148
Müller und Kempf, Photometrische Durchmusterung
148
B.D.
Sternzeit
I
II
III
IV
J
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 57
. 1887 Januar 18.
Beobachter:
Müller
Photometer
D. Vergleichsterne: Nr. 4 und Nr. 6. Luft: 2.
IO°
168
3 h 35 m
i6?o
i4?o
I 4?7
1580
14892
5082
8.8214
8.8702
8
385
3 37
25-4
22.4
27.6
24.1
CO
00
45-9
9.2480
9.2848
15
244
3 40
16.6
17-3
18.6
18.5
17-75
44.1
8.9682
9.OOO7
0.1068
+ 0.27
6-95
1 5
245
3 41
24-5
23.6
23-5
24.9
24.12
44-3
9.2227
9-2557
0.1482
— 0-37
6.31
13
255
3 43
16.4
17.6
18.1
17.6
17.42
46.6
8-9525
8.9911
0.1164
4- 0.29
6.97
l 9
282
3 45
22.4
21.0
22.0
234
22.20
41.0
9.1546
9.1808
O.0733
— 0.18
6.50
16
196
3 47
18.4
19.1
19.6
174
18.62
43-4
9.0084
9.0394
O.0681
+ 0.17
6.85
16
203
3 49
24.7
26.7
24.6
25.8
25-45
43-8
9.2664
9.2983
0.1908
— 0.48
6.20
IO
168
3 51
15.0
16.0
16.5
16.3
15-95
52.0
8.8781
8-9330
8
385
3 53
23.0
25.8
24.8
22.5
24.02
47.0
9- 2I 93
9.2589
IO
241
3 56
13-4
14.1
! 3-3
144
13.80
50.2
8-7551
8.8039
O.3036
4- 0.76
7-44
15
268
3 58
10.4
14.4
12.5
11.8
12.28
45-2
8.6555
8.6906
O.4169
4- 1.04
7.72
19
296
4 0
17.2
17-3
17.4
18.0
17.48
41.6
8-9553
8.9826
O.1249
4-0.31
6.99
17
276
4 i
17-5
19.6
19-3
17.0
18.35
43-6
8.9961
9.0275
0.0800
4- 0.20
6.88
11
248
4 3
13-7
15-2
15-1
13.8
14-45
48.7
8-7943
8.8386
0.2689
-f-0.67
7-35
11
251
4 4
11*4
12.0
12.7
11.8
11.98
48.6
8.6344
8.6784
O.4291
4-1-07
7-75
IO
168
4 7
16.2
1 5-6
17.2
16.5
16.38
54 -o
8.9005
8.9630
8
385
4 10
26.5
27-3
24.8
26.4
26.25
48.4
9.2914
9-3349
Mittel aus den Vergleichsternbeobachtungen: 9.0775; 9.0960; 9.1489.
Zur Reduction benutzt: 9.1075.
Zone 58
. 1887 Januar 18.
Beobachter: Kempf.
Photometer :
Ci. Vergleichsterne: Nr. 9 und Nr.
11. Luft :
2.
8°
652
4 h 20 m
1985
2 2?0
230
2585
22862
4384
9.1700
9.2010
9
683
4 21
26.5
234
27-5
22.5
24.98
42.7
9 - 2 5 12
9.2807
15
632
4 28
45-6
41.0
49-5
46.4
45.62
36.8
9.7083
9.7276
0.4718
—1.18
3.82
15
631
4 29
38-7
39-2
44.6
43-7
41-55
36.7
9.6434
9.6626
0.4068
— 1.02
3-98
15
637
4 31
22.8
22.0
27.0
25.1
24.22
3 6 -4
9.2261
9.2449
O.OIO9
+ 0.03
5-03
15
639
4 33
17.2
1 5-5
18.0
18.4
17.28
36.9
8.9456
8.9651
O.2907
4-0.73
5-73
12
598
4 35
19.0
18.0
19.4
21.0
19-35
39-6
9.0406
9.0643
0.1915
4- 0.48
5-48
1
757
4 37
17-5
15.6
16.9
18.8
17.20
51-3
8.9417
8.9941
O.2617
+ 0.65
5-65
8
652
4 39
24.0
22.1
22.5
23-5
23.02
43-8
9.1845
9.2164
9
683
4 40
22.4
24-5
27.9
26.5
25.32
42.4
9.2622
9.2911
13
690
4 43
15-5
17-5
17.0
20.4
17.60
39 - 1
8.9611
8.9840
O.27 18
4- 0.68
5.68
14
720
4 44
24-5
26.0
28.9
26.1
26.38
37-9
9.2954
9 - 3 i 63
0.0605
— 0.15
4-85
9
607
4 46
32.0
29.2
35-5
32.2
32.22
42.5
9-4538
9.4829
O.227 I
— 0.57
4-43
0
798
4 49
17.9
16.7
18.7
18.0
17.82
5 1 -7
8 - 97 I 5
9-0253
0.2305
4-0.58
5.58
12
618
4 5 1
26.0
28.0
31-5
32.0
29.38
40.2
9-3815
9.4063
0.1505
— 0.38
4.62
15
665
4 53
22.0
20.0
20.3
21.1
20.85
37 -o
9.1027
9.1223
0.1335
4-0.33
5-33
8
652
4 55
25.0
24.4
26.5
244
25.08
44.4
9-2545
9.2877
9
683
4 57
22.4
25.1
25-7
24.0
24.30
42.4
9.2288
9-2577
Mittel aus den Vergleichsternbeobachtungen: 9.2409; 9.2537; 9.2727.
Zur Reduction benutzt: 9.2558.
Zone 5g
. 1887 Januar 18.
Beobachter : Müller.
Photometer :
D. Vergleichsterne: Nr. 12 und Nr.
14. Luft:
2.
IO°
1149
6 h 22 m
2685
2I?5
2 5°4
2383
24818
4280
9.2247
9.2528
IO
818
6 24
35-8
26.7
29.4
324
31.08
43-7
9-4257
9-4573
9
860
6 27
9-5
10.6
12.5
12.0
11 - I 5
44.9
8.5729
8.6073
O.7791
4 - 1-95
8.04
1
1058
6 30
18.7
18.3
20.2
19.2
19.10
52.7
9.0297
9.0872
0.2992
4-0.75
6.84
3
964
6 31
34-6
35-5
34-3
36.0
35 - 1 °
50.5
9-5193
9.5691
0.1827
— 0.46
5-63
5
958
6 33
16.0
17.7
19.0
17.1
17-45
48.6
8-9539
8.9979
0.3885
4-0.97
7.06
8
1016
6 38
23-5
23.0
24.7
22.4
23.40
45-6
9-!979
9-2339
0 -I 525
4- 0.38
6.47
4
989
6 40
9 - 1
10.2
10.8
10.6
10.18
49.8
8.4947
8.5423
0.8441
4- 2.11
8.20
IO
818
6 42
2 8.6
31.8
34-6
32.4
31-85
44-7
9.4447
9.4786
IO
1149
6 43
26.2
25-5
23.8
25-7
25-30
42.2
9.2616
9.2901
