190
Müller und Kempf, Photometrische Durchmusterung
190
1 U).
Sternzeit
I
II
III
IV
J
z
logsin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 162
1887 October 13.
Beobachter : Kempf.
Photometer :
D. Vergleichsterne: Nr. 38 und Nr.
40. Luft :
2.
IO°
3573
20 1
39 m
2I?3
2 2?5
23 ?2
2 I?7
2 2?I 8
49 ?i
9-1539
9- 1 994
IO
3981
20
42
18.7
18.0
19.6
18.6
18.72
43-9
9.0129
9.0450
4
4114
20
44
2 I .O
19.4
20.0
19.1
19.88
50.8
9.063 i
9-1139
0.0117
+ O.03
6.87
2
3892
20
46
2 Ó.O
27.1
28.5
26.1
26.92
52.6
9 - 3 II 7
9.3688
0.2432
— 0.61
6.23
2
39°4
20
48
20.8
23.2
25.O
23.0
24.50
52.6
9-2355
9.2926
0.1670
— O.42
6.42
8
4112
20
50
I5-I
13-5
1 4-5
134
14.12
47-3
8.7746
8.8150
0.3106
-\~ 0.78
7.62
i
4010
20
52
28.5
24.2
25.2
26.0
25.98
54 -o
9.2831
9-3456
0.2200
-O.55
6.29
i
4021
20
53
23.2
21.2
21.5
22.0
2 I.98
53-8
9.1464
9.2081
0.0825
0.2 I
6.63
IO
3573
20
56
23-5
19.7
22.6
21.8
2 I.90
50.9
9- I 434
9-1945
IO
3981
20
58
18.2
19.1
18.5
19-5
18.82
45 -i
9 -OI 73
9.0521
3
4043
2 I
0
26.4
22.4
23.0
21.9
23.42
53 -o
9.1986
9.2572
0.1316
— 0-33
6.51
5
4 D 7
21
2
19.0
18.5
18.0
1 7-9
1845
50.9
8.9961
9.0472
0.0784
+ 0.20
7.04
7
4116
2 I
4
20.0
20.9
18.9
20.2
20.00
49-3
9.0681
9.1142
0.0114
+ 0.03
6.87
9
4139
2 I
6
17.4
17.1
1 7-5
16.4
I 7.IO
47-7
8.9368
8.9783
0-1473
+ O.37
7.21
4
4152
2 I
8
25.2
21.8
25-4
23.6
24.OO
51-9
9.2186
9 - 273 I
0.1475
— 0-37
6.47
IO
3573
2 I
10
22.2
20.1
20.4
20.4
2O.78
52.6
9.0999
9-1570
.
IO
3981
2 I
12
21.0
20.0
20.0
19.0
20.00
46.2
9.0681
9 - 1 °5 ^
Mittel aus den Vergleichsternbcobachtungen: 9.1222; 9.1233; 9.1313.
Zur Reduction benutzt: 9.1256.
Zone 163
. 1887 October 13.
Beobachter: Müller.
Photometer: D. Vergleichsterne: Nr. 40
und Nr. 42. Luft: 1
—2.
IO°
3981
2 1 1
i6 m
17-4
l6?2
16? 7
1 7?4
l6?92
4686
8.9279
8.9665
IO
4351
2 1
19
21.3
I9.4
2 1.6
19.4
20.42
42.4
9.0854
9- 1J 43
IO
3984
2 I
21
26.2
24.6
26.4
26.4
25.90
46.9
9.2806
9-3 ! 99
0.2464
O.Ó 2
6.18
18 4162
2 I
22
19.0
20.4
19-5
1 9*5
19.60
40.0
9-0513
9-0757
0.0022
— 0.01
6.79
18 4168
2 I
24
14.4
16.O
17-5
16.4
16.08
40.4
8.8849
8.9100
0.1635
+ 0.41
7.2 1
16
3925
2 I
25
16.6
14.8
16.6
1 7-5
16.38
41.7
8.9005
8.9280
0.1455
4- 0.36
7.16
16
3928
2 I
26
13-3
II.4
14-3
11-3
12.58
41.8
8.6761
8.7038
0.3697
+ 0.92
7.72
16 3936
2 I
28
24.6
22.7
22.6
21.6
22.88
42.5
9-1795
9.2086
0.1351
— 0.34
6.46
IO
3981
2 I
29
18.5
16.4
20.6
16.9
18.10
47.8
8.9846
9.0264
IO
4351
2 I
31
24.4
20.4
22.4
,20.5
21.92
43 -o
9.1442
9-1743
18 4182
2 I
34
13-5
11*4
12.7
11.1
12.18
40.7
8.6485
8.6742
0-3993
“f- I .OO
7.80
18
4204
2 I
35
17.7
16.3
18.0
17.4
17-35
41.2
8.9491
8-9757
0.0978
+ 0.24
7.04
16
3947
2 I
37
15-7
13.6
14-3
14.0
14.40
43-5
8.7913
8.8225
0.2510
+ 0.63
7-43
12
4027
21
38
15.0
1 5-7
14-3
14-3
14.82
46.4
8.8157
8-8537
0.2198
+ 0.55
7-35
I I
3954
2 I
39
22.4
21.1
21.7
21.8
21-75
47-3
9-1377
9.1781
0.1046
— 0.26
6-54
12
4059
2 I
41
24.6
21-5
25-4
23.4
23.72
46.3
9.2090
9.2468
0.1733
— 0.43
6-37
IO
3981
2 I
43
17.6
15-3
18.2
18.7
17-45
49-3
8-9539
9.0000
IO
4351
2 I
45
21.9
20.9
23-5
19.6
21.48
43-8
9.1274
9-1593
Mittel aus den Vergleichstcrnbeobachtungen : 9.0404; 9.1004; 9.0796.
Zur Reduction benutzt: 9.0735.
Zone 164
. 1887 October 13
Beobachter: Kempf.
Photometer :
D. Vergleichsterne: Nr. 40 und Nr. 42. Luft:
2.
IO C
4351
2 l 1
48 m
22? 3
2 2?9
23-5
2384
23802
4480
9.1845
9.2 168
IO
398 i
2 1
50
22.5
19-5
23.O
20.5
21.38
50.0
9-1235
9.1717
IO
4032
2 I
53
18.5
14.2
16.4
17.7
16.70
49.8
8.9169
8.9645
0.2346
4- 0.59
7-39
I 2
4060
2 I
56
20.0
20.4
20.9
21.6
20.72
47-9
9-0975
9-!395
0.0596
+ 0.15
6-95
13
4154
2 I
58
19.4
18.4
17-5
17.6
18.22
47-5
8.9901
9.0310
0.1681
+ 0.42
7.22
l8 4216
22
0
19.0
20.5
20.4
21.2
20.28
43-7
9.0797
9 - 1 113
0
b
00
"j
CO
-f- 0.22
7.02
15
3944
22
2
13-3
15-4
134
12.1
13-55
45-9
8.7396
8.7764
0.4227
+ 1.06
7.86
IO
4058
22
3
25-5
24-5
25.0
26.4
25-35
5°-6
9.2632
9-3133
0.1142
— 0.29
6.51
IO
398 i
22
5
20.4
20.5
21.6
21-5
2 1 .OO
51.8
9.1087
9.1629
