338
Müller und Kempf, Photometrische Durchmusterung
338
B.D.
Sternzeit
I
II
III
IV
J
z
log sin 2 /
corrig.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 534. 1892 Januar 7.
Beobachter :
Müller.
Photometer :
D. Vergleichsterne: Nr. 16 und Nr.
18. Luft:
3 -
ii°
1588
5 h 48 m
2583
2383
24?6
2388
24825
4582
9.2271
9.2622
IO
1818
5 50
22.5
22.7
21.4
21.6
22.05
52.4
9 -H 9 I
9-2055
i 4
1850
5 52
23-4
23.0
2'8.8
23-5
24.68
46.4
9.2414
9.2794
0.0370
— 0.09
6-59
i6
1662
5 55
29.7
28.4
29.8
314
29.82
44.1
9-3932
9-4257
O.1833
— 0.46
6.22
11
1785
5 57
17.0
12.7
16.0
13.8
14.88
48-5
8.8192
8.8629
0-3795
+ 0.95
7-63
11
1787
5 59
18.3
154
17.2
15-3
i 6.55
48.7
8.9093
8-9536
0.2888
+ 0.72
7.40
18
1882
6 0
24-5
22.3
24-5
25-5
24.20
42.5
9.2254
9-2545
O.OI 2 I
— 0.03
6.65
13
1868
6 2
26.7
254
24-3
'25.6
25-50
46.3
9.2680
9-3058
0,0634
— 0.16
6.52
11
1588
6 4
254
22.8
234
25.6
24.30
44.0
9.2288
9.2611
IO
1818
6 8
23.2
21.2
22.6
22.7
22.42
50.3
9.1627
9.2118
16
1669
6 10
16.8
14.6
16.5
14-3
15-55
42.9
8.8565
8.8864
0.3560
4- 0.89
7-57
i6
1679
6 13
24.0
23.2
22.4
22.9
23-12
43-3
9.1880
9.2187
O.0237
4- 0.06
6.74
i6
1687
6 14
19.0
18.4
19.2
18.3
18.72
42.8
9.0129
9.0426
0.1998
4- 0.50
7.18
14
1879
6 16
154
14.0
16.6
14.0
15.00
45.2
8.8260
8.8611
0.3813
+ 0.95
7 -63
i 5
1805
6 18
16.6
14-5
17.6
15-2
1 5-98
44.0
8.8796
8.9119
0-3305
+ 0-83
7-51
i6
1704
6 19
21.7
I 9-7
22.6
2 2.7
21.68
42.6
9 -i 35 o
9-1643
0.0781
4- 0.20
6.88
11
1588
6 21
25-9
25-3
25-5
25-1
25-45
42.9
9.2664
9.2963
IO
1818
6 23
244
21.3
23.8
21.3
22.70
48.7
9 -I 730
9-2173
Mittel aus den Vergleichsternbeobachtungen: 9.2339; 9.2364; 9.2568. Zur Reduction benutzt: 9.2424.
Zone 535. 1892 Januar 19
Beobachter: Kempf.
Photometer: Oll. Vergleichsterne: Nr. 7
und Nr. 9.
Luft: 2-
-3-
8°
455
2 11 1 i m
2 I?2
1980
2 1 ?4
2 2?9
2 1 ? 1 2
4488
9 -II 34
9 -H 75
8
652
2 15
19-5
19-5
17.6
20.6
19.30
49 - 1
9.0384
9.0839
18
243
2 18
28.4
31-3
31-9
28.0
29.90
34 -i
9-3953
9.4110
O.2914
— 0.73
4.27
2
317
2 21
29.6
32-5
30.0
3OÖ
30.65
50.4
9.4148
9.4643
0-3447
— 0.86
• 4-14
*J 2
317
2 23
16.0
18.9
16.1
I7.9
17.22
50.5
8.9427
8.9925
0.1271
4- 0.32
3-97
2
422
2 25
39-9
37-7
38.6
37-2
38.35
49-7
9-5855
9.6328
O.5132
— 1.28
3-72
*\ 2
419
2 28
29-5
29-5
27.0
25.2
27.80
49.1
9-3375
9-3830
O.2634
— 0.66
2.99
8
455
2 30
22.7
22.6
22.7
22.5
22.62
44.2
9.1700
9.2028
8
652
2 33
18.5
18.6
18.4
I9.6
18.78
47-5
9-0155
9.0564
8
5 1 1
2 36
35-5
34-5
384
39 -o
36.88
44-7
9-5565
9.5904
0.4708
- 1.18
3.82
i5
612
2 38
314
344
37-6
37 -o
35 -io
41.6
9 - 5 I 93
9.5466
0.4270
— 1.07
3-93
i 7
712
2 41
35-3
32.0
30.6
30.5
32.10
39-8
9.4508
9-4749
0-3553
— 0.89
4 -ii
*) 1 7
712
2 43
15-5
I 9-7
15.6
* 7-5
17.08
39-6
8-9358
8-9595
0.1601
4 0.40
4-05
18
640
2 45
39-5
35 -o
354
35-5
36.35
38.4
9-5457
9-5674
0.4478
.— 1.12
3-88
8
455
2 48
20.5
22.1
21.5
20.0
21.02
43-9
9 - 1 °95
9.1416
8
652
2 50
20.0
20.0
17-5
20.6
I9-52
46.2
9.0479
9.0854
Mittel aus den Vergleichsternbeobachtungen: 9.1157; 9.1296; 9.1135. Zur Reduction benutzt: 9.1196.
*) Mit Blende 4 beobachtet.
Zone 536. 1892 Januar 20
#
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18
Luft : 1-
—2.
ii°
1588
5“ 35“
23%
20?5
2 2?5
2380
2 2?40
4684
9.1620
9.2000
IO
1818
5 38
2 1.1
I9.O
20.6
19.7
20.10
53-9
9.0723
9- J 344
i 9
1896
5 42
18.6
15-5
18.5
154
I 7.OO
42.0
8.9319
8.9600
0.2359
40.59
7.27
18
1816
5 44
17-5
I4.O
1 7-5
154
IÓ.IO
42.3
8.8859
8.9146
0.2813
+ 0.70
7-38
18
1778
5 45
17.0
14-5
174
1 5-5
IÓ.IO
41.7
8.8859
8.9134
0.2825
4 0.71
7-39
17
1696
5 47
15.6
134
154
14-5
I4.72
42.4
8.8100
8.8389
0.3570
4- 0.89
7-57
16
1580
5 49
17.0
15.0
16.0
14-5
I5.62
43 -o
8.8603
8.8904
0.3055
4 0.76
7-44
16
1590
5 51
33-5
33-5
32.2
35 -o
33-55
43-3
9.4850
9-5157
0.3198
— 0.80
5.88
16
1598
5 54
28.5
28. 1
29.6
2 8.6
28.70
42-5
9.3629
9.3920
O.1961
— 0.49
6.19
