Müller und Kempf, Photometrische Durchmusterung
154
154
B.D.
Sternzeit
I
a
III
IV
J
2
log sin 2 /
corrig.
für Ext.
. Diff.
in log.
Diff. in
Grössen
Grösse
Zone 72
1887 Februar 5'.
Beobachter :
Kempf.
Photometer :
D. Vergleichsterne: Nr. 6 und Nr.
8. Luft: 2.
9 °
472
4 1
39m
19-5
19?8
2 i?9
i8?7
I 9?98
44°6
9.0673
9.1010
8
385
4
42
25.1
29.9
35-3
31.0
30-32
51-5
9.4063
9-4594
19
432
4
45
19.4
19-3
18.5
19-5
19.18
39-4
9-0331
9.0565
0.1948
+ O.49
7-35
19
433
4
46
19.7
19.0
22.0
20.9
20.40
39-7
9.0846
9.1085
0.1428
+ O.36
7.22
17
454
4
47
21.2
20.1
25.0
18.5
21.20
42.0
9.H65
9.1446
0.1067
4 - O.27
7- 1 3
1 7
458
4
49
37 -i
39-4
39-9
35 -i
37.88
41.9
9-5763
9.6042
0.3529
— 0.88
5-98
*) 17
457
4
51
36.5
35-2
39-2
38.6
37-38
42.0
9-5665
9.5946
0-3433
— 0.86
6.00
14
492
4
53
14.0
12.9
13-7
13.0
13-40
45-4
8.7300
8.7656
0.4857
+ 1.21
8.07
8
385
4
55
2 5-7
29.9
32.2
30.8
29.65
53 -o
9.3887
9-4473
9
472
4
57
17.6
1 7-5
18.4
17-5
17-75
45-8
8.9682
9.0047
15
414
4
59
19.0
19.2
20.9
20.2
19.82
44-5
9.0605
9.0939
0.1574
+ 0.39
7-25
17
461
5
1
19.2
20.1
21.4
20.1
20.20
43 -i
9.0764
9.1067
0.1446
+ 0.36
7.22
17
471
5
2
19.4
22.4
21.9
21-5
21.30
42.9
9.1204
9-1503
0.1010
4-0.25
7.11
13
484
5
4
18.4
16.0
21.1
17.4
i8.22
47-2
8.9901
9.0302
0.22 11
+ 0.55
7.41
10
401
5
5
34-9
34-8
35-5
37-5
35-68
49-5
9-5317
9-5784
0.3271
— 0.82
6.04
14
502
5
8
15-2
17-3
18.6
1 7-5
I 7 -I 5
46.1
8-9393
8.9766
0.2747
+ 0.69
7-55
8
385
5
10
28.8
30.5
32.9
30.0
30.55
54-8
9.4122
9.4781
9
472
5
12
17.4
16.8
19.0
18.6
17-95
47.0
8-9777
9 -OI 73
Mittel aus den
Vergleichsternbeobachtungen: 9.2802; 9.2260; 9.2477. Zur Reduction benutzt: 9.2513
*) i 7 ° 457 - Die röthliche Farbe erschwert die Messungen.
Zone 73
1887 Februar 5.
Beobachter : Müller.
Photometer: D. Vergleichsterne: Nr. 8 und Nr. 10.
Luft: 2-
- 3 -
9 °
472
5 k
i6 m
I 4?7
i3?i
15-5
I3?6
I 4?2 2
4784
8.7806
8.8213
11
632
5
18
18.4
18.4
2 1.2
17.8
18.95
42.3
9-0231
9.0518
16
523
5
20
27.7
26.0
27-9
26.6
27.O5
39-8
9 - 3 1 56
9-3397
O.4142
— 1.04
6.21
16
527
5
21
17.6
17.6
18.5
18.7
l8.IO
40.5
8.9846
9.0099
0.0844
0.2 I
7.04
13
61Ó
5
23
12.4
I 3*5
14.4
11.5
12-95
43-3
8.7009
8.7317
O.1938
4- 0.48
7-73
13
62 1
5
25
18.0
16.0
18.7
18.7
I 7-85
42.8
8.9730
9.0027
O.0772
O. ig
7.06
16
544
5
26
23.0
22.8
23.1
20.5
22-35
39-7
9.1602
9.1841
0.2586
— O.65
6.60
17
666
5
28
28.2
29.6
26.5
2 7-3
27.90
39 -i
9.3404
9-3633
04378
1.09
6.16
9
472
5
30
13.6
13.6
I 5-9
12.8
13.98
48.7
8.7662
8.8105
11
632
5
31
19.6
19-5
19.4
17.4
18.98
43 -o
9.0244
9-0545
13
627
5
36
13-7
15.0
15.8
13.8
14.58
43-8
8.8018
8.8337
0.0918
+ O.23
7.48
19
643
5
38
18.5
16.6
18.0
16.3
17-35
38.2
8.9491
8.9705
0.0450
0.1 I
7- I 4
17
676
5
40
17.7
16.8
20.3
18.4
18.30
40.5
8.9938
9.0191
O.0936
— O.23
7.02
18
581
5
41
11.4
14.2
15.2
12.6
13-35
39 -o
8.7268
8-7495
0.1760
4- O.44
7.69
H
657
5
43
29.4
27.1
27-3
31-3
28.78
42.6
9-3651
9-3944
0.4689
— 1-1 7
6.08
16
559
5
45
1 1-7
11.4
12.4
10.7
ii -55
41.6
8.6030
8.6303
O.2952
4-0.74
7.99
9
472
5
47
14-3
13-4
14.2
12.0
13.48
5°-4
8.7351
8.7846
11
632
5
50
16.5
17-4
20.4
19.2
18.38
44.2
8-9975
9.0303
Mittel aus den Vcrgleichsternbeobachtungen : 8.9366; 8.9325; 8.9074. Zur Reduction benutzt: 8.9255.
Zone 74
. 1887 Februar 5.
Beobachter :
Kempf.
Photometer:
D. Vergleichsterne: Nr. 8 und Nr. io. Luft: 3.
ii°
632
5 1
55 m
20?5
2 I ?2
0 r O-
2 5-7
21?4
2 2?20
44%
9.1546
9.ì883
9
472
5
56
18.5
16.4
18.9
17-5
CN 1
00
51-4
8.9715
9.0243
19
672
5
59
45 -o
46.6
43-7
48.4
45-92
40.0
9.7127
9-7371
O.6232
-1.56
5-69
13
648
6
0
29.4
28.5
34 -i
33-5
31-38
45-7
9-4332
9.4695
0.3556
— 0.89
6.36
18
594
6
1
2 1.2
21.5
25.0
24-5
23-05
41.2
9.1856
9.2122
0.0983
— 0.25
7.00
15
592
6
3
17-3
1 7.0
19-5
18.1
17.98
43-6
8.9791
9.0105
O.IO34
4- 0.26
7-51
16
567
6
4
19.8
19.4
21.8
21.0
20.50
43 -o
9.0887
9.1188
O.OO49
— 0.01
7.24
16
569
6
5
29.8
30.9
33-5
31-5
3142
42.4.
9.4342
9.4631
1 O.3492
— 0.87
6.38
9
472
6
7
17.0
16.0
18.3
17.0
17.08
52.6
8.9358
8.9929
