132
Müller und Kempf, Photometrtsche Durchmusterung
132
B.D.
Sternzeit
I
II
III
IV
J
2
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 16.
1886 October 27.
Beobachter: Müller. Photometer: D. Vergleichsterne: Nr. 42 und Nr. 44.
Luft: 1-
-2.
IO °435 1
22 h 8 m
2 2?I
18?6
2286
2183
21815
4587
9.1146
9.1509
io 4604
22 IO
23.2
22.5
2 8.6
24.4
24.68
42.6
9.2414
9.2707
3 4551
22 12
l8.6
19-3
22.7
19.6
20.05
49.9
9.0702
9.1181
0.1142
+ O.29
6-77
2 4348
22 15
20.5
21.8
26.4
19.4
22.02
51-4
9.1479
9.2007
0.0316
+ 0.08
6.56
9 4800
22 17
25-3
20.4
26.6
22.3
23-65
44-3
9.2066
9.2396
0.0073
0.02
6.46
0 4726
22 19
2Ó.I
22.0
28.6
23-7
25.10
53-2
9-2551
9-3145
0.0822
0.2 I
6.27
9 4809
22 2 I
9.6
12.6
14.0
12.5
12.18
44.4
8.6485
8.6817
0.5506
+ U38
7.86
4 4675
22 23
18.7
17.2
22.4
18.5
19.20
49.1
9.0340
9-0795
0.1528
+ O.38
6.86
10 4351
22 25
22.6
22.6
23-4
22.6
22.80
47.2
9.1766
9.2167
10 4604
22 28
27.6
23.6
27-3
22.4
25.22
43-3
9.2590
9.2898
2 4362
22 31
12-5
10.2
13.0
13-3
12.25
51.6
8.6534
8.7069
0.5254
4- 1-31
7-79
7 4696
22 33
23.6
22.3
26.7
22.6
23.80
46.9
9.2118
9-2511
0.0188
— 0.05
6-43
5 4790
22 35
22.5
20.1
24.9
21.1
22.15
48.5
9.1528
9.1965
0.0358
+ O.O9
6-57
3 4568
22 37
l6.6
12.2
18.5
15-1
15.60
51-2
8.8592
8.9113
0.32 IO
+ O.80
7.28
4 4697
22 38
15.0
13.0
14.7
134
14.02
50.2
8.7686
8.8174
0.4149
+ 1.04
7-52
0 4750
22 41
14.4
12.5
16.5
16.0
14.85
54-o
8.8175
8.8800
0.3523
+ 0.88
7-36
10 4351
2 2 44
22.0
20.6
24.1
20.4
21.78
49.1
9.1388
9.1843
10 4604
2 2 46
25-9
23.2
1 27-3
23.2
24.90
44-3
9.2486
9.2816
Mittel aus den Vergleichsternbeobachtungen: 9.2108; 9.2533; 9.2329.
Zur Reduction benutzt: 9.2323
Zone 17.
1886 October 27
Beobachter:
Kempf.
Photometer :
D. Vergleichsterne: Nr. 48 und Nr.
2. Luft: 2.
9° 5 2 7 7
O h 20 m
2 588
2285
2980
2580
25-58
4386
9.2705
9.3019
9 47
O 24
32.5
28.8
34-7
30.1
3I-52
42.8
9-4367
9.4664
6 5216
O 27
32.0
26.5
34-9
30.9
31.08
46.6
9-4257
9.4643
0.1087
— 0.27
6.25
7 5101
O 31
I9.9
18.3
21.4
20.2
19-95
45-6
9.0660
9.1020
O.2536
+ 0.63
7-15
9 5300
O 34
l8.0
16.0
19.0
15-5
17.12
43-9
8.9378
8.9699
0.3857
+ 0.96
7.48
3 4909
0 37
I 7.O
17-5
22.2
21.3
19.50
49.2
9.0470
9.0928
0.2628
+ 0.66
7.18
7 5113
0 39
I4.4
12.9
17.6
17.8
15.68
45-9
8.8636
8.9004
04552
+ 1.14
7.66
8 5164
0 42
25-5
26.0
27.0
25.2
25.92
45-i
9.2812
9.3160
O.0396
+ 0.10
6.62
9 5 2 77
0 44
23.6
22.3
25.0
25-9
24.20
44-7
9.2254
9-2593
9 47
0 48
25-5
26.9
29-5
30.0
27.98
43-i
9.3426
9-3729
7 5121
0 51
35'6
33-6
32.2
35-6
34-25
45-9
9.5007
9-5375
0.1819
— 0.45
6.07
8 5172
0 52
12.3
12.1
14.0
13.0
12.85
44.6
8.6943
8.7280
O.6276
+ i-57
8.09
7 5
0 54
15.0
14.0
17.0
16.4
15.60
46.2
8.8592
8.8967
0.4589
+ 1.15
7.67
7 13
0 57
16.0
14-3
17-5
14-5
I5-58
46.3
8.8581
8.8959
0-4597
+ 1.15
7.67
0 19
0 59
21.1
18.6
25.0
21.8
21.62
52.7
9.1328
9.1903
O.1653
+ 0.41
6-93
0 22
1 0
16.9
16.2
21.1
17.6
17-95
52.8
8.9777
9-0356
0.3200
+ 0.80
7-32
9 5277
i 3
24-5
22.6
27-3
25.0
24.85
46.0
9.2470
9.2840
9 47
i 5
28.3
2 7-5
35-6
31.6
30.75
43-8
9.4174
9-4493
Mittel aus den Vergleichsternbeobachtungen: 9.3842; 9.3161 ; 9.3666.
Zur Reduction benutzt: 9.3556.
Zone 18
1886 October 27
Beobachter:
Müller. Photometer
: D. Vergleichsterne: Nr.
2 und Nr.
4. Luft: 2.
9° 47
l h IO m
2788
2582
2685
2486
26802
43°9
9.2843
9.3164
10 168
l 13
17.2
15.O
16.7
15.0
15.98
41-5
8.8796
8.9067
6 43
1 16
18.6
17-3
21.2
20.1
19.30
46.7
9.0384
9.0772
0.0440
+ 0.11
6.80
3 46
1 18
16.4
16.7
18.4
16.4
16.98
50.7
8.9309
8.9813
0.1399
+ 0.35
7.04
4 63
I 19
21.3
19.6
23.8
21.0
2 I.42
49-5
9-1251
9.1718
0.0506
— 0.13
6.56
8 64
1 21
17.4
16.4
18.7
16.3
I 7.2O
45-3
8.9417
8.9770
O.1442
+ 0.36
7-05
6 64
I 23
28.4
27-5
35-5
29.6
30.25
47-5
9.4045
9-4454
O.3242
— 0.81
5.88
9 62
I 25
14.6
16.6
18.6
17.7
16.88
44-3
8.9259
8.9589
O.1623
+ 0.41
7.10
9 47
1 27
24-3
26.4
28.5
2 3-7
25.72
44.8
9.2749
9.3090
