360
Müller und Kempf, Photometrische Durchmusterung
360
B.D.
Sternzeit
I
II
III
IV
J
z
logsill 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
o °3337
i 3 h 55 m
25-1
2 2?2
26? 8
2385
24 ? 4 o
54°9
9.2321
9.2984
0.2568
— O.64
6.16
i 3059
13 57
18.8
17.O
18.7
18.3
18.20
53-5
8.9892
9.0497
0.0081
0.02
6.78
1 3067
13 59
29.4
31.0
30.0
28.4
29.70
53-7
9.3900
94513
0.4097
1.02
5-78
0 3349
14 0
15-4
12.0
14.1
14-3
13-95
54 -o
8.7643
8.8268
0.2148
4 - 0.54
7-34
9 3025
14 2
14.9
13-7
14.6
11-9
1378
45-6
8.7539
8.7899
0.2517
4- 0.63
7-43
11 2780
14 5
19-3
19-3
21.2
18.8
19.65
43.2
9-0534
9.0839
9 3203
14 7
17-5
16.3
18.7
16.9
17-35
50.7
8.9491
8-9995
Mittel aus den Vergleichsternbeobachtungen: 9.0389; 9.0443; 9.0417.
Zur Reduction benutzt: 9.0416.
*) 9° 3000 dupl. ; eng. Als ein Stern gemessen ;
unsicher.
Zone 589. 1892 Mai 12.
Beobachter: Müller.
Photometer: Cu. Vergleichsterne: Nr. 27 und Nr. 33. Luft:
X—2.
11° 2485
I4 h l6 m
1 386
1383
14?i
i 3°5
13862
4682
8-7439
8.7814
7 3023
14 19
16.0
14-5
15.8
17.4
I5-92
47-7
8.8765
8.9180
4 266g
14 2 1
25-7
25.2
23-7
2Ó.1
25.18
51-9
9.2577
9.3122
0.4599
— i • 15
3-71
*) 4 2669
14 22
14.2
14-3
13-7
13.8
14.00
52.0
8.7674
8.8223
0.0300
+ 0.08
3-59
11 2529
14 24
33 -o
34-5
33-7
38.5
34-92
44-5
9 - 5 I 54
9.5488
0.6965
— 1.74
3.12
0 3076
14 2 7
25.6
254
25.6
31-3
26.98
53-9
9-3135
9-3756
0.5233
— 1-31
3-55
19 2725
14 29
34-7
354
32.8
36.6
34.88
34-3
9.5146
9-5306
0.6783
— 1.70
3.16
11 2485
14 31
13.0
12.7
12.7
12.8
12.80
47.6
8.6909
8.7321
7 3023
14 33
17.7
17-3
174
16.3
17.18
46.8
8.9407
8.9798
14 2770
14 35
22.5
22.5
23.0
22.2
22.55
38.2
9-i675
9.1889
0.3366
— 0.84
4.02
17 2768
14 38
18.9
18.3
16.8
16.5
17.62
35-5
8.9620
8-9795
0.1272
— 0.32
4-54
11 2821
14 39
22.5
21.2
21.3
22.0
2 i -75
42.7
9-1377
9.1672
0.3149
— 0.79
4.07
6 3088
14 43
34*9
36.6
39-7
44-5
38.92
47.0
9-5963
9-6359
0.7836
— 1.96
2.90
*) 6 3088
14 45
17.8
I9.4
18.5
20.8
19.12
46.9
9.0306
9.0699
0.2 I 76
— 0.54
2 .97
7 3023
14 46
154
I7.4
16.3
16.9
16.50
46.1
8.9067
8.9440
11 2485
14 48
12.6
I3.6
13.2
13-1
13.12
49.4
8.7120
8.7584
Mittel aus den Vergleichsternbeobachtungen
: 8.8497; 8.8560; 8.8512.
Zur Reduction benutzt: 8.8523
*) Mit Blende 4 beobachtet.
Zone 590. 1892 Mai 22.
Beobachter: Kempf.
Photometer:
Ci. Vergleichsterne: Nr. 31
und Nr. 33. Luft:
1.
I 2 ° 2 7 29
1 4 h 4 1 111
1785
1985
20?4
1985
19822
4083
9.0349
9.0598
7 3023
H 43
33-6
29.7
3°.8
30.7
31.20
46.2
9.4287
9.4662
19 2935
14 46
17-5
18.5
16.7
18.0
17.68
33-2
8.9649
8-9795
O.277 I
+ 0.69
5-86
5 2985
14 48
22.9
20.5
20.9
23-5
21-95
47.2
9-1453
9.1854
O.0712
4-0.18
5-35
0 3327
14 49
17.4
18.5
17-3
17.8
17-75
51.8
8.9682
9.0224
O.2342
-f-0.59
5-76
2 2944
14 51
22.8
24.4
22.5
23.6
23-32
50.4
9 -I 95 I
9.2446
O.OI 20
4- 0.03
5.20
15 2858
14 53
24.6
24-5
24.6
25-3
24-75
37 -o
9.2438
9.2634
O.O068
— 0.02
5-15
13 2982
14 56
21.5
21.0
19-5
21.9
20.98
40.0
9.1079
9-1323
O.I243
4- 0.31
5-48
12 2729
14 57
18.0
1 8.9
18.4
19-5
18.70
4°-5
9.0120
9-0373
7 3 02 3
H 59
32.5
324
30.5
31-5
3 I -72
45-5
9.4416
9-4774
18 3074
15 i
43-5
43-5
43-6
42.5
43.28
34-9
9.6721
9.6889
O.4323
— 1.08
4.09
2 3007
15 3
22.5
22.8
19.6
20.5
2 i -35
5°-6
9.1224
9-I725
O.084I
4- 0.21
5-38
18 3101
15 5
254
23.6
23-3
24-5
24.20
35-7
9.2254
9.2432
O.OI34
4- 0.03
5.20
17 2964
15 7
26.0
25.8
25.0
25.6
25.60
36.8
9.2711
9.2904
O.O338
— 0.08
5-09
5 3165
15 9
20.5
20.0
20.5
19-5
20.12
48.6
9-0731
9-ii7i
O.I395
4-0.35
5-52
i 3215
15 ii
254
254
25-7
26.9
25-85
52.9
9.2790
9-3372
O.0806
— 0.20
4-97
12 2729
15 13
17.6
19-5
18.6
16.5
18.05
40.9
8.9823
9.0083
7 3023
15 15
1 314
33-8
31.6
324
32.30
45 -o
9-4557
9 - 49 Ò 3
Mittel aus den Vergleichsternbeobachtungen: 9.2630; 9.2574; 9.2493.
Zur Reduction benutzt: 9.2566.
