184
Müller und Kempf, Photometrische Durchmusterung
184
B.D.
I
Sternzeit
I
II
m |
IV
J
1
2
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 147. 1887 April 27.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 22
und Nr. 24. Luft: 2
— 3 -
9° 2 374
I2 h 23 m
3385
3585
3 6?2
3Ö?o
35830
498 o
9.5236
9.5688
ii 2372
12 25
24.2
25.0
25.O
21.4
23.90
42.3
9.2152
9.2439
2 2387
12 26
38.7
43-9
43-5
43-2
42.32
52.8
9.6563
9.7141
0.2938
— 0.73
5-67
3 2475
12 29
19.0
19.9
23.0
21.4
20.82
52-3
9.1015
9-1575
0.2628
+ 0.66
7.06
8 2476
12 31
30.0
33 -o
34-6
31.6
32 - 3 °
46.8
94557
9.4948
0.0745
— 0.19
6.21
2 2411
12 33
32.5
31.6
33-3
34 -o
32.85
52.8
9.4687
94265
0.1062
— 0.27
6.13
7 2440
12 34
20.0
19.7
23-4
20.0
20.78
47-8
9.0999
9 -I 4 I 7
0.2786
+ 0.70
7.10
7 2443
12 36
18.0
18.5
19-5
19.0
18.75
48.0
9.0142
,9-0565
0.3638
+ 0.91
7-31
9 2374
12 37
38.0
34 -o
42.5
38.0
38.12
504
9.5810
9-6305
•
11 2372
12 39
23-4
23-3
22.8
21-5
22.75
43 -i
9.1748
9.2051
9 2482
12 41
19.0
20.1
23.0
2 1.0
20.78
46.0
9.0999
9.1369
0.2834
+ 0.71
7.11
0 2782
12 43
29.8
29.2
34-4
324
3145
54-7
94350
9.5004
0.0801
— 0.20
6.20
2 2418
12 44
38.0
40.4
43-6
40.1
40.52
53-5
9.6255
9.6860
0.2657
— 0.66
5-74
4 2461
12 46
17.0
17.2
21.5
20.5
19.05
51-7
9.0275
9.0813
0.3390
+ 0.85
7.25
4 2463
12 47
21.5
22.9
26.0
24.O
23.60
51-2
9.2049
9.2570
0.1633
+ 0.41
6.81
9 2494
12 49
23-9
22.3
23-3
2 2.0
22.88
46.7
9* 1 795
9.2183
0.2020
+ 0.51
6.91
9 2374
12 51
44.4
37-4
37-4
39-3
39.62
51-9
9.6093
9.6638
11 2372
12 53
21.9
20.4
23-5
254
22.80
44.2
9.1766
9.2094
Mittel aus den Vergleichsternbeobachtungen: 9.4064; 9.4178; 9.4366.
Zur Reduction benutzt: 9.4203.
Zone 148. 1887 April 27.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 24
und Nr. 26. Luft:
3 -
11° 2372
12^ 56™
i 9?4
i8?2
2I?6
i8?6
19845
4484
9.0449
9.0781
11 2440
12 58
29.2
25-7
27.6
254
26.98
42.7
9-3135
9-3430
7 2480
13 O
15.8
14.7
17.2
14.6
15-58
47-5
8.8581
8.8990
O.3078
+ O.77
7.24
9 2549
13 I
32.5
34-9
33 - 1
32.8
33-32
464
9.4797
9 - 5 D 7
O.3IO9
— 0.78
5-69
0 2843
13 3
21.0
20.6
20.8
19.6
20.50
54-7
9.0887
9 " I 54 I
O.O527
+ 0.13
6.60
5 2545
13 5
19.0
1 7-5
18.4
18.7
18.40
49.6
8.9984
9.0454
O.1614
-b 0.40
6.87
1 2624
13 7
20.4
24.0
22.3
18.5
21.30
53-8
9.1204
9.1821
O.O247
-b 0.06
6-53
4 2553
13 8
20.8
17.8
18.4
18.5
18.88
50.8
9.0200
9.0707
O.I361
+ 0.34
6.81
11 2372
13 IO
18.7
17-5
18.8
17.6
18.15
45-6
8.9869
9.0229
11 2440
13 12
27.8
27.1
28.6
25.6
27.28
43-5
9.3224
9.3536
1 2633
13 14
13-3
12.0
134
13.2
12.98
53-7
8.7029
8.7642
O.4426
4 -1.11
7.58
1 2636
13 16
23.1
19.7
22.3
21.6
21.68
54-0
9 .i 35 o
9-1975
O.OO93
-b 0.02
6.49
j 2 2499
13 i 7
17.4
16.6
15.6
16.5
16.52
52.8
8.9077
8.9655
O.2413
—b 0.60
7.07
6 2543
13 19
22.0
20.7
22.7
20.3
2 I.42
49 * 1
9-1251
9.1706
O.O362
+ 0.09
6.56
4 2569
13 21
14.7
* 3-7
I4.I
i 3 -i
I3.9O
5 i.1
8.7612
8.8129
0-3939
+ 0.98
7-45
1 2656
13 22
13.8
13.6
15.6
14.7
14.42
53-7
8.7925
8.8538
0-3530
+ 0.88
7-35
11 2440
13 24
26.0
26.9
28.7
26.4
27.OO
44-2
9 - 3 i 4 i
9.3469
11 2372
13 26
19.4
19.9
19-3
20.3
I9.72
47.1
9.0563
9.0962
Mittel aus den Vergleichsternbeobachtungen: 9.2106; 9.1882; 9.2216.
Zur Reduction benutzt: 9.2068.
Die Unruhe der Luft ist so gross, dass die Messungen sehr erschwert werden.
Zone 14g. 1887 April 27.
v
Beobachter: Kempf.
Photometer:
Cl. Vergleichsterne: Nr. 27 und Nr.
29. Luft
3 -
11° 2485
1 3 11 3 7 m
2486
2 I?2
2 69 o
2 3?8
23?90
4384
9.2152
9.2462
IO 2654
13 38
23.0
18.4
22.2
20.5
21.02
42.3
9.1095
9.^82
18 2682
13 40
27-5
24.8
31.0
27.7
2745
35-6
9-3361
94538
O.1999
— 0.50
4-79
18 2697
13 42
32.5
27.8
3 i -5
30.5
30.58
35-0
94130
9.4299
O.2760
— 0.69
4.60
14 2591
13 44
22.9
18.5
18.9
18.4
19.68
38.6
9-0547
9.0768
O.0771
+ 0.19
548
6 2722
13 46
30.0
2Ö.2
29.7
25.0
27.72
46.8
9.3352
9-3743
0.2204
— 0.55
4-74
2 2664
13 47
19-5
15.0
15.0
14.7
16.05
50.1
8.8833
8.9318
O.222 1
+ 0.56
5-85
14 2621
13 49
22.0
I 8.3
l8.6
18.5
19-35
38.3
9.0406
9.0622
0.0917
+ 0.23
5-52
II 2485
13 5 i
25.1
22.2
23.6
23.0
23.48
44.2
9.2007
9-2335
