158
Müller und Kempf, Photometrîsche Durchmusterung
158
HD.
Sternzeit
I
11
III
IV
J
Z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 82.
1887 Februar io
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 10 und Nr. 12. Luft: 1
—2.
ii°
632
5 h
28 m
20?4
20? 2
21?9
2 I?4
20898
4288
9 - 1 079
9* 1 3 76
IO
818
5
31
32.0
32.5
35-6
37-5
34-40
42.2
9.5040
9-5325
6
865
5
33
14.0
15-2
15.6
LI -5
14.58
46.0
8.8018
8.8388
O.4971
+ 1.24
7.69
i
938
5
35
25.6
26.4
27.0
27.9
26.72
50.9
9-3057
9.3568
0.0209
— 0.05
6.40
i
957
5
37
24.0
21.8
23-4
24.0
23 - 3 °
50.9
9- I 944
9-2455
0.0904
+ O.23
6.68
o
988
5
38
25.0
25.0
28.5
25 - 1
25.90
52.4
9.2806
9-3370
0.001 I
0.00
6-45
4
877
5
40
35-3
36.1
36.6
37-5
36-38
47.8
9-5463
9.5881
0.2522
— 0.63
5.82
*) 8
900
5
42
12.9
12.i
14-5
12.8
13.08
44.6
8.7094
8.7431
0.5928
+ 148
7-93
11
632
5
45
16.7
18.0
21.i
19-9
18.92
43-9
9.0218
9-0539
IO
818
5
48
35-8
3 6 -9
33-9
39-0
36.40
42.4
9-5467
9-5756
2
916
5
52
39-5
44.4
40.9
41.0
41-45
50-5
9.6417
9 - 69 1 5
0-3556
— 0.89
5-56
2
920
5
54
16.8
15-4
18.2
17.6
i 7.00
50.6
8.9319
8.9820
0.3539
4- 0.89
7-34
2
924
5
55
25.0
20.8
27.0
23.6
24.10
50.7
9.2220
9.2724
0.0635
4-0.16
6.61
2
926
5
57
21.5
20.7
19.0
21.8
20.75
50-3
9.0987
9.1479
0.1880
4- 0.47
6.92
3
857
5
59
20.9
20.4
22.0
21.0
21.08
49-3
9.1118
9* 1 5 79
0.1780
+ 045
6.90
9
806
6
0
23.6
19.6
24.0
22.5
22.42
43-8
9.1627
9.1946
0.1413
+ 0.35
6.80
8
933
6
2
28.5
25.6
28.1
30-4
28.15
45-1
9-3475
9-3823
0.0464
— 0.12
6.33
11
632
6
5
20.4
18.5
21.6
22.5
20.75
45-4
9.0987
9- I 343
IO
818
6
6
35-4
36.7
37-5
37-0
36.65
42.8
9 * 55 1 9
9.5816
Mittel aus den Vergleichsternbeobachtungen: 9.3351; 9.3147; 9.3580-
Zur Reduction benutzt: 9-3359-
*) 80 900 dupl. Gemessen die hellere, nördlichere Componente. Messung sehr schwierig.
Zone 83.
1887 Februar io
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr.
und Nr.
16. Luft:
2.
IO°
1149
7 1 '
37 m
2384
2 I?2
2385
2 2?8
22872
44°6
9-1737
9.2074
11
1588
7
39
19-3
I 7.O
20.4
I 7.6
18.58
41.4
9.0066
9.0336
5
1 4 3 4
7
41
16.5
15-2
16.5
16.O
16.05
48.0
8.8833
8.9256
O.1936
4- 0.48
6-95
6
1405
7
42
I 5 ‘ I
12.5
15-5
I3.6
14.18
47.8
8.7782
8.8200
O.2992
+ 0.75
7.22
5
1448
7
44
13-7
12.6
16.3
I4.9
14.38
48.7
8.7901
8.8344
O.2848
4- 0.71
7.18
2
1437
7 46
10.4
IO.7
12.4
ii.4
11.22
5 1-i
8.5782
8.6299
O.4893
4- 1.22
7.69
3
1437
7
47
19.4
16.6
20.3
16.8
18.28
50.8
8.9929
9-0437
O.O755
4- 0.19
6.66
8
1543
7
49
22.7
26.7
24.4
23.80
45-7
9.2118
9.2481
O.1289
— 0.32
6.15
IO
1149
7
51
22.0
21.5
23.0
21.9
22.10
45-7
9.1509
9.1872
11
1588
7
53
20.5
16.7
19.2
18.3
18.68
41.7
9.0111
9.0386
8
1562
7
55
19.8
1 9-5
20.4
19-5
19.80
45-9
9-0597
9.0965
O.O227
4- 0.06
6-53
8
1568
7
57
15.0
14.4
14.0
12.7
14.02
45-6
8.7686
8.8046
O.3146
4 - 0.79
7.26
7
1539
7
58
19.8
20.3
20.5
19.4
20.00
46.5
9.0681
9.1064
O.OI28
«4- 0.03
6.50
7
1544
8
0
18.6
16.8
19.6
19-3
18.58
46.9
9.0066
9.0459
O.O733
4- 0.18
6.65
3
1488
8
i
22.4
23-5
24-5
24-5
23.72
50.6
9.2090
9 - 259 1
O.I399
— 0.35
6.12
5
1513
8
3
15.8
16.4
19.0
17-3
17.12
49.4
8.9378
8.9842
O.I35O
+ 0.34
6.81
IO
1149
8
5
21.6
21.3
22.4
21.0
21.58
46.8
9.1312
9 - 1 703
11
1588
8
7
18.6
19.2
20.1
20.3
19-55
42.3
9.0492
9.0779
Mittel aus den Vergleichsternbeobachtungen : 9.1205; 9.1129; 9.1241.
Zur Reduction benutzt: 9.1192
Zone 84.
1887 Februar io
•
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18. Luft:
—2.
li 0
1588
8 1
IO m
2 I?2
20?0
2 2?9
2381
21880
4284
9 - I 39 6
9* 1 685
IO
1818
8
13
25.I
22.0
23.2
22.5
23.20
42.0
9.1909
9.2190
2
1685
8
15
I9.O
2O.5
2I.5
22.5
20.88
51.0
9.1039
9* 1 5 53
O.0668
4-0.17
6.85
3
i 708
8
D
I7.6
18.5
23.6
22.0
20.42
50.5
9.0854
9-1352
O.0869
4- 0.22
6.90
3
1715
8
18
31-9
3I.8
36.7
37-3
34-42
50.0
9-5045
9-5527
O.3306
— 0.83
5.85
3
1719
8
20
28.1
27.4
31-4
32.6
29.88
50.0
9.3948
9.4430
O.2209
— 0.55
6.13
3
I 7 2 3
8
21
21.5
2 I.9
22.2
21.6
21.80
50.5
9 -Ï 396
9.1894
O.O327
4- 0.08
6.76
3
1724
8
23
16.3
I5.4
16.3
15.0
15-75
50.1
8.8674
8.9159
O.3062
4-0.77
7-45
3
1725
8
24
20.5
2O.3
22.1
22.6
21.38
50.2
9- I2 35
9-1723
O.O498
4-0.12
6.80
