168
Müller und Kempf, Pi-iotometrische Durchmusterung
168
B.
1 ).
Sternzeit
I
II
III
IV
J
z
log sin 2 J
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 107. 1887 März 8.
Beobachter: Müller.
Photometer:
I). Vergleichsterne: Nr. 10
und Nr. 12. Luft: 2.
io° 818
7 h
5 m
25%
2483
2 6?3
2Ö?5
25868
4684
9.2737
9 . 3 II 7
11
632
7
7
14.7
12.6
I4.8
12.6
13.68
51.8
8.7477
8.8019
IO
688
7
9
14.0
12.6
154
13.2
13.80
49.8
8.7551
8.8027
0.2655
+ 0.66
7 - 1 1
11
702
7
10
13-3
11.6
13.0
1 1-3
12.30
49-2
8.6569
8.7027
0.3655
+ 0.91
7 o 6
11
704
7
12
10.6
1 1*3
12.0
10.9
I 1.20
48.7
8.5767
8.62 10
0.4472
4 ~ 1.12
7-57
14
825
7
13
14.4
14.0
15.6
14-3
14.58
46.2
8.8018
8.8393
0.2289
+ 0.57
7.02
13
803
7
15
12.5
10.8
13.0
11.0
I 1.82
46.9
8.6228
8.6621
0.4061
+ 1.02
7-47
19
847
7
16
17.6
16.4
18.7
16.6
17.32
42.2
8.9476
8.9761
0.0921
+ O.23
6.68
11
632
7
18
14-3
134
154
13-7
14.20
53*2
8.7794
8.8388
IO
818
7
20
25-7
24-5
26.0
23.0
24.80
47.8
9.2454
9.2872
1 2
732
7
23
8-3
7.0
8.8
7.6
7.92
49.0
8.2785
8.3237
0.7445
4 " 1 -86
8.31
11
724
7
25
13.0
11 -7
13-3
11.0
12.25
49-9
8.6534
8.7013
0.3669
+ 0.92
7-37
IO
718
7
26
12.5
ii -3
12.9
13-3
12.50
50.8
8.6707
8.7215
0.3467
4-0.87
7.32
13
821
7
28
Do
154
16.3
16.0
16.25
48.4
8.8938
8-9373
0.1309
+ 0.33
6.78
iQ
853
7
30
18.ö
17.6
19.4
17.6
18.15
43-4
8.9869
9.0179
0.0503
4-0.13
6.58
19
876
7
3 i
10.3
9-7
10.6
10.7
IO.32
42.7
8.5064
8-5359
0.5323
+ i -33
7.78
11
632
7
33
14.7
12.4
16.4
134
14.22
55 -i
8.7806
8.8477
IO
818
7
35
25-9
23.8
28.7
24.6
2545
49-3
9.2759
9.3220
Mittel aus den Vergleichsternbeobachtungen: 9.0568; 9.0630; 9.0849.
Zur Reduction benutzt: 9.0682
Zone 108. 1887 März 8.
Beobachter:
Etempf.
Photometer:
D. Vergleichsterne: Nr. 12 und Nr. 14. Luft:
3 -
IO°
818
7 h
39 ™
3185
3186
3281
2986
31820
4987
9.4287
9.4760
IO
1149
7
41
25.0
23-5
22.9
24.0
23.85
44.9
9.2135
9.2479
IO
885
7
44
13.0
134
13-9
12.6
13.22
48.4
8.7185
8.7620
0.6226
+1-56
7.65
14
1025
7
45
26.0
27.7
30.5
27.6
27-95
45-2
9.3418
9.3769
0.0077
4- 0.02
6.11
17
1004
7
47
32.0
32-5
32.5
34 -i
32.78
42.6
9.4670
94963
0.1117
— 0.28
5.81
12
896
7
48
17.9
16.3
18.4
16.3
17.22
47-5
8.9427
8.9836
0.4010
4- 1.00
7.09
12
902
7
49
17-5
19-5
19.9
16.1
18.25
47-4
8.9915
9.0322
0.3524
4-0.88
6-97
I I
945
7
5 i
18.6
15.0
18.0
15.0
16.65
48.0
8.9144
8.9567
0.4279
4- 1-07
7.16
IO
818
7
52
29.1
30.8
30.0
28.5
29.60
5 i.i
9.3874
9-4391
IO
M 49
7
54
26.1
25.0
25.0
27.0
25.78
45-9
9.2768
9 . 3 I 36
l8
970
7
56
14.4
13-7
14.9
14.1
14.28
43 -o
8.7842
8.8143
0.5703
+ 1-43
7.52
l8
987
7
58
17-5
18.7
20.9
18.6
18.92
42.8
9.0218
9.0515
0.3331
4-0.83
6.92
l 8
990
7
59
15.0
15.0
16.6
16.5
1548
42.8
8.8689
8.8986
0.4860
-h 1-22
7-31
14
1047
8
0
19.0
16.5
19.4
18.6
18.38
46.6
8.9975
9.0361
0.3485
4 - 0.87
6.96
14
1048
8
1
17.6
19.2
234
19.0
19.80
47.1
9.0597
9.0996
0.2850
-hO.71
6.80
I I
953
8
3
18.5
17.9
17.6
16.8
17.70
49.4
8.9658
9.0122
0.3724
+ O.93
7.02
IO
818
8
4
32.0
31.0
3 i-i
31-3
31-35
52.5
9.4325
9.4892
IO
1149
8
6
26.4
26.9
28.2
25.0
26.62
46.9
9.3027
9.3420
Mittel aus den Vergleichsternbeobachtungen
: 9-3620; 9.376
3; 9.4156. Zur Reduction benutzt: 9.3846.
Zone 109. 1887 März 8.
Beobachter: Müller.
Photometer:
D. Vergleichsterne: Nr. 18 und Nr. 20. Luft:
3 -
IO°
1818
9
1 53 m
i8?6
i6? 4
1982
1789
18802
45?4
8.9809
9.0165
9
2239
9
55
15-4
14.0
15-7
15.6
15.18
43-4
8.8361
8.8671
2
2145
9
57
20.4
19.7
22.4
20.9
20.85
51-8
9.1027
9.1569
0.2221
— O.56
6-39
3
2144
9
59
17.4
15.0
18.4
17-5
17.08
50.8
8.9358
8.9866
O.O5 18
— 0.13
6.82
8
2 1 72
10
1
14.4
13.6
16.7
14.6
14.82
45-9
8.8157
8.8525
O.0823
4- 0.21
7.16
9
2133
10
3
15-7
14.0
16.7
15.0
15-35
44.6
8.8456
8.8793
O.O555
4-0.14
7.09
0
2477
10
4
16.3
144
17.6
14.6
15-72
53 -o
8.8658
8.9244
O.OIO4
4-0.03
6.98
6
2 120
10
6
19.1
17-3
21.1
19.0
iq.12
48.1
9.0306
9.0732
O.I384
— 0.35
6.60
IO
l8l8
10
7
18.6
17.0
20.4
17.6
18.40
46.5
8.9984
9.0367
9
2239
10
9
15-3
13-3
154
15-5
14.88
43-7
8.8192
8.8508
