274
Müller und Kempf, Photometrische Durchmusterung
274
B.D.
Sternzeit
I
II
III
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
i o°
818
5 h 54 m
3287
28?I
2 983
3087
30?20
4285
9.4032
94323
8
1379
5 56
15.8
14.0
I4.8
14.1
14.68
43-9
8.8076
8.8397
0.4873
-f- 1.22
7 - 3 1
9
1259
5 57
18.9
16.2
l8.6
16.7
17.60
43-6
8.9611
8.9925
0-3345
—f— 0.84
6-93
5
1267
5 59
18.2
15.0
I7.4
17.6
17-05
46.8
8.9344
8-9735
0-3535
+ 0.88
6.97
*\ e
6 1
6.8
5 -o
6.7
5 -i
5-90
46.9
8.0239
8.0632
1.2638
+ 3-i6
9-25
) 5
6 2
15.0
14.2
I4.8
14.6
14.65
46.8
8.8059
8.8450
0.4820
+ 1.21
7-30
5
1283
6 5
18.0
16.2
16.4
17.7
17.08
47.6
8-9358
8.9770
0.3500
+ 0.88
6.97
4
1304
6 6
27.4
29.0
29.O
24.2
27.40
47-7
9-3259
9.3674
0.0404
— 0.10
5-99
IO
1149
6 7
24.6
20.7
22.9
24-5
23.18
42.1
9.1902
9.2185
IO
818
6 9
32.8
29-5
28.4
31-1
30.45
43 -o
9.4097
9.4398
Mittel aus den Vergleichsternbeobachtungen: 9.3102; 9.3416; 9.3292. Zur Reduction benutzt: 9.3270.
*) 5 0 1280 dupl. Zuerst die schwächere,
vorangehende Componente gemessen.
Zone
373 -
1889 December 27.
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 14
und Nr. 16. Luft: 2.
IO°
1149
6 h 1 5 m
2884
2Ö?0
2885
2 7 ? i
27850
4280
9.3288
9-3569
11
1588
6 17
23.6
22.0
22.3
21-5
22.35
43-2
9.1602
9.1907
8
1712
6 19
32.0
32.0
31-5
33-6
32.28
45-4
9-4552
9.4908
0.2058
— 0.51
5-96
o
1871
6 2 1
23-7
2 2.0
23.0
23-9
23-15
534
9.1891
9.2493
0.0357
-f- 0.09
6.56
6
1594
6 23
21.4
20.4
20.0
20.8
20.65
46.5
9.0947
9-1330
0.1520
+ 0.38
6.85
7
1684
6 24
29.2
30.0
29.9
29.7
29.70
46.2
9.3900
9-4275
0.1425
— 0.36
6.11
2
1640
6 25
30.7
31.0
29-5
30.1
30-32
50.5
9.4063
9.4561
0.1711
— 0.43
6.04
9
1603
6 27
21.6
I9.O
21.0
18.8
20.10
43-9
9.0723
9.1044
0.1806
+ 0.45
6.92
IO
1149
6 29
27.6
29.7
28.0
30.5
28.95
42.0
/9.3698
9-3979
11
1588
6 31
22.0
25.O
24.7
25.2
24.22
42.4
9.2261
9-2550
o
I 9°9
6 33
20.5
l8.I
19.0
19.0
19 - 1 5
52.5
9.0319
9.0886
0.1964
+ 0.49
6.96
o
1915
6 34
28.5
28.2
274
28.6
28.18
52.7
9-3483
9.4058
0.1208
— 0.30
6.17
o
1916
6 35
23.6
2 1.6
234
234
23.00
52.2
9 .ì 838
9.2394
0.0456
+ 0.1 I
6.58
3
1649
6 37
18.5
16.O
18.0
17.2
17.42
49.2
8-9525
8.9983
0.2867
+ 0.72
7.19
7
1729
6 39
44.2
42.8
41.6
48.5
44.28
46.0
9.6879
9.7249
0.4399
I.IO
5-37
6
1688
6 40
25.8
21-5
21.7
21.0
22.50
464
9-1657
9.2037
0.0813
+ 0.20
6.67
11
1588
6 42
23.1
I9.9
21.5
23.1
21.90
41.9
9-1434
9 - 1 7 13
IO
1149
6 44
29-5
23.O
274
27-5
26.85
42.2
9.3096
9 - 338 i
Mittel aus den Vergleichsternbeobachtungen: 9.2738; 9.3265; 9.2547.
Zur Reduction benutzt: 9.2850
Zone 374. 1890 Januar 8.
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. io und Nr.
12. Luft:
2.
n c
632
3 11 3 ° m
2Ó?0
2 I ?4
2484
2 2?8
23865
4289
9.2066
9-2365
IO
818
3 33
4O.9
35-5
36.8
384
37-90
48.3
9-5767
9.6199
9
860
3 35
1 4 * 7
12.8
15-5
1 3-5
I4.I 2
48.7
8.7746
8.8189
0.6013
+ 1 - 5 °
7-95
i
1058
3 36
24.8
22.4
24.4
25.2
24.2O
56.2
9.2254
9.2974
0.1228
+ 0.31
6.76
3
964
3 38
41.4
40.0
394
43-2
41.00
53-9
9-6339
9.6960
0.2758
— 0.69
5-76
5
958
3 40
23-4
22.3
2 1.6
21.2
22.12
51-9
9 -i 5 i 6
9.2061
0.2141
+ 0.54
6.99
8
IOIÓ
3 41
28.7
29-5
26.5
27.6
28.08
48.9
9-3455
9.3904
0.0298
4- 0.07
6.52
4
989
3 43
13-5
134
13.0
14.5
I3.60
52-7
8.7427
8.8002
0.6200
+ 1-55
8.00
IO
818
3 45
37-5
37-6
40.5
40.0
38.9O
47.1
9-5959
9-6358
11
632
3 47
25.0
22.1
21-5
234
23.OO
42.1
9-ì838
9.2121
7
953
3 49
31-9
32.0
33-2
35-6
33 - 1 8
49.6
9.4764
9-5234
0.1032
— 0.26
6.19
8
1024
3 50
22.6
21.6
22.5
24-5
22.80
48.6
9.1766
9.2206
O.1996
+ 0.50
6-95
o
1152
3 53
31.0
29.0
29.0
30.0
29.75
56.3
9 - 39 I 4
9-4639
0.0437
O.I I
6.34
9
925
3 54
16.6
13-7
15-3
15.0
I 5 -I 5
47-9
8.8344
8.8764
0-5438
+ !- 3 6
7.81
5
973
3 56
20.0
16.8
19.1
17.4
18.32
50.5
8.9947
9.0445
0-3757
+ O.94
7-39
3
1007
3 58
19-5
19.0
20.0
1 7-5
19.00
52.8
9-0253
9.0831
0-3371
+ O.84
7.29
IO
818
4 0
42-5
33-6
34-0
364
36.62
45-9
9-5512
9.5880
11
632
4 2
23.2
2 2.0
24.6
24.2
23-50
41.6
9.2014
9.2287
Mittel aus den Vergleichsternbeobachtungen: 9.4282; 9.4240; 9.4083.
Zur Reduction benutzt: 9.4202
