244
Müller und Kempf, Photometrische Durchmusterung
244
13 .D.
Sternzeit
I
11
III
IV
J
z
log sin 2 «/
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
9 °
472
3 h 7 m
i 4?8
i6?8
17?o
1586
16805
438 i
8.8833
8.9136
5
443
3 n
19.6
16.7
18.7
1 7.0
18.00
46.7
8.9800
9.0188
0.1515
+ 0.38
7.24
1
534
3 13
27.0
27.4
29.4
26.7
27.62
51.0
9-3323
9-3837
0.2134
— 0.53
6-33
9
397
3 15
12.6
10.0
12.5
11.1
ii -55
43 -o
8.6030
8.6331
0.5372
+ 1-34
8.20
9
408
3 17
20.7
18.3
19.4
17.0
18.85
42.9
9.0187
9.0486
0.12 I 7
+ O.30
7.16
7
478
3 20
26.2
26.3
26.3
22.7
25-38
44-5
9.2642
9.2976
0.1273
— O.32
6-54
1
561
3 22
19.6
16.6
19.2
19.0
18.60
50.6
9.0075
9.0576
0.1127
+• 0.28
7.14
8
385
3 24
31-5
30.0
31-4
27-5
30.10
45 -o
9.4006
9-4352
9
472
3 27
17.1
15.6
17.0
15.0
16.18
42.7
8.8901
8.9196
Mittel aus den Vergleichsternbeobachtungen: 9.2044; 9.1292; 9.1774. Zur Keduction benutzt: 9.1703.
Wolkenstreifen in der Nähe des Vergleichsterns Nr. 6.
Zone 298.
1888 December 20.
Beobachter:
Kempf.
Photometer:
D. Vergleichsterne: Nr. 6
und Nr. 8. Luft: 3.
8°
385
i h 54 m
3 189
3080
3 l 8 o
33°4
31858
4387
9.4381
9.4697
9
472
i 57
20.3
16.4
18.8
17.4
18.22
47.2
8.9901
9.0302
18
507
i 59
17.6
15.6
18.5
16.6
1 7.08
38.1
8-9358
8-9571
0.3244
H- 0.81
7.67
18
517
2 1
17-5
14-5
18.O
16.0
16.50
37-8
8.9067
8.9275
0.3540
+ 0.89
7-75
19
562
2 2
19-5
16.4
18.3
18.8
18.25
36.9
8.9915
9.0110
0.2705
+ 0.68
7-54
14
586
2 4
28.5
29.0
26.4
28.0
27.98
41.2
9.3426
9.3692
0.0877
— 0.22
6.64
13
579
2 5
23.6
22.5
25-5
250
24.28
42.6
9.2281
9-2574
0.0241
+ 0.06
6.92
16
484
2 7
32.5
28.0
30.6
31-5
30-65
40.0
9.4148
9.4392
0.1577
— 0.39
6.47
9
472
2 8
22.0
19.6
2 1 .0
19.6
20-55
46.3
9.0907
9.1285
8
385
2 11
33-9
32.9
33-7
37 - 6
34-52
43-4
9.5067
9-5377
16
497
2 14
21.4
18.0
20.6
20.4
20.10
39 -o
9.0723
9.0950
0.1865
+ 0.47
7-33
19
582
2 16
32.6
31-5
32.0
30.9
31-75
36.6
9-4423
9.4613
0.1798
— 0.45
6.41
10
479
2 18
17.0
15.0
17.0
16.0
16.25
45-3
8.8938
8.9291
0.3524
+ 0.88
7-74
13
594
2 19
23.6
19.6
21.5
21.5
21-55
42.4
9-1301
9.1590
0.1225
+ 0.31
7-17
12
5i6
2 21
29-5
26.6
29.0
29.0
28.52
43 -i
9-3579
9.3882
0.1067
— 0.27
6-59
*3
613
2 23
15-5
14.0
14-5
12.5
14.1 2
41.9
8.7746
8.8025
0.4790
+ 1.20
8.06
8
385
2 25
3Ó.8
31.6
32.8
33-6
33 - 7 °
43-3
9.4883
9 - 5 i 9 i
9
472
2 27
20.6
15-5
18.9
16.1
17.78
44.9
8.9696
9.0040
Mittel aus den Vergleichsternbeobachtungen: 9.2500; 9.3331; 9.2615. Zur Keduction benutzt: 9.2815.
Zone
299.
1888 December 30.
Beobachter:
Müller.
Photometer:
D. Vergleichsterne: Nr. 8
und Nr. 10. Luft: 3.
9 °
472
2“ 32™
16? 7
1489
i 7 ?7
1780
16858
4486
8.9108
8.9445
11
632
2 34
22.7
19-5
23-3
22.1
2 1.90
47-3
9-1434
9.1838
*) 0
616
2 36
29.4
26.4
28.0
31-4
28.80
53-4
9-3657
9.4258
0.3449
— 0.86
6-39
3
503
2 38
16.7
14.2
17.2
15-7
15-95
49.9
8.8781
8.9260
0.1549
+ 0.39
7.64
8
542
2 39
13-5
12.1
13-9
11-5
12-75
45 -o
8.6876
8.7222
0.3587
+ 0.90
8.15
4
571
2 41
23.0
I9.O
21.8
20.6
21.10
48.9
9.1126
9-1575
0.0766
— 0.19
7.06
8
553
2 42
17.4
15-9
18.9
17.2
17-35
45-5
8.9491
8.9849
0.0960
+ 0.24
7-49
2
602
2 43
22.0
20.4
21.7
18.0
20.52
51-4
9.0895
9.1423
0.0614
— 0.15
7.10
9
472
2 45
18.0
17.4
17.0
17.6
17-50
43-9
8.9563
8.9884
11
632
2 47
21.3
21.1
21-5
20.0
20.98
46.1
9.1079
9.1452
6
582
2 50
17-3
16.9
16.9
17-3
17.10
46.6
8.9368
8-9754
0.1055
-f- 0.26
7-51
6
583
2 51
35-2
34 -o
33-4
32.0
33-65
47.0
9.4872
9.5268
0.4459
— 1.11
6.14
6
590
2 53
14-3
13.2
13-3
12.3
13.28
47-3
8.7223
8.7627
0.3182
+ 0.80
8.05
8
567
2 55
17.6
17.0
18.1
18.9
17.90
44.8
8-9753
9.0094
0.0715
+ 0.18
7-43
9
494
2 56
23-7
21.4
24.8
23-5
23-35
44.1
9.1962
9.2287
0.1478
— 0.37
6.88
8
574
2 58
22.5
21.2
21.6
20.4
21.42
44-3
9-1251
9.1581
0.0772
— 0.19
7.06
9
472
3 0
16.8
16.5
18.6
16.8
17.18
43-3
8.9407
8-9715
11
632
3 2
24.6
23.0
24.4
23-9
23.98
44.8
9.2179
9.2520
Mittel aus den Vergleichsternbeobachtungen: 9.0642; 9.0668; 9.1117. Zur Keduction benutzt: 9.0809.
*) o°6i6 dupl. Gemessen die folgende, hellere Componente.
