170
Müller und Kempf, Photometrische Durchmusterung
170
B.D.
Sternzeit
I
II
III
IV
J
2
log sin 2 /
corrig,
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 112. 1887 März 10.
Beobachter; Müller. Photometer: D
Vergleichsterne: Nr. 10
und Nr. 12. Luft: 1
—2.
IO°
818
6 h 50™
28°5
2 6? 4
2 787
2781
27842
4583
9.3265
9.3618
11
632
6
52
17.4
16.6
I 9*5
16.2
17.42
50.1
8-9525
9.0010
19
811
6
55
21.4
19.0
234
20.3
2 1.02
41-3
9 - 1 °95
9 -I 363
0.0540
+ 0.14
6-59
16
664
6
56
14-3
12.0
13-3
13.0
I 3 -I 5
43-6
8.7140
8-7454
0.4449
+ 1.11
7.56
16
667
6
58
15.8
14-3
15.6
14.1
14-95
44-3
8.8232
8.8562
0.3341
+ 0.84
7.29
11
672
6
59
12.7
14.0
13-3
12.5
13.12
48.3
8.7120
8.7552
0.4351
+ 1.09
7-54
12
673
7
0
17.4
14.1
154
13-5
15.1°
48.1
8.8316
8.8742
0.3161
-4-0.79
7.24
11
675
7
2
35-4
32.5
34-5
32.6
33-75
49.1
9.4895
9-5350
0.3447
— 0.86
5-59
11
632
7
5
17.6
15-7
17.8
15.6
16.68
51.6
8.9159
8.9694
IO
818
7
7
26.6
28.7
30.3
27.0
28.15
46.6
9-3475
9.3861
16
668
7
9
14-3
13.6
14.6
134
13.98
45-3
8.7662
8.8015
0.3888
+ 0-97
7.42
16
671
7
IO
14.0
134
134
13-4
13-55
45-2
8.7396
8.7747
0.4156
+ 1.04
7-49
14
787
7
12
24.6
2 3-7
25.6
24-3
24-55
47.0
9.2372
9.2768
0.0865
— 0.22
6.23
14
796
7
14
22.3
21.6
254
23.6
23.22
47.1
9.1916
9-2315
0.0412
— 0.10
6-35
14
804
7
15
17.7
16.0
18.0
1 5-7
16.85
47-3
8.9244
8.9648
0.2255
4- 0.56
7.01
15
713
7
16
1 7-7
17.4
18.3
174
17.70
46.3
8.9658
9.0036
0.1867
+ 0.47
6.92
11
632
7
18
16.4
15.8
19.4
17.2
17.20
53-2
8.9417
9.0011
IO
818
7
20
30.2
29.9
28.7
28.6
29-35
47-8
9.3807
9.4225
Mittel aus den Vergleichsternbeobachtungen: 9.1814; 9.1778; 9.2118. Zur Reduction benutzt: 9.1903.
Zone 113. 1887 März 10.
Beobachter: Kempf.
Photometer;
D. Ver
gleichsterne : Nr. 12
und Nr. 14. Luft: 2.
IO°
818
7 b
2 5 m
4280
37 ?o
39?0
3580
38825
4883
9.5836
9.6268
IO
1149
7
27
29.0
28.5
28.0
27.1
28.15
44 -o
9-3475
9 - 379 8
7
1150
7
29
22.5
20.2
23-5
21.1
2 1.82
48.2
9.1404
9 -I 833
0.3428
+ 0.86
6-95
7
1178
7
31
17-5
18.0
18.1
17.4
17-75
48.2
8.9682
9.0111
0.5150
+ 1-29
7-38
6
1155
7
32
19.0
19.1
21.1
19.6
I9.7O
48.9
9-0555
9.IOO4
0.4257
—(— 1 .06
7-15
6
1160
7
33
21.6
23.0
24-5
254
23.62
49.6
9.2056
9.2526
0.2735
-j- 0.68
6-77
6
11 72
7
34
24.0
30.4
32-5
28.4
28.82
49.4
9.3662
9.4126
0.1135
-j- 0.28
6-37
*) 2
1139
7 37
27.0
27.9
26.5
26.0
26.85
53-6
9.3096
9 - 37°5
0.1556
+ 0.39
6.48
IO
818
7
39
32-9
38.1
41.9
364
37-32
49-7
9-5653
9.6126
IO
1149
7
41
26.5
30.6
33-2
32.0
30-58
44.9
9.4130
9.4474
2
1144
7
43
22.4
22.7
23.0
23.0
22.78
53-6
9-1759
9.2368
0.2893
+ 0.72
6.81
2
1 1 71
7
45
16.5
16.0
18.4
14-5
16.35
53-9
8.8990
8.9611
0.5650
+ 1.41
7-50
4
11 8 1
7
47
19.4
19.4
19.0
18.6
19.10
52.1
9.0297
9.0850
0.4411
+ I.IO
7.19
5
1156
7
49
17.4
17.4
17.4
17-3
17-38
51-5
8.9505
9.0036
0.5225
+1.31
7.40
1
1275
7
50
23.0
24.1
24-5
25-5
24.28
55-3
9.2281
9.2961
0.2300
+ 0.58
6.67
1
1278
7
51
19.6
21.5
23-9
20.4
21-35
55-4
9.1224
9.1908
0.3353
4-0.84
6-93
IO
818
7
54
34-6
37 -i
384
37-8
36.98
5 T -3
9-5585
9.6109
IO
1149
7
55
27.7 1 30.8
38.0
30.5
31-75
46.0
9.4423
9-4793
Mittel aus den Vergleichsternbeobachtungen: 9.^033; 9.3300; 9.3431.
Zur Reduction benutzt: 0.^261.
*) 2 0 1139 Hellere Componente eines sehr weiten Doppelsterns.
Zone 114. 1887 März 10.
Beobachter: Müller.
Photometer: D. Vergleichsterne: TSTr. 12
und Nr. 14. Luft: 1
—2.
IO C
1149
7 1 59 ™
2483
20?4
2487
1 2 3°4
23820
4683
9.1909
9.2287
IO
818
8
1
32.0
28.4
30.2
; 28.7
29.82
52.1
9-3932
9.4485
IO
1015
8
3
18.6
1 7*7
20.6
18.3
18.80
48.6
9.0164
9.0604
0.3063
4 - 0.77
6.86
15
1087
8
.5
14.7
14.4
16.3
14.8
15-05
43-6
8.8288
8.8602
0.5065
4- 1.27
7-36
13
1147
8
6
16.6
16.0
I7.4
16.4
16.60
45-7
8.9118
8.9481
0.4186
4-1-05
7.14
13
H51
8
7
24.7
23.6
26.9
24-3
24.88
45-7
9.2480
9.2843
0.0824
4- 0.21
6.30
18
I I 12
8
9
23-4
22.4
23.2
1 21.3
22.58
42.0
9.1686
9.1967
0.1700
+ o -43
6.52
*7
1154
8
IO
14.0
13-3
14-5
13-5
13.82
42.7
8-7563
8.7858
0.5809
4 - 1-45
7-54
IO
8l8
8
12
30.4
29.4
31-3
29.8
30.22
53-4
9-4037
9.4639
IO
1149
8
14
25.6
24.4
26.2
24.1
25.08
47-7
9-2545
9.2960
