202
Müller und Kempf, Photometrische Durchmusterung
202
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone
192.
1887 December 7.
Beobachter : Kempf.
Photometer: D. Verg
deichsterne : Nr. 12
und Nr. 14. Luft: 2.
io° 8i8
4 h i 5 m
34?4
3580
3686
34?6
35815
4488
9.5204
9-5545
io 1149
4 17
29.2
28.3
29.7
28.8
29.00
49.O
9 - 37 11
9.4163
19 1106
4 19
17.9
17-5
18.5
1 7 - 1
17-75
36.9
8.9682
8.9877
0.5236
+ 1 - 3 1
7.40
19 IIIO
4 21
31.6
29.4
314
33-2
31.40
36.5
9-4337
9.4526
0.0587
+ 0.15
6.24
19 1113
4 22
I 5 - 1
13.2
IÓ.8
14.0
14.78
36.6
8.8134
8.8324
0.6789
-h 1-70
7-79
14 1060
4 24
35-4
384
354
414
37-65
41.6
9*5 7 1 9
9.5992
0.0879
— 0.22
5.87
11 960
4 26
18.6
18.0
18.8
17.0
18.10
43-7
8.9846
9.0162
0.4951
4 - 1-24
7-33
12 937
4 28
16.8
13.6
14.6
14.6
14.90
43 - 1
8.8203
8.8506
0.6607
4 -1-65
7-74
10 818
4 30
42.4
36.8
33 -o
37-6
3745
43-8
9.5679
9.5998
10 1149
4 32
31-5
29.8
31-5
29.8
30-65
47-5
9.4148
9-4557
10 927
4 34
29.0
29-3
35-6
31.6
31-38
44.4
9-4332
9.4664
0.0449
+ 0.1 I
6.20
11 964
4 37
24.8
22.0
24.6
21.6
23-25
43 -°
9.1927
9.2228
0.2885
4- 0.72
6.81
19 1126
4 38
28.2
28.6
32.5
30.5
29-95
35-4
9.3966
9.4140
0.0973
4- 0.24
6-33
14 1074
4 40
22.4
234
28.4
22.2
24.10
40.6
9.2220
9.2475
0.2638
4- 0.66
6-75
13 1036
4 42
25-5
26.4
25.6
25.2
25.68
40.8
9-2737
9.2995
0.21 l8
+ 0.53
6.62
16 926
4 44
17.2
15-5
16.1
15-5
16.08
38-4
8.8849
8.9066
O.6047
4 - 1.51
7.60
IO 818
4 46
34 -o
344
35-6
43-9
36.98
43 -i
9-5585
9.5888
10 1149
4 48
31-4
31.2
27-5
32.6
30.68
46.1
9.4156
9-4529
Mittel aus den Vergleichsternbeobachtungen: 9.4854; 9.5278; 9.5208. Zur Reduction benutzt: 9.5113.
Zone
193 .
1887 December 9.
Beobachter : Müller.
Photometer: D. Vergleichsteme: Nr. 4 und Nr. 6.
Luft: 2—
3-
IO° 168
o h 4i m
i 8?5
I 9?2
20? 7
1986
19850
4281
9.0470
9-0753
8 385
0 43
33 -o
27.6
29.4
26.0
29.00
47-9
9*3 7 11
9 - 4 I 3 I
7 362
0 45
20.0
19.4
21.2
17.6
19-55
48.2
9.0492
9.0921
O.1407
4-0.35
7-03
7 37 1
0 46
17-3
14.4
15-7
14.8
15-55
48.8
8.8565
8.9011
0.3317
4- 0.83
7-51
5 338
0 48
21.5
19-3
20.4
19-3
20.12
50.3
9-0731
9-1223
0.1105
4- 0.28
6.96
9 319
0 49
18.9
16.4
14.8
14.7
16.20
46.1
8.8912
8.9285
0.3043
4- 0.76
7-44
9 321
0 52
20.6
18.7
17.0
18.6
18.72
46.0
9.0129
9.0499
0.1829
4- 0.46
7.14
9 323
0 53
22.8
21.8
22.4
23.6
22.65
46.3
9.1712
9.2090
0.0238
4- 0.06
6.74
8 385
0 54
304
29-5
30.6
26.4
29.22
47.0
9-3771
9.4167
10 168
0 56
19.6
17.4
19.2
17.6
18.45
41.6
9.0007
9.0280
i 431
0 58
23.6
20.8
22.5
21-5
22.10
53-8
9 - I 5°9
9.2126
0.0202
+ 0.05
6-73
*\ ^ ^ T ri
1 1
12.4
10.7
12.7
10.0
ii -45
54-8
8-5956
8.6615
°- 57 I 3
4 - i -43
8.11
J 0 4 X 5 |
1 2
12.4
12.0
12.6
13-5
12.62
54-8
8.6788
8.7447
0.4881
4* 1-22
7.90
0 421
i 3
16.6
154
15.8
14.0
15-45
54-8
8.8511
8.9170
0.3158
+ O.79
7-47
6 392
i 4
26.8
25.8
27.6
27.6
26.95
48.6
9.3126
9-3566
0.1238
— O.3I
6-37
6 398
i 5
32.7
29.0
28.7
30-7
30.28
49-3
9-4053
9 - 45 x 4
0.2 186
— 0.55
6.13
7 402
i 7
28.7
29.0
29-3
29.4
29.10
48.3
9-3739
9.4171
0.1843
O.46
6.22
10 168
1 8
19.4
17.7
I 9 .I
20.6
19.20
41.4
9.0340
9.0610
8 385
1 10
28.5
29.6
26.5
30.6
28.80
45-9
9-3657
9.4025
Mittel aus den Vergleichsternbeobachtungen: 9.2442; 9.2224; 9.2317.
Zur Reduction benutzt: 9.2328
*) o°4i5 dupl. Zuerst die südlich vorangehende Componente gemessen.
Zone 194. 1888 Februar 6
•
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 12
und Nr. 14. Luft:
2.
1O 0 818
7 h 42 m
2 I ?5
2 I?2
24?o
2o?5
2i?8o
5081
9.1396
9.1881
IO 1149
7 44
17-3
17-5
19-5
19.2
18.38
45-2
8-9975
9.0326
16 8 22
7 49
20.5
234
234
20.6
21.98
44.6
9.1464
9.1801
0.0570
O.I4
5-95
10 828
7 51
18.1
19.0
194
I9.9
19.10
50.1
9.0297
9.0782
0.0449
4 - 0.1 I
6.20
12 852
7 52
12.9
11 -5
12.8
12.2
12.35
48.1
8.6604
8.7030
0.4201
4- 1.05
7- x 4
*) 15 887
7 54
12.9
13.0
14.7
I3.8
13.60
46.3
8.7427
8.7805
0.3426
4- 0.86
6-95
18 920
7 56
15-5
12.5
13-5
11 -5
13-25
43 -i
8.7204
8-7507
0.3724
4- 0.93
7.02
18 923
7 57
14.4
14.0
144
13-5
14.08
43-3
8.7722
8.8030
0.3201
4- 0.80
6.89
