234
Müller und Kempf, Photometrische Durchmusterung
234
JLD.
Sternzeit
I
11
III
IV
J
z
logsin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
io°4Ó04
o h
o m
31-7
2783
28? 7
2982
29822
5180
9-3771
9.4285
9
5 111
0
■
24.4
23.0
25.0
22.4
23.70
45-3
9.2083
9.2436
14
4790
0
3
21.3
19.8
21.2
20.9
20.80
43 -o
9.1007
9 - i 3°8
0.2113
+ 0.53
7.07
14 4786
0
4
22.5
21.4
21.2
18.6
20.92
42.9
9-1055
9-1354
O.2067
+ 0.52
7.06
15
4639
0
6
21.4
20.0
20.2
20.0
20.40
42.4
9.0846
9 -i 135
0.2286
+ 0.57
7.11
16
4724
0
7
19.4
16.9
16.6
17.2
17-52
41-3
8-9573
8.9841
0.3580
+ 0.90
7-44
17 4746
0
9
31-9
28.0
27.4
28.2
28.88
40.6
9-3679
9-3934
O.0513
— 0.13
6.41
11
4804
0
IO
19.6
17-7
19.8
16.5
18.40
46.0
8.9984
9-0354
O.3067
+ 0.77
7 - 3 1
IO
4604
0
12
I 30-4
28.5
29-3
28.3
29.12
524
9-3744
9.4308
9
5 111
0
13
25.6
23-3
25.0
21.8
23.92
46.2
9.2159
9-2534
Mittel aus den Vergleichsternbeobachtungen: 9.3481 ; 9.3361; 9.3421.
Zur Keduction benutzt: 9.3421.
Zone
273 -
1888 December
5 -
Beobachter: Kempf.
Photometer: D. Vergleichsterne: Nr. 42 und Nr. 44. Luft: 1
—2.
io {
’4351
22^
55 ™
2 7?o
2482
2581
2685
25870
5082
9-2743
9-3231
IO
4604
22
59
30.6
27.1
30.0
32-3
30.00
45-2
9-3979
9-4330
13
4692
23
3
21.0
20.0
20.4
18.4
19-95
44.1
9.0660
9.0985
O.3046
+ 0.76
7.24
17
4577
23
5
14.1
12.1
14-5
12.5
13-30
40.1
8.7236
8.7482
O.6549
+ 1-64
8.12
14
4609
23
10
24.0
21.7
22.6
234
22.92
43 -i
9.1809
9.2112
O.1919
+ 0.48
6.96
15
4416
23
11
27.0
23-5
25-5
24-3
25.08
42.7
9-2545
9.2840
0.1191
-4- 0.30
6.78
17
4582
23
13
24.0
23.0
24.8
22.5
23-58
41.2
9.2042
9.2308
0.1723
+ 0.43
6.91
18
4794
23
16
3
30.0
31.2
28.8
30.28
40.3
9-4053
9.4302
O.O271
— 0.07
6.4-1
IO
4351
23
18
30.8
26.9
29-5
27.0
28.55
53 -o
9-3587
9 - 4 I 73
IO
4604
23
21
30.2
30.6
29-5
28.4
29.68
47.1
9-3895
9.4294
13
4708
23
25
17-5
19.2
19-5
18.5
18.68
46.3
9.0111
9.0489
0.3542
4- 0.89
7-37
IO
4547
23
27
20.5
18.6
23.0
214
20.88
49.2
9.1039
9.1497
0.2534
4- 0.63
7.11
IO
4554
23
29
27-3
24.6
26.4
254
25.92
48.9
9.2812
9.3261
O.O77O
+ 0.19
6.67
11
4573
23
31
19.8
16.6
19-9
17.6
18.48
48.3
9.0021
9-0453
0.3578
+ 0.89
7-37
17
4592
23
33
28.1
29-3
29.6
27.4
28.60
43 -i
9.3601
9.3904
0.0127
+ 0.03
6.51
17
4594
23
35
19.0
16.6
18.4
17.9
17.98
42.7
8.9791
9.0086
0.3945
4- 0.99
7-47
IO
435 1
23
37
27.6
26.0
27-5
26.4
26.88
55-3
9-3105
9-3785
IO
4604
23
39
29-5
29.6
30.6
29.6
29.82
48.7
9-3932
9-4375
Mittel aus den Vergleichsternbeobachtungen: 9.3781; 9.4233; 9.4080.
Zur Keduction benutzt: 9.4031.
Zone
274.
1888 December
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 44 und Nr. 46. Luft: 1-
—2.
IO f
’4604
23
54 m
31-4
31-5
31-5
2985
30898
5083
9.4232
9-4723
9
5 “ 1
23
56
26.5
25-5
26.9
27.1
26.50
44.9
9.2991
9-3335
16 4673
O
0
20.6
18.4
18.6
18.5
19.02
42.2
9.0262
9-0547
0.3293
4- 0.82
7-36
13
4861
O
1
254
25.8
28.0
27.0
26.55
44-7
9.3006
9-3345
O.O495
4-0.12
6.66
18 4946
O
3
33-9
31.2
33-2
30.0
32.08
40.4
94503
9-4754
O.O914
— 0.23
6.31
IO
4701
O
5
37-5
32.8
37-6
36.3
36.05
47.8
9-5395
9-5813
0.1973
— 0.49
6.05
15
4592
O
8
34 -o
30.6
33-6
36.5
33-68
44.0
9.4879
9.5202
O.I362
— 0.34
6.20
17
4712
O
IO
27.8
25.2
25-9
24.4
25.82
42.1
9.2780
9.3063
0.0777
+ 0.19
6-73
IO
4604
O
11
27.0
29-5
31-2
30.0
29.42
52.3
9.3825
9-4385
9
51H
O
14
27.7
25-5
244
24.1
25.42
46.2
9.2654
9.3029
*)i6 4694
O
18
29-5
27.8
30.7
30.0
29.50
43-9
9-3847
9.4168
O.O328
— 0.08
6.46
11
4765
O
21
18.5
154
18.1
154
16.85
48.8
8.9244
8.9690
O.415O
4-1.04
7-58
12
4793
O
25
17.4
15.6
18.5
14-3
16.45
48.1
8.9041
8.9467
0.4373
+ 1.09
7-63
12
4797
O
26
19-5
19.8
20.5
20.4
20.05
48.2
9.0702
9 -ii 3 i
O.2709
4- 0.68
7,22
13 4887
O
28
22.1
20.7
21.0
21.8
21.40
47-3
9-1243
9.1647
O.2193
+ 0.55
7-09
14 4766
O
30
21.7
19.0
21.2
17-5
19.85
46.8
9.0618
9.1009
O.283I
+ 0.71
7-25
IO
4604
O
32
32.6
304
324
31.0
31.60
54-9
9.4386
9.5049
9
5 111
O
35
23.0
22.4
26.5
23.0
23.72
48.1
9.2090
9.2516
Mittel aus den Vergleichsternbeobachtungen: 9.4029; 9.3707; 9.3783.
Zur Reduction benutzt: 9.3840.
*) 16° 4694 dupl. Gemessen die hellere, südliche Componente.
