272
Müller und Kempf, Photometrische Durchmusterung
272
B.D.
0 • 1
bternzeit
I
II
III !
IV
/ 1
z
log sinV
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
IO°
197
o h 4 m
1585
1381
1685
1581
15805
45 82
8.8288
8.8639
0.2315
+ 0.58
7.26
0 6
13.6
“•5
134
12.4
12.72
43-7
8.6855
8.7171
0.3783
+ 0.95
7-63
r T
J 11
20I<|
0 7
10.0
7.0
8-3
74
8.18
43-6
8.3063
8-3377
0.7577
+ 1-89
8-57
11
205
0 8
29.0
27.0
31.6
30.5
29.52
44.1
9-3852
9-4177
0.3223
— 0.81
5.87
11
207
0 10
17-5
16.2
17.7
16.4
16.95
44.1
8.9294
8.9619
0-1335
-f-0.33
7.01
13
24O
0 12
22.0
20.5
22.4
21.5
21.60
41-3
9-Ì320
9- 1 588
0.0634
— 0.16
6.52
16
I 76
0 14
26.4
24.4
25-5
23-5
24-95
38.5
9-2503
9.2722
0.1768
— 0.44
6.24
IO
l68
0 16
17.4
15-1
17.1
16.1
16.42
43 - 1
8.9025
8.9328
8
385
0 19
26.5
25.0
22.2
23.0
24.18
50.2
9.2247
9-2735
Mittel aus den Vergleichsternbeobachtungen: 9.0890; 9.0942; 9.1031.
Zur Reduction benutzt: 9.0954.
*) ii° 201 dupl. Zuerst die vorangehende Componente gemessen.
Zone 368.
1889 November 23.
Beobachter:
Kempf. Photometer
D. Vergleichsterne: Nr. 6 und Nr. 8. Luft:
[.
8°
385
l‘ 54 »
2585
22? 6
2 3?o
2386
23868
4387
9.2076
9.2392
9
472
I 56
14-5
12.5
14.9
x 3-7
13.90
47-3
8.7612
8.8016
6
496
I 58
30.9
29.0
29.7
29.1
29.68
48.3
9-3895
9-4327
0.3848
— 0.96
5-90
6
508
I 59
16.5
15.O
14.7
13-5
14.92
48.3
8.8214
8.8646
0.1833
+ 0.46
7-32
7
493
2 4
14.0
il.6
14.0
xx -3
12.72
47.2
8.6855
8.7256
0.3223
+ 0.81
7.67
3
461
2 6
29.9
26.4
30.5
29.6
29.10
5 1 - 1
9-3739
9.4256
0.3777
— 0.94
5.92
0
581
2 8
21.0
18.5
19.0
20.5
1 9-7 5
53-9
9.0576
9.H97
0.0718
— 0.18
6.68
1
597
2 IO
13-3
12.0
12.0
11.0
1 2.08
52.7
8.6415
8.6990
0.3489
+ 0.87
7-73
8
385
2 12
26.8
24.4
26.5
23-9
2540
43-4
9.2648
9.2958
9
472
2 15
154
I3.O
x 4-5
13-1
14.00
45-8
8.7674
8.8039
5
495
2 16
15.0
I3-I
15.0
14.0
14.28
48.8
8.7842
8.8288
0.2 191
4- 0.55
7.41
5
502
2 18
24.8
25.2
24.1
26.5
25-15
48.6
9.2568
9.3008
0.2529
— 0.63
6.23
5
511
2 19
19.0
18.O
19.9
19-5
19.10
48.5
9.0297
9-0734
0.0255
— 0.06
6.80
8
528
2 20
26.5
25-7
25-5
26.4
26.02
45-5
9.2843
9.3201
0.2722
— 0.68
6.18
9
447
2 22
17.2
16.4
16.0
14.8
16.10
44.1
8.8859
8.9184
0.1295
4- 0.32
7.18
2
552
2 23
20.6
20.0
22.1
19-5
20.55
5 x -°
9.0907
9.142 1
0.0942
— 0.24
6.6 2
8
385
2 25
26.5
26.5
23.O
24.6
25-15
43-3
9.2568
9.2876
9
472
2 27
16.5
15-4
14-5
x 3-5
14.98
44.9
8.8249
8.8593
Mittel aus den Vergleichsternbeobachtungen: 9.0204; 9.0499; 9.0734. Zur Reduction benutzt: 9.0479.
Zone 369.
1889 November 24.
Beobachter: Kempf.
Photometer:
Clt. Vergleichsterne: Nr. 7 und Nr.
9. Luft :
2.
8°
455
2 ii 2 6 ra
i8?4
1584
1885
1488
CO
0 •
sO
4483
8.9209
8-9539
8
652
2 30
13-5
12.0
15.6
14-3
X 3-85
47-7
8.7582
8.7997
18
243
2 33
26.0
21.4
23.0
25-5
23.98
34-8
9.2179
9-2345
0.3548
— 0.89
4.11
2
317
2 35
26.0
21.6
25-9
20.0
23-38
50.8
9.1972
9.2479
0.3682
— 0.92
4.08
2
422
2 37
30-3
24.0
24.7
22.1
25.28
49.6
9.2610
9.3080
0.4283
— 1.07
3-93
3
419
2 40
39 -o
44.0
46.9
37 -o
41.72
48.8
9.6462
9.6908
O.81 11
— 2.03
2.97
8
455
2 42
16.3
14.4
16.2
14.0
15.22
44.0
8.8383
8.8706
8
652
2 45
14.0
12.5
14.9
12.9
I 3-58
46-5
8.7414
8.7797
8
5 11
2 47
30.8
27-5
25-5
25-5
27.32
44-3
9.3236
9-3566
O.4769
— 1.19
3 - 8 i
15
612
2 49
28.4
25.6
27.0
23.2
26.05
40-5
9-2853
9.3106
O.4309
— 1.08
3-92
*) x 5
612
2 51
22.8
20.6
22.1
20.9
21.60
40.4
9 - x 32 o
9- 1 5 7 1
O.2774
— 0.69
3-89
17
712
2 55
25.0
21.0
24-5
26.0
24.12
38.6
9.2227
9.2448
O.3651
— 0.91
4.09
18
640
2 57
31.6
29.8
28.3
25.0
28.68
37-3
9.3623
9-3823
O.5026
— 1.26
3-74
8
455
2 59
17.9
17.4
18.0
14.6
16.98
43-9
8.9309
8.9630
8
652
3 i
16.0
16.0
17.0
14.6
15.90
45-5
8.8754
8.9112
Mittel aus den Vergleichsternbeobachtungen: 8.8768; 8.8252; 8.9371. Zur Reduction benutzt: 8.8797.
*) Mit Blende 3 beobachtet.
