
6 - 93
7 - 73
7-37
6.78
6.96
7-31
7.61
7-13
7.02
7-95
7-52
7-59
7-75
7.90
7-54
B.D.
Sternzeit
I
II
III
IV
/
z
log sin 2 /
corrig.
für Ext. j
Diff.
in log.
Diff. in 1
Grössen 1
Grösse
IO°
4604
22 h
5 ° m
30?5
3 ° 8 l
2780
29-4
29825
44°6
9.3780
9.4117
10
4514
22
52
20.8
20.0
19.6
18.5
19.72
45-8
9.0563
9.0928
0.2284
+ O.57
7-05
IO
4516
22
53
28.5
30.9
29.1
32-4
30.22
4 Ó -3
9-4037
9 - 44 I 5
0.1203
-O.30
6.18
17
4549
22
54
20.0
23-3
2 1.2
21.1
21.40
40.2
9.1243
9.1491
0.1721
+ 0.43
6.91
12
4600
22
56
18.9
17.2
17-5
16.0
17.40
44-7
8.9515
8.9854
0.3358
+ 0.84
7-3 2
l6
4502
22
58
15-5
16.4
15-5
14.7
I 5-52
41-4
8.8549
8.8819
0-4393
+ I.IO
7-58
15
4404
22
59
1 5-7
I4.6
H -5
15.0
H -95
41-5
8.8232
8.8503
O.4709
+ 1.18
7.66
IO
4351
23
1
21.0
25.6
24.2
23-5
23.58
50.8
9.2042
9-2549
IO
4604
23
3
29.0
28.2
26.4
25.2
27.20
45-5
9.3200
9-3558
Mittel aus den Vergleichsternbeobachtungen
: 9-2945
; 9-3638; 9 - 3 ° 54 -
Zur Reduction benutzt: 9.3212
Zone 180. 1887 October 27.
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 42
und Nr. 44. Luft:
2 — 3 -
IO°
4604
23b
6 m
2Ó?4
23?6
2481
2383
24835
45?8
9-2305
9.2670
IO
4351
23
8
21.6
234
22.2
21.0
22.05
51-7
9 .I 49 1
9.2029
13
4Ó92
23
IO
18.4
18.4
18.4
16.5
17.92
44.8
8.9762
9.OIO3
O.2229
+ O.56
7.04
13
4708
23
11
1 7-3
16.9
18.4
17.1
17.42
44.9
8.9525
8.9869
O.2463
+ O.Ó 2
7.10
17
4577
23
13
134
13.2
12.0
12.6
12.80
40.9
8.6909
8.7169
O.5163
+ 1.29
7-77
17 4582
23
H
20.1
18.7
18.O
15-3
18.02
41-3
8.9809
9.OO77
O.2255
+ O.56
7.04
14 4609
23
15
19.6
18.8
19.4
18.3
19.02
43-6
9.0262
9.0576
O.1756
+ O.44
6.92
18
4794
23
17
26.2
25.O
25.O
23-4
24.90
40.4
9.2486
9-2737
O.0405
O. IO
6.38
IO
4351
23
19
22.7
2 I .O
21.0
20.4
21 .28
53 -o
9.1196
9.1 782
IO
4604
23
20
24.6
24.6
24.9
23-3
24-35
46.9
9-2305
9.2698
IO
4547
23
22
154
16.3
16.4
144
15.62
48.6
8.8603
8.9043
O.3289
-f- 0.82
7-30
IO
4554
23
23
20.6
20.0
20.2
17.4
19-55
48-3
9.0492
9.0924
0.1408
+ 0.35
6.83
11
4573
23
25
14.0
I4.9
13-5
14.7
14.28
47.6
8.7842
8.8254
O.4078
+ 1.02
7-50
15 4416
23
27
19-3
I9.6
l8.6
18.3
18.95
44-3
9.0231
9.0561
O.1771
+ 0.44
6.92
17
4592
23
28
22.6
2 1.6
23.6
22.3
22.52
42.6
9.1664
9- 1 95 7
O.O375
+ O.O9
6-57
17
4594
23
29
14.0
I 2.8
13-5
13.0
13-32
42.0
8.7249
8.7530
0.4802
+ .1-20
7.68
IO
4351
23
31
22.4
20.6
21.8
20.6
2 i -35
54-5
9.1224
9.1870
10
4604
23
33
25.6
24.4
25-9
24.0
24.98
48.2
9 - 2 5 12
9.2941
Mittel aus den
Vergleichsternbeobachtungen: 9.2350; 9.2240; 9.2405. Zur Reduction benutzt: 9.2332
Zone
l8l.
1887 November
3 *
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 40 und Nr. 42. Luft:
4 -
IO (
5 398 1
2I h t8 m
2482
22?5
2588
2386
24802
4888
9.2193
9.2639
IO
435 1
2 1
40
29.2
25.O
2 6.6
27.0
26.95
43-5
9.3126
9-3438
13
4120
21
42
16.5
16.5
16.4
16.9
16.58
40.9
8.9108
8.9368
0.3783
+ 0.95
7-75
17 4282
2 1
44
13.8
14-5
16.O
15-4
14.92
38.7
8.8214
8.8436
O.4715
+ i -18
7.98
16
4220
2 1
46
23-5
23-3
24-5
23.0
. 23-58
39-7
9.2042
9.2281
0.0870
+ 0.22
7.02
13
4355
2 1
47
21.1
20.1
20.9
19.1
20.30
42.6
9.0805
9.1098
O.2053
+ 0.51
7-31
13
4356
2 1
49
21.8
21.6
25.0
24.9
23-32
42.8
9 -! 95 i
9.2248
O.O903
+ 0.23
7-°3
15
4 U 7
2 1
51
23-5
23-5
2 3-7
25-5
24.05
41.8
9.2203
9.2480
O.0671
+ 0.17
6.97
IO
3981
2 I
53
23-5
24.0
254
23-5
24.10
50.4
9.2220
9-2715
IO
435 1
21
55
27-5
26.4
27.6
25.6
26.78
44-5
9-3075
9.3409
13
4360
2 I
58
31.0
33 -o
32.1
131*6
31.92
44.2
9.4465
9-4793
0.1642
— 0.41
6-39
11
4223
22
0
2 7.2
27.6
28.5
26.0
27.32
46.4
9.3236
9.3616
O.0465
— 0.12
6.68
14 4264
22
2
29.6
32.5
30.0
31-4
30.88
43-7
9.4207
9-4523
O.1372
— 0.34
6.46
14
4268
22
3
244
24.0
24-3
24.6
24.32
43-2
9.2295
9.2600
O.0551
+ 0.14
6-94
17
4294
22
5
38.6
39 - 6
39-5
40.1
39-45
41.1
9.6061
9-6325
0.3174
— 0.79
6.01
1 3
43 7 1
22
7
18.4
18.0
16.7
154
17.12
44.9
8.9378
8.9722
0.3429
-f- 0.86
7.66
IO
3981
22
9
23-5
22.6
25.8
22.9
23.70
52-3
9.2083
9.2643
IO
4351
22
11
294
28.9
28.4
29.1
28.95
45-8
9.3698
9.4063
Mittel aus den
Vergleichsternbeobachtungen: 9.3039; 9.3062; 9.3353-
Zur Reduction benutzt: 9.3151