248
Müller und Kempf, Photometrische Durchmusterung
248
B.D.
Sternzeit
I
II
III
IV
J
£
log sin 2 »/
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
i 5 °
1087
41.35m
i8?o
1580
I 7?2
17?o
16880
4085
8.9219
8.9472
0.5404
+ i -35
7-44
13
1147
4 37
20.1
16.6
17.2
17.2
17.78
42.4
8.9696
8.9985
0.4891
+ 1.22
7 - 3 i
13
1 1 5 I
4 38
3 i -5
274
2 6.0
2 6.8
27.92
42.4
9.3410
9.3699
0.1177
+ 0.29
6.38
i 9
1253
4 40
31-4
3 i -9
3 i -7
324
31-85
36.5
9.4448
9-4637
0.0239
+ 0.06
6.15
18
1112
4 42
22.5
20.9
23-3
234
22.52
37-8
9.1664
9.1872
0.3004
+ 0.75
6.84
1 7
1154
4 43
14.1
13.0
14.0
13.0
13-52
38.5
8.7377
8.7596
0.7280
-j- 1.82
7.91
IO
818
4 45
384
33-8
32.5
3 i -5
34-05
43 -i
9-4963
9.5266
IO
1149
4 47
374
29.0
30-5
30.6
31.88
46.1
9-4455
9.4828
Mittel aus den Vergleichsternbeobachtunge
n: 9 - 4343 ; 9 - 5238 ; 9 - 5047 -
Zur Reduction benutzt: 9.4876
Zone 308. 1889 Januar 5.
Beobachter: Müller.
Photometer: D. Vergleichster.ie: Nr. 8 und Nr. io.
Luft: I-
-2.
9 °
472
2 h 5 l m
20?9
i 8?5
I 9?7
1984
19862
4387
9.0521
9.0837
I I
632
2 53
26.7
25.0
2 5-7
22.9
25.08
45-6
9-2545
9.2905
I
667
2 57
274
24.6
26.4
24.0
25.60
52.2
9.2711
9.3267
O.1906
— 0.48
6-77
I
673
2 59
23.8
22.2
24.0
21.5
22.88
51.6
9-1795
9.2330
O.O969
— 0.24
7.01
6
594
3 2
384
38.0
40.0
35-2
37-90
47.1
9-5767
9.6166
O.4805
— 1.20
6.05
7
560
3 4
17.1
16.0
16.9
15.6
16.40
45-7
8.9015
8.9378
O.I983
+ 0.50
7-75
8
596
3 6
18.2
15-1
16.6
16.7
16.65
44.4
8.9144
8.9476
O.1885
+ 0.47
7.72
i
679
3 9
24.2
21.1
22.5
21.8
22.40
5 i -3
9.1620
9.2144
O.O783
— 0.20
7-05
9
472
3 12
19.1
1 5 - 1
17.1
16.9
17-05
43 -o
8-9344
8.9645
11
632
3 17
244
22.0
2 54
25.6
24-35
43-7
9-2305
9.262 1
2
628
3 22
21.4
18.9
21.1
18.8
20.05
50.1
9.0702
9.1187
0.0174
+ 0.04
7.29
5
564
3 24
30.0
30.0
28.0
2 8.8
29.20
47.0
9-3766
9.4162
0.2801
— 0.70
6-55
i
685
3 26
16.7
14.9
16.0
15.0
15-65
51.6
8.8620
8.9155
0.2206
+ o -55
7.80
9
524
3 29
28.0
24.6
274
26.2
26.55
42.7
9.3006
9 - 33 oi
0.1940
— 0.49
6.76
9
532
3 32
26.0
22.7
26.7
21.3
24.18
43 -i
9.2247
9.2550
0.1189
— 0.30
6-95
8
625
3 35
27.6
244
25.1
24.6
25.42
44.0
9.2654
9.2977
0.1616
— 0.40
6.85
5
584
3 38
444
464
43-3
44.2
44-58
47-5
9.6926
9-7335
0.5974
— 1.49
5-76
9
472
3 40
19.6
18.0
174
1 7.0
18.00
42.7
8.9800
9.0095
11
632
3 43
24.8
21.8
22.8
21.9
22.82
42.3
9-1773
9.2060
Mittel aus den Vergleichsternbeobachtungen: 9.1871
; 9.1133; 9.1078. Zur Reduction benutzt: 9.1361
Zone 309. 188g Januar 5.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 12 und Nr. 14
Luft: 1-
—2.
IO°
818
3 h 52 m
04
• O
CO
3785
3883
3783
37872
4685
9-5732
9 - 6 ii 5
IO
1149
3 55
31-9
28.3
32.6
27.7
30.12
5 i -4
9.4011
9-4539
19
I 106
3 59
18.5
15-2
18.6
17.9
17-55
38.8
8.9587
8.9811
0.5465
+ i -37
7.46
19
I I IO
4 0
32.9
29.0
32-5
31-5
31.48
38.5
9-4357
9-4576
0.0700
+ 0.18
6.27
19
II13
4 2
15.8
14-3
15-5
Ho
15.02
38.4
8.8271
8.8488
O.6788
+ 1-70
7-79
19
11 26
4 3
33-6
304
30.8
31.2
31-50
38.5
9.4362
9.4581
O.0695
+ 0.17
6.26
14
1074
4 6
24.6
22.0
23-3
21.3
22.80
43-3
9.1766
9.2074
O.3202
-j— 0.80
6.89
H
1060
4 8
39 -i
35-2
37-2
37-5
37-25
43 -o
9-5639
9.5940
O.0664
— 0.17
5-9 2
IO
818
412
37-8
38.7
38.7
39-6
38.70
45 -o
9.5921
9.6267
IO
1149
4 14
32.0
27.6
31.0
29-3
29.98
49-3
9-3974
9-4435
11
964
4 17
24-3
20.6
24.6
24.9
23.60
44-5
9.2049
9-2383
O.2893
4- 0.72
6.81
11
960
4 19
21.2
17.0
18.9
18.0
18.78
4 - 1-3
9 -oi 55
9.0485
0.4791
-h 1.20
7.29
I 2
937
4 21
15-3
15-2
144
134
14.58
43-6
8.8018
8.8332
O.6944
4 - i -74
7-83
IO
927
4 24
32.6
28.5
30.7
28.8
30.15
45 -i
9.4019
9-4367
O.0909
4- 0.23
6.32
13
1036
4 27
26.6
24.8
27.6
25.8
26.20
41.9
9.2899
9.3178
O.2098
4- 0.52
6.61
l6
926
4 28
17.0
16.3
18.9
16.5
17.18
39-4
8.9407
8.9641
0.5635
4 - 1.41
7-50
IO
818
4 32
4 i -3
37 -2
35-7
40.0
38.55
43-7
9-5893
9.6209
IO
1149
4 34
29.8
28.5
28.8
28.5
28.90
47-3
9.3684
9.4088
Mittel aus den Vergleichsternbeobachtungen
: 9 - 53 2 7 ; 9 - 5351 ; 9 - 5 r 49 - Zur Reduction benutzt: 9.5276.
