186
Müller und Kempf, Photometrische Durchmusterung
186
13 .D.
Sternzeit
I
II
III
IV
/
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 152. 1887 Mai i.
Beobachter : Müller.
Photometer :
D. Vergleichsterne: Nr. 24 und Nr. 26. Luft:
2.
ii°
2372
I 2* 1
53 m
17?6
I 7?2
20?7
17?8
18832
44 82
8.9947
9.0275
11
2440
12
56
28.2
26.7
28.5
27-3
27.68
42.6
9-3340
9-3633
/
*) 1 5
2345
12
58
24.1
22.5
24.6
21.4
23-I5
41.6
9.1891
9.2 164
0.0635
— 0.16
6.31
18
2507
12
59
15-7
13.2
13.6
12.8
13.82
38.3
8-7563
8-7779
0.3746
+ 0.94
7.41
18
2510
13
0
14-3
13-7
1 5- 1
13.8
14.22
38.1
8.7806
8.8019
0.3506
4- 0.88
7-35
11
2376
13
2
1 7-7
*7-7
18.1
17-3
17.70
44.6
8.9658
8-9995
0.1530
-b 0.38
6.85
11
2377
13
3
18.4
18.6
18.1
18.3
18.35
44.9
8.9961
9-0305
0.1220
+ 0.31
6.78
i3
2436
13
5
12.6
12.4
13.6
12.0
12.65
43-o
8.6809
8.7110
O.4415
+ 1.10
7-57
11
2372
13
6
17.6
16.9
18.3
16.4
17.30
45-2
8.9466
8.981 7
11
2440
13
8
25.0
25-9
27.0
25.0
25.72
43-2
9.2749
9-3054
%
13
IO
7-i
7.0
8.7
7.2
7-50
37-8
8.2314
8.2522
O.9OO3
4- 2.25
8.72
J l y j
13
11
J 3-4
11.6
13-5
12.6
12.78
37-8
8.6896
8.7104
O.442I
4- 1.11
7-58
'9
2492
13
13
12.3
12.2
13.6
13.0
12.78
384
8.6896
8.7113
O.4412
4- I.IO
7-57
13
2443
13
15
14.4
134
14.9
13-5
14.05
44.2
8.7704
8.8032
0-3493
4- 0.87
7-34
15
2374
13
17
19-3
19-3
21.5
18.3
19.60
42.2
9-0513
9.0798
O.O727
4-0.18
6.65
15
2381
13
18
23-7
21.6
24-3
24-5
23-52
42.0
9.2021
9.2302
O.O777
— 0.19
6.28
16 2296
13
20
16.4
J 5-6
16.4
15-7
16.02
40.4
8.8817
8.9068
O.2457
4- 0.61
7.08
11
2372
13
21
16.6
15.8
18.3
174
17.02
46.6
8.9329
8-9 7 1 5
11
2440
13
23
24.7
25.2
24-5
23-3
24.42
44.2
9.2328
9.2656
Mittel aus den Vergleichsternbeobachtungen : 9.1954; 9.1436; 9.1x85.
Zur Redxiction benutzt: Q.i=;2i.
*) 15
2345 dupl.
Gemessen die hellere
, südlich folgende Componente.
**) 19
2483 dupl.
Zuerst die vorangehende Componente gemessen.
Zone 153.
1887 Mai 1.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 24 und Nr. 26. Luft: 2-
-3-
ii°
2440
13
27m
3089
34-0
32?I
3180
32800
4484
9.4484
9.4816
11
2372
13
29
22.9
21.5
234
21.4
22.30
47-4
9-1583
9.1990
17
2402
13
31
30.0
29.2
27.O
304
29-I5
41.4
9-3753
9.4023
O.0613
— 0.15
6.32
13
2465
13
34
25.2
25-5
254
234
24.88
45-i
9.2480
9.2828
O.O582
+ 0.15
6.6 2
12
2388
13
36
18.6
17.0
I 8.4
18.5
18.12
45-6
8.9855
9.0215
0.3195
4- 0.80
7.27
16
2307
13
38
17.9
174
I 7.6
18.5
I7-85
42.4
8.9730
9.0019
0-339 1
+ 0.85
7-32
16
2319
13
40
37-4
40.0
36.5
35-9
37-45
42.1
9-5679
9.5962
0.2552
— 0.64
5-83
18
2539
13
42
13.0
12.3
I3I
11.6
12.50
40-3
8.6707
8.6956
0.6454
4- 1.61
8.08
11
2372
13
45
21.9
21.4
19-3
20.5
20.78
49. 1
9.0999
9- I 454
11
2440
13
47
324
3°-5
33-5
33-8
32-55
46.0
9.4616
9.4986
14
2452
13
50
23.0
20.5
22.6
22.1
22.05
44.4
9-I49I
9.1823
0.1587
4- 0.40
6.87
18 2546
13
51
20.0
18.8
21.4
22.5
20.68
41.4
9.0959
9.1229
0.2181
+ 0.55
7.02
13
2482
13
53
18.4
19-5
17.7
19.7
18.82
45-9
9.0173
9.0541
0.2869
4- 0.72
7.19
19
2526
13
55
13.2
12.7
12.2
12.9
12.75
40.0
8.6876
8.7120
0.6290
+ 1 -57
8.04
18 2566
13
56
15.0
13-7
14-5
13.2
14.10
41-3
8-7734
8.8002
0.5408
+ i-35
7.82
17
2431
13
58
11.9
11.9
12.8
11.6
12.05
41.9
8.6394
8.6673
0.6737
4- 1.68
8.15
11
2372
13
59
20.4
234
22.5
22.8
22.28
50.7
9-I576
9.2080
11
2440
14
1
32.9
35-6
30.0
33-6
33-02
47-3
9.4727
9-5i3i
Mittel aus den Vergleichsternbeobachtungen: 9.3403; 9.3220; 9.3606.
Zur Reduction benutzt: 9.3410.
Zone
154 -
1887 Mai 5.
Beobachter: Müller.
Photometer:
Ci. Vergleichsterne: Nr. 25 und Nr. 27. Luft:
3-
9 (
2560
II 1
^ ? m
I 6?2
i3?i
i 5 ?4
1486
14882
43 ”4
8.8157
8.8467
11
2485
1 1
34
234
22.0
22.7
22.9
22.75
43-3
9.1748
9.2056
9
2545
11
37
23-5
20.6
21.3
22.5
2 I.98
43-5
9.1464
9.1776
0.1452
— 0.36
5-°9
7
2479
11
38
33-5
31.0
33-2
32.0
32.42
45-2
9-4585
9.4936
0.4612
— I - I 5
4-30
4
2556
1 1
40
ì5.ò
13-7
17-5
154
15-55
48.2
8.8565
8.8994
0.1330
+ 0.33
5.78
7
2502
1 1
41
24.8
24.8
24-5
24.8
24.72
45-3
9.2428
9.2781
0.2457
— 0.61
4.84
9
2583
11
43
324
30.6
33-7
334
32.52
43 - 1
9.4609
9.4912
0.4588
— 1-15
4-30
15
2436
11
44
20.0
18.0
19.9
20.0
19.48
37-2
9.0461
9.0660
0.0336
— 0.08
5-37
9
2560
11
47
II 1 5*7
144
16.9
154
15.60
43-3
8.8592
8.8900