298
Müller und Kempf, Photometrische Durchmusterung
298
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
9 °
1064
6 h 29 111
4286
3983
4084
4I?2
40888
4383
9.6318
9.6626
i
1105
6 32
28.0
29.0
28.6
30.1
28.92
52.3
9.3689
9.4249
0.1420
+ 0.36
5.01
13
979
6 34
2 3-7
22.8
23-5
22.5
23.12
39-9
9.1880
9.2122
o -3547
+ 0.89
5-54
6
1027
6 38
23.6
23-5
23.6
25.0
23.92
47-4
9.2159
9.2566
0.3103
+ 0.78
5-43
12
912
6 41
28.7
29.1
29-5
29.9
29.30
4 T -5
9-3793
9.4064
0.1605
4- 0.40
5-05
H
1041
6 48
21.6
20.5
24.0
22.5
22.15
40.2
9 - i 5 2 8
9.1776
0.3893
+ 0.97
5.62
1
11 5 1
6 50
28.6
31-5
29-3
31-4
30.20
52.3
9.4032
9.4592
0.1077
+ 0.27
4.92
9
683
6 52
29.4
28.4
29.6
32.2
29.90
49. 1
9-3953
9.4408
9
1064
6 55
38.5
36-5
36.5
39-8
37.82
44.4
9-575 2
9.6084
Mittel axis den Vergleichsternbeobachtungen: 9.5952; 9.5810; 9.5246.
Zur Reduction benutzt: 9.5669.
Zone 433
. 1891 Februar 25.
Beobachter: Müller.
Photometer :
Ci. Vergleichsterne: Nr. n und Nr.
13. Luft:
3 -
9 °
683
22 m
3084
2 8°5
3182
3 2°6
30868
4289
9.4156
9-4455
9
1064
5 25
40.9
36.5
35-7
38.O
37-78
43-2
9-5744
9.6049
1
872
5 27
32.5
33 -o
31-9
33-3
32.68
51-3
9.4647
9 - 5 i 7 i
O.OO71
4- 0.02
4.67
15
732
5 29
30.8
29.9
29.7
30.6
30.25
37-6
9.4045
9.4250
O.O992
4- 0.25
4.90
18
779
5 31
27.1
25.6
2 6.8
26.2
26.42
34-4
9.2966
9-3127
0 . 2 II 5
+ 0.53
5.18
8
866
5 34
20.5
20.9
20.8
2 I .O
20.80
44-5
9.1007
9 -i 34 i
O.39OI
4- 0.98
5-63
15
752
5 36
25-9
24.1
26.0
2 5-7
25.42
37-5
9.2654
9.2857
O.2385
4- 0.60
5-25
15
759
5 38
23.0
24.0
24.7
25.3
24.25
37 - 1
9.2271
9.2468
O.2774
4- 0.69
5-34
9
683
5 40
30.0
31-3
28.4
31.6
30.32
43-6
9.4063
9-4377
9
1064
5 41
38.3
36.4
39 -°
44-3
39-50
42.9
9.6070
9.6369
2
888
5 44
30-3
29.8
28.9
28.3
29.32
50.3
9-3798
9.4289
O.O953
4- 0.24
4.89
*) 3
871
5 47
24.0
24.1
23-9
24.4
24.10
49.4
9.2220
9.2684
O.2558
4- 0.64
5-29
17
920
5 51
23-3
26.0
25.1
24.8
24.80
35-7
9-2454
9.2632
0 . 2 ÓI 0
4- 0.65
5-30
i
1005
5 53
25.0
23-3
24.9
27.4
25-15
51.2
9.2568
9.3089
O.2153
+ 0.54
5-19
2
962
5 58
26.4
30.6
25.1
2 9 - 7 '
27-95
50.0
9.3418
9.3900
O.1342
4- 0.34
4.99
5
939
6 1
37 -o
37 -i
34 -o
37-5
36.40
47. 1
9-5467
9.5866
O.0624
— 0.16
4.49
9
683
6 3
27.4
27.4
29.4
31.0
28.80
45 -o
9-3657
9.4003
9
1064
6 6
35 -i
40.6
40.3
38.4
38.60
42.8
9.5902
9.6199
Mittel aus den Vergleichsternbeobachtungen: 9.5252; 9.5373; 9.5101. Zur Reduction benutzt: 9.5242.
*) 3^871. Messung schwierig, weil der sehr nahe stehende Stern B.D. + 30872 stört.
Zone 434
. 1891 Februar 25.
Beobachter : Kempf.
Photometer:
Ci. Vergleichsterne: Nr. 13 und Nr. 15. Luft:
3.
9 °
1064
6ii 2 i m
39?6
3885
4282
4085
40820
438 i
9.6197
9.6500
11
1428
6 25
23-5
22.4
24.6
26.5
24.25
41.8
9.2271
9.2548
0
1239
6 27
24-5
23.6
22.9
23-7
23.68
52.4
9.2076
9.2640
O.1873
4- 0.47
5-25
19
1 186
6 29
24.4
26.1
25-5
25.1
25.28
33-3
9.2610
9-2758
0.1755
4- 0.44
5.22
14
1152
6 31
34-4
32.5
32.6
35-5
33-75
38.1
9.4895
9.5108
O.O595
— 0.15
4-63
14
1187
6 33
32.6
33-1
39-5
32.7
34-48
38.6
9-5058
9-5279
O.O766
— 0.19
4-59
16
io 35
6 35
26.5
24.4
26.9
28.4
26.55
36.7
9.3006
9.3198
O.I 3 I 5
+ 0.33
5 - 1 1
16
1060
6 37
21.2
22.4
21.9
25.0
22.62
36.6
9.1700
9.1890
O.2623
4- 0.66
5-44
9
1064
6 39
39 -o
39-2
36.6
4°-4
38.80
43-7
9.5940
9.6256
11
1428
6 41
25-5
24.6
25.0
25.0
25.02
41.4
9-2525
9-2795
H
1247
6 44
20.6
20.1
21.4
20.0
20.52
38.2
9.0895
9.1109
0.3404
4- 0.85
5-63
4
1236
6 47
31-5
30.0
32.5
36.4
32.60
48.2
9.4628
9-5057
O.O544
— 0.14
4.64
0
1426
6 49
23.2
22.7
21.6
26.4
23.48
52.3
9.2007
9.2567
O.I946
4- 0.49
5-27
11
1209
6 51
23.0
23.0
23-5
22.4
22.98
41.1
9-1831
9.2095
O.2418
4- 0.60
5-38
7
1 3 37
6 53
30.6
27.7
28.0
32.0
29.58
45-3
9.3869
9.4222
O.O29I
4- 0.07
4-85
9
1064
6 57
37-7
41.4
40.7
37-6
39-35
44.6
9.6043
9.6380
11
1428
6 59
24.2
23-5
24.7
25-3
24.42
41-3
9.2328
9.2596
Mittel aus den Vergleichsternbeobachtungen: 9.4524; 9.4526; 9.4488.
Zur Reduction benutzt: 9.4513.
