334
Müller und Kempf, Photometrische Durchmusterung
334
B.D.
Stern zeit
1
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grosse
Zone 524. 1891 October 9
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 38
und Nr. 40. Luft:
2.
io°
3573
20'
5 2 m
2484
22? 6
2486
2385
23878
5085
9.2111
9.2609
IO
3981
20
54
25-5
22.4
24.4
23.2
23.88
44-7
9.2145
9.2484
12
3818
20
56
17.4
15.0
17.9
15.6
16.48
46.2
8.9057
8.9432
0.3041
+ 0.76
7.60
I I
3749
20
58
27.4
20.8
26.O
24.1
24.58
47.2
9.2381
9.2782
0.0309
— 0.08
6.76
IO
3801
20
59
22.9
18.6
21-5
19.4
20.60
48.3
9.0927
9-1359
0.1114
+ 0.28
7.12
19 3956
2 I
1
33-6
31-4
35 -o
34-5
33-62
38-9
9.4865
9.5090
0.2617
— 0.65
6.19
*9
3959
2 I
3
23.0
18.4
21.2
18,5
20.28
39-7
9.0797
9.1036
0.1437
+ 0.36
7.20
18
4014
2 I
4
21-5
18.4
21.7
19.6
20.30
40.1
9.0805
9-1051
0.1422
+ 0.36
7.20
18
4011
2 I
6
29.0
25.2
28.9
304
28.38
40.8
9-3539
9-3797
O.1324
— 0.33
6.51
19
3975
21
8
23-4
22.0
24.9
22.6
23.22
39-7
9.1916
9-2155
O.0318
+ 0.08
6.92
IO
3573
2 I
10
26.8
23.0
26.2
23.1
24.78
52.6
9.2447
9 - 3 °i 8
IO
3981
2 I
11
25.0
21.0
22.5
21.6
22.52
46.1
9.1664
9.2037
16
3809
2 I
13
17.6
154
18.8
15.6
16.85
42.8
8.9244
8.9541
O.2932
+ 0.73
7-57
16 3812
2 I
15
20.9
18.9
20.5
18.7
1 9-75
43-2
9.0576
9.0881
O.1592
4~ 0.40
7.24
15 3762
21
16
14.6
12.5
14.4
i 3-9
13-85
44.1
8.7582
8.7907
O.4566
+ 1.14
7.98
15
3747
2 I
18
19.2
16.5
20.0
17-3
18.25
44.2
8 - 99 1 5
9.0243
O.2230
+ 0.56
7.40
14 3846
2 I
20
45-6
41.9
454
43 -o
43-98
45-5
9.6832
9.7190
°- 47 1 7
— 1.18
5.66
13
3981
2 I
21
1 7-7
14.6
17.0
15-5
16.20
46.0
8.8912
8.9282
0.319 1
—1~ 0.80
7.64
11
3801
2 I
24
18.2
134
16.4
H -9
I 5-72
48.2
8.8658
8.9087
0.3386
-j- 0.85
7.69
IO
3573
21
26
27.6
22.5
24.0
24.0
24-52
54-6
9.2362
9.3912
IO
3981
2 I
28
24.9
20.0
2 i -5
19.4
2 i -45
47-7
9.1263
9.1678
Mittel aus den Vergleichsternbeobachtungen: 9.2547; 9.2527; 9.2345.
Zur Reduction benutzt: 9.2473.
Zone 525. 1891 October g
Beobachter: Kempf.
Photometer:
D. Vergleichsterne: Nr. 2
und Nr. 4.
Luft: 1—
-2.
9 °
47
22“
45 m
34°2
2 896
3280
3186
3 i?6o
4782
9-4386
9.4787
10
168
22
48
24-5
22.5
23-5
23.0
23-38
51.0
9.1972
9.2486
14
76
22
5i
36.5
34 -i
35-7
33-7
35 -oo
42.7
9 - 5 I 72
9-5467
0.201 1
— 0.50
6.19
IO
65
22
54
22.8
18.8
20.5
19.6
20.42
46.1
9.0854
9.1227
O.2229
+ 0.56
7-25
IO
70
22
55
16.7
14.6
16.7
14.8
i 5 - 7 o
46.0
8.8647
8.9017
0-4439
—j— 1.11
7.80
I 2
87
22
58
19.6
16.4
18.5
16.5
17-75
44.8
8.9682
9.0023
0-3433
+ 0.86
7-55
I I
106
23
0
24-5
22.4
23.0
20.0
22.48
45-4
9.iöso
9.2006
0.1450
+ 0.36
7-05
I 2
104
23
2
16.0
14-3
18.0
14.6
I 5-72
44-5
8.8658
8.8992
O.4464
4- 1.12
7.81
9
47
23
4
34-5
31.6
34-5
32.0
33-15
45-7
9-4757
9 - 5 12 o
IO
168
23
7
22.5
22.1
22.9
20.5
22.00
48.9
9 -H 72
9.1921
15
106
23
9
28.1
26.9
27.0
25.0
26.75
40.2
9.3066
9.3314
O.O142
4- 0.04
6-73
18
IOI
23
10
32.4
314
31-5
28.6
30.98
37-9
9.4232
9.4441
0.0985
— 0.25
6.44
18
103
23
12
16.1
13.6
16.5
13.6
14-95
38.3
8.8232
8.8448
0.5008
+ 1.25
7-94
17
105
23
13
16.0
14.4
17.9
144
15.68
38.5
8.8636
8.8855
0.4601
+ 1 • 1 5
7.84
17
106
23
14
1 3*5
12.5
14.4
12.5
13.22
38.9
8.7185
8.7410
0.6046
4 - 1.51
8.20
14
117
23
16
24.1
22.7
23-5
21.4
22.92
41.9
9.1-809
9.2088
O.1368
+ 0.34
7.03
9
47
23
18
324
32.2
31-5
28.3
31.10
44.8
9.4262
9.4603
IO
168
23
19
21-5
22.5
21.8
21.5
21.82
47.6
9.1404
9.1816
Mittel aus den Vergleichsternbeobachtungen: 9.3637; 9.3520; 9.3210.
Zur Reduction benutzt: 9.3456.
Zone 526. 1891 October g
#
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 1-
—2.
io°4Ö04
23
l 25 n >
3182
2784
2982
2586
2 8? 35
4784
9-3531
9-3938
9
5 111
23
28
26.1
234
23-5
23.2
24.05
43-4
9.2203
9-25I3
6
4919
23
30
30.0
2 7-5
29.6
25-5
28.15
50.5
9-3475
9-3973
0.0967
— 0.24
6.30
1
4560
23
32
17.4
16.5
17.7
16.0
16.90
54-9
8.9269
8.9932
0.3074
4-0.77
7-3i
3
4640
23
35
18.4
16.7
1 7-5
17.2
17-45
53-2
8-9539
9 -oi 33
0.2873
4- 0.72
7.26
3
4644
23
36
17.7
17.8
20.0
194
18.72
53-5
9.0129
9.0734
O.2272
+ 0.57
7.n
23
39
18.7
14.0
194
154
16.88
51.8
8.9259
8.9801
0.3205
4- 0.80
7-34
^ 1
23
40
14.4
13.0
13-3
10.7
12.85
5 i -9
8.6943
8.7488
0.5518
+ 1.38
7.92