332
Müller und Kempf, Photometrische Durchmusterung
332
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 51g. 1891 October i.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 40
und Nr. 42. Luft:
2.
io°3g8i
2 I L
3 m
2488
24?4
2 5?o
23-5
24842
45”5
9.2328
9.2686
io 4351
2 I
6
34-4
27.0
27.8
26.9
29.02
42.0
9-3717
9.3998
0 4265
2 I
9
20.4
16.4
20.2
17.6
18.65
56.0
9.0098
9.0809
0.2410
+ O.60
7.40
2 3932
21
I I
29-5
24.7
26.9
27.8
27.22
53-9
9.3206
9.3827
0.0608
— O.15
6.65
3 4065
21
13
23-5
18.6
2 1.6
20.0
20.92
53-5
9-1055
9.1660
0.1559
+ O.39
7.19
3 4097
21
15
28.6
24-3
25-3
27.0
26.30
53-6
9.2929
9-3538
0.0319
— 0.08
6.72
4 4210
2 I
17
14.7
13.2
15.6
15-9
14.85
51.8
8.8175
8.8717
0.4502
+ I.I 3
7-93
5 4209
2 I
19
26.0
23.0
20.8
25-5
25-32
51.6
9.2622
9 - 3 I 57
0.0062
4" 0.02
6.82
10 3981
2 I
21
24-3
21.0
25.O
24.0
23-58
47.1
9.2042
9.2441
10 4351
21
22
29.9
24.4
30.0
29.0
28.32
42.6
9-3523
9.3816
5 4190
2 I
25
31.0
27-3
29.4
29.1
29.20
53 -o
9.3766
9-4352
0.1133
0.28
6.52
7 4130
21
27
17-3
13.6
16.0
14.5
15-35
50.9
8.8456
8.8967
0.4252
+ I.06
7.86
7 4133
2 I
28
20.5
18.4
21.5
18.7
19.78
51.0
9.0589
9 -i i °3
0.2 I 16
+ 0.53
7-33
7 4175
2 I
30
19.8
17.4
19-5
18.5
18.80
50.8
9.0164
9.0672
0.2547
4 - 0.64
7-44
8 4190
2 I
31
24.4
19-5
22.0
20.4
21.58
50.0
9-1312
9.1794
0.1425
4~ O.36
7.16
9 4233
2 I
34
29-5
24.0
27.4
25.6
26.62
49.1
9.3027
9.3482
0.0263
— 0.07
6-73
10 3981
2 I
36
25.0
20.5
25.0
21.5
23.00
48.5
9.1838
9-2275
10 4351
21
38
32.8
24.7
30.8
2 8.8
29.28
43-5
9.3788
9.4100
Mittel aus den Vergleichsternbeobachtunge
n: 9-3342; 9-3J29; 9-3!87-
Zur Reduction benutzt: 9.3219.
Zone 520. 1891 October 6.
Beobachter: Kempf.
Photometer :
Dil. Vergleichsterne: Nr. 39 und Nr.
41. Luft
1.
io °3787
2 0*
9 ™
i 6°5
i6?o
I3?6
i 4 ?6
15-18
4386
8.8361
8.8675
8 4261
20
11
17.4
17-5
15-5
17-5
16.98
44.4
8.9309
8.9641
9 3564
20
15
27-5
27.0
27-5
28.0
27-50
50.6
9.3288
9-3789
O.4541
— I.14
3-94
14 3736
20
18
23-5
24.4
244
24.2
24.12
41.0
9.2227
9.2489
O.3241
— O.81
4.27
13 3899
20
20
36.5
37-5
38.9
41.7
38.65
41.9
9.5912
9.6191
O.6943
— 1.74
3-34
*)i3 3899
20
22
28.6
27.9
30.0
304
29.22
42.0
9-3771
9.4052
0.4804
1.20
3-46
2 3879
20
24
29.2
29-3
31.8
29-5
29-95
51.2
9.3966
9.4487
0-5239
— 1-31
3-77
*)io 4043
20
28
37-5
34 -i
32.5
33 -i
34-30
43 -i
9.5018
9-5321
0.6073
— I.52
3-14
10 3787
20
29
16.0
16.4
15-1
15-5
15-75
45 -i
8.8674
8.9022
8 4261
20
31
17-3
15.0
16.5
16.2
16.25
45 -i
8.8938
8.9286
19 4229
20
33
31.2
28.0
29-3
30.0
29.62
34 -o
9-3879
9-4035
0.4787
1.20
3.88
10 4321
20
35
22.7
21.4
22.2
22.4
22.18
41-5
9-1539
9.1810
O.2562
O.64
4.44
14 4369
20
38
27-5
26.0
26.0
26.5
26.50
38.2
9.2991
9-3205
0-3957
— O.99
4.09
*)i 4 4369
20
39
22.4
21.6
24.0
23.1
22.78
38.2
9-1759
9-1973
O.2725
— 0.68
3-98
15 4222
20
41
26.5
25.2
24.9
254
25-50
36.8
9.2680
9.2873
O.3625
— 0.91
4.17
15 4255
20
43
25-4
23.6
24.4
26.6
25.00
36.7
9.2519
9.27 11
0-3463
— 0.87
4.21
10 3787
20
45
16.0
16.4
15.6
16.5
16.12
46.4
8.8870
8.9250
8 4261
20
48
16.9
17-4
16.0
17.1
16.85
45-9
8.9244
8.961 2
Mittel aus den Vergleichsternbeobachtungen: 8.9x58; 8.9154; 8.9431.
Zur Reduction benutzt: 8.9248.
*) Mit Blende 3 beobachtet.
Zone 521. 1891 October 6.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 38 und Nr. 40. Luft: 1
—2.
l °°3573
20 1
53 ra
2483
2 1?5
22? 5
2 2?0
22858
5086
9.1686
9.2 187
IO 3981
20
55
22.7
20.4
20.5
20.1
20.92
44.8
9-1055
9.1396
10 3813
20
58
20.0
19-5
18.5
I9.O
19-25
48.0
9.0362
9.0785
O.1044
4- 0.26
7.10
10 3803
21
0
17.4
14-3
16.7
I4.2
15-65
47-6
8.8620
8.9032
O.2797
+ 0.70
7-54
ii 3752
2 I
2
18.0
15-5
16.5
l6.6
16.63
47-3
8.9144
8.9548
0.2281
+ 0.57
7.41
ii 3775
2 I
3
18.0
17.0
18.5
18.O
17.88
47.2
8.9744
9.OI45
0.1684
4- 0.42
7.26
ii 3778
2 I
5
25-3
21.6
24.4
21-5
23.20
47.0
9.1909
9-2305
O.0476
— 0.12
6.72
10 3839
21
7
16.5
14.6
16.0
14.8
15.48
48.3
8.8527
8.8959
0.2870
4-0.72
7-56
