182
Müller und Kempf, Photometrische Durchmusterung
182
P.D.
Sternzeit
I
II
1—1
1—1
1—1
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 142. 1887 April 16.
Beobachter: Müller.
Photometer: Ci. Vergleichsterne: Nr. 23 und Nr.
25. Luft:
2.
8°2455
1l h 13 m
2 5-3
21?4
23" 7
2287
23828
4485
9-1937
9.2271
9 2 56o
II 15
14.8
14.4
16.0
i 3-7
14.72
43-8
8.8100
8.8419
14 2294
11 17
16.3
i 3 -i
15.2
14.0
14.65
38.3
8.8059
8.8275
0.1834
-f- O.46
5.80
11 2283
II 19
16.3
14.4
1 5 -i
i 3-3
14.78
41.9
8.8134
8.8413
0.1696
+ O.42
5-76
4 2 4°7
11 21
20.3
20.4
22.5
20.8
21.00
48.5
9.1087
9.1524
0.1415
— 0-35
4.99
6 2384
II 22
18.8
15.8
19.4
17.7
17.92
46.0
8.9762
9.0132
0.0023
O.OI
5-33
0 2761
I I 24
17-5
13-3
16.2
15-2
15-55
5 i -9
8.8565
8.91 IO
0.0999
+ 0.25
5-59
14 2367
I I 26
16.8
14.4
16.4
16.2
15-95
38.6
8.8781
8.9002
0.1107
+ 0.28
5.62
8 2455
I I 27
23-4
22.4
22.8
22.5
22.78
44.8
9-1759
9.2100
9 2560
I I 29
14.8
12.0
14.6
13.8
13.80
43-5
8-7551
8.7863
2 240g
II 31
17.0
15.8
16.7
16.8
16.58
50.0
8.9108
8.9590
0.0519
+ 0.13
5-47
6 2437
II 33
29.0
28.7
304
27.2
28.82
45-9
9.3662
9-4030
0.3921
— 0.98
4-36
11 2348
II 35
29.1
27.7
3 i -3
29.6
29.42
41.4
9-3825
9.4095
0.3986
1.00
4-34
3 2504
11 37
18.6
15.6
19.1
18.1
17-85
49.0
8.9730
9.0182
0.0073
0.02
5-32
19 2459
11 39
15.6
12.3
15.6
13-3
14.20
33-5
8-7794
8.7944
0.2165
+ O.54
5-88
17 2374
11 40
12.5
9.6
1 1-5
II.7
11.32
35 -i
8.5858
8.6028
0.4081
1.02
6.36
8 2455
11 42
23.8
21.4
234
23.0
22.90
45-2
9.1802
9-2153
9 2560
11 44
154
12.4
14-3
13.0
13-78
43-3
8-7539
8.7847
Mittel aus den Vergleichsternbeobachtungen: 9.0345; 8.9982; 9.0000. Zur Reduction benutzt: 9.0109.
Zone 143. 1887 April 16.
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 22
und Nr. 24. Luft:
2.
9° 2 374
I 2 11 34 m
32.5
34 3
34-9
3680
34842
5081
9-5045
9-5530
II 2372
12 36
22.0
21.9
21.5
21.4
2 I.70
42.9
9-1358
9 -i 657
16 2123
12 38
16.0
16.4
14.6
16.6
15.90
44.8
8.8754
8.9095
0.4277
+ 1-07
7-47
17 2231
12 40
17.1
17-5
18.5
17-5
I 7-65
43-8
8.9635
8.9954
0.3418
4 - 0-85
7-25
15 2206
12 42
17-5
17.7
17.0
20.7
18.22
46-5
8.9901
9.0284
0.3088
+ 0.77
7.17
H 2255
12 43
41.0
46.0
49.0
41.1
44.28
46.5
9.6879
9.7262
0.3890
— 0.97
5-43
18 2372
12 45
12.5
11.7
15.2
13.0
13.10
43-3
8.7107
8-7415
o -5957
4 ~ i -49
7.89
13 2280
12 46
11.7
12.2
12.7
11.0
11.90
47-3
8.6286
8.6690
0.6682
4 - 1-67
8.07
9 2374
12 48
32.5
31-5
34 *o
31.0
32-25
5 i -5
9-4545
9.5076
11 2372
12 5°
18.6
21.1
21.0
19.2
19.98
43-9
9.0673
9.0994
16 2144
12 52
19-5
22.5
21.1
21.6
21.18
44.9
9 - 1 1 57
9-1501
p
CO
+ 0.47
6.87
17 2259
12 53
10.5
1 1*5
12.0
11.1
11.28
44.2
8.5828
8.6156
0.7216
4 * 1 -8o
8.20
11 226g
12 55
14.7
18.4
18.4
18.0
17.38
49-9
8.9505
8.9984
0.3388
4-0.85
7-25
18 2390
12 56
17.9
16.7
17-5
16.2
1 7.08
43-3
8-9358
8.9666
0.3706
4-0.93
7-33
19 2366
12 57
13.0
15.0
1 5 *i
11.2
I 3-58
43 -i
8.7414
8.7717
0.5655
4 - 1.41
7.81
19 2368
12 58
21.9
22.5
22.0
24.0
22.60
43-2
9.1693
9.1998
0.1374
+ 0.34
6-74
9 2374
13 0
33-9
33-5
34-5
32.5
33 - 6 o
52.9
9.4861
9-5443
11 2372
13 2
20.0
20.0
22.9
22.1
21.25
44.9
9.1185
9.1529
Mittel aus den Vergleichsternbeobachtungen: 9.3594; 9.3035; 9.3486.
Zur Reduction benutzt: 9.3372.
Zone 144. 1887 April 16.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 26 und Nr. 28. Luft:
2.
11°2440
13 11 7 ’"
25-3
2884
3283
2987
28892
4382
9-3689
9-3994
9 2798
13 10
2 6.6
23.6
26.O
27-3
25.88
43-7
9.2800
9 - 3 ii 6
2 2517
13 12
30.7
30.0
29.7
27.7
29.52
51.8
9-3852
9-4394
0.0777
— 0.19
6.06
6 2559
13 14
33-8
28.5
30.0
32.9
31-30
48.2
9.4312
9.4741
0.1124
— 0.28
5-97
4 2583
13 15
18.8
16.5
19.4
17.4
18.02
49.8
8.9809
9.0285
0.3332
4-0.83
7.08
3 2616
13 17
18.7
15.8
17.4
18.0
17.48
5 i -5
8-9553
9.0084
o -3533
+ 0.88
7 -i 3
0 2920
13 19
27.4
27.0
27.O
26.6
27.OO
54-4
9 - 3 i 4 i
9.3782
0.0165
— 0.04
6.21
*) 6 2599
13 21
22.0
22.3
23-7
22.0
22.50
48.3
9 -i 657
9.2088
0.1529
4-0.38
6.63
11 2440
13 24
294
28.3
29.6
28.5
28.95
44.2
9.3698
9.4026
9 2798
13 26
26.3
24.4
26.6
23.8
25.28
43-4
9.2610
9.2920
