342
Müller und Kempf, Photometrische Durchmusterung
342
B.D.
| Steinzeit
1 I
II
III
IV
J
z
logsin 2 /
•
corng.
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zone 544. 1892 März 4.
Beobachter: Müller.
Photometer:
Ci. Ver gleichster ne: Nr. 17 und Nr.
19. Luft:
2.
11°1670
8 h 48™
3 i -4
2883
2983
2 8?0
29825
4386
9.3780
9.4094
11 1984
8 50
30-0
27.2
26.6
294
28.30
41.4
9-3517
9-3787
17 1731
8 55
27-3
25.8
27.7
27.6
27.10
36.7
9 * 3 1 7 1
9-3363
O.0679
+ O.17
5.68
2 1854
8 57
j 47-4
424
44.2
47-5
45-38
5 J -3
9.7047
9-7571
0.3529
— 0.88
4-63
13 1831
8 59
32.6
3 °.!
29.8
27.7
30-05
40.8
9-3993
9 - 425 I
0.0209
— O.05
5-46
18 1867
9 2
48.0
44.8
42.6
4 i -5
44.22
36.1
9.6870
9-7053
O.301 I
— 0-75
4.76
8 2053
9 4
32.5
29.7
29.6
3 I> 7
30.88
45-4
9.4207
9-4563
O.0521
— O.13
5-38
13 1912
9 6
27.0
24.2
2 1.0
24.8
24.25
40.4
9.2271
9.2522
O. I 52O
+ O.38
5-89
11 1670
9 8
3 uo
28.7
30.9
28.6
29.80
45 -o
9-3927
9-4273
11 1984
9 10
31.8
25-5
29.8
294
29.1 2
4 I -3
9-3744
9.4012
Mittel aus den Vergleichsternbeobachtungen: 9.3941; 9.4142. Zur Reduction benutzt: 9.4042.
Zone SäS- 1892 März q.
Beobachter:
Müller. Photometer
: D. Vergleichsterne: Nr.
20 und Nr. 22. Luft: 2.
9° 2239
8 ll 44 m
17?8
1 4?0
i 5?5
1385
15°20
4489
8.8372
8.87 16
9 2374
8 46
27.1
274
274
25.0
26.72
48.0
9-3057
9.3480
1 2406
8 49
19.0
16.5
1 7-5
15.0
I 7.00
53 -o
8.9319
8.9905
0.1184
+ 0.30
6.86
3 2334
8 50
13-3
10.6
i 3 -i
12.2
12.30
5 i -4
8.6569
8.7097
0.3992
+ 1.00
7-56
3 2352
8 53
18.3
16.9
16.3
16.2
16.92
52-4
8.9279
8.9843
0.1246
+ 0.31
6.87
3 2358
8 54
21.0
20.4
21.9
20.0
20.82
52.5
9-1015
9.1582
0.0493
0.1 2
6-44
3 2361
8 55
20.3
17.0
19.0
17.0
18.32
52.5
8.9947
9.0514
0.0575
+ 0.14
6.70
3 2365
8 57
16.0
13.2
154
134
14.50
51.8
8.7972
8.8514
0.2575
-f- O.64
7.20
9 2239
8 59
16.0
14.2
16.7
15-2
I 5-52
44.2
8.8549
8.8877
9 2374
9 1
27.1
27.4
2 7.2
26.0
26.92
46.7
9 - 3 ii 7
9-3505
6 2265
9 3
20.5
16.7
18.8
16.5
18.12
47-4
8-9855
9.0262
0.0827
-j- 0.21
6.77
5 2301
9 5
27.6
25-7
274
26.0
26.68
49.0
9-3045
9-3497
0.2408
O.60
5-96
6 2301
9 8
20.4
18.1
18.9
15-2
18.15
48.4
8.9869
9.0303
0.0786
-J- 0.20
6.76
7 2289
9 IO
22.6
20.6
23-7
21-5
22.10
47-3
9.1509
9.1913
0.0824
— 0.21
6.35
9 2344
9 12
17.7
17-3
19.7
17.6
18.08
44-9
8.9837
9.0181
0.0908
+ 0.23
6.79
9 2351
9 i 3
30-4
28.8
29-3
26.1
28.65
45 - 1
9 - 36 i 5
9.3963
0.2874
1
p
tO
5-84
9 2374
9 16
29-3
25-7
27.7
26.0
27.18
45-7
9 - 3 I 94
9-3557
9 2239
9 19
15.8
i 3 -i
15-3
14.6
I4.7O
43-5
8.8088
8.8400
Mittel aus den Yergleichsternbeobachtungen: 9.1098; 9.1191; 9.0979. Zur Reduction benutzt: 9.1089.
Zone 546. 1892 März 9.
Beobachter: Kempf. Photometer: D. Vergleichsterne: Nr. 18 und Nr. 20. Luft: 2
3 -
0
0
00
00
9I1 2 7 m
2 1 ?o
18?o
1984
i8? 4
I9?20
4386
9.0340
9.0654
9 2239
9 30
16.6
154
17.0
14.6
15.90
43-4
8.8754
8.9064
11 1830
9 32
254
24.0
23-9
234
24.18
44 -o
9.2247
9.2570
0.2843
— 0.71
6.24
10 1816
9 35
19-3
16.5
17.7
16.0
17-38
44-4
8.9505
8.9837
0.01 IO
— 0.03
6.92
11 1874
9 37
13-7
12.4
14.0
12.0
13.02
42.9
8.7055
8-7354
0-2373
+ 0.59
7-54
13 1940
9 39
24.6
24.4
25-9
21.4
24.08
4 i -3
9.2213
9.2481
0.2754
— 0.69
6.26
14 1899
9 4 i
25-5
27.9
26.5
23.0
25.72
40.9
9.2749
9.3009
0.3282
— 0.82
6.13
15 1842
9 43
14.7
14.0
14.8
13.0
14. I 2
39-8
8.7746
8.7987
0.1740
+ 0.44
7-39
10 1818
9 45
19.0
18.6
20.6
17.8
I9.OO
44.8
9-0253
9.0594
9 2239
9 47
1 7-5
14-3
16.9
134
I 5-52
43-3
8.8549
8.8857
17 1836
9 50
16.0
15.0
16.5
15-5
15-75
39-2
8.8674
8.8904
0.0823
+ 0.21
7.16
17 1842
9 5 i
24.0
23.0
24.0
.20.5
22.88
39-3
9-1795
9.2027
0.2300
— 0.58
6-37
18 1930
9 53
254
254
27.0
24.0
25-45
38.6
9.2664
9.2885
0.3158
— 0.79
6.16
18 1963
9 55
36.6
364
37-7
32-5
35 - 8 o
38.2
9-5342
9-5556
0.5829
—1.46
5-49
19 2027
9 57
23.6
21.1
22.5
20.4
21.90
37-6
9-1434
9.1639
0.1912
— 0.48
6.47
15 1851
9 59
22.0
21.4
21.8
20.4
21.40
40.7
9-1243
9.1500
0.1773
— 0.44
6.51
10 1818
10 2
21.0
18.5
19-5
17-5
19.12
46.1
9.0306
9.0679
9 2239
10 4
16.4
13-3
15-5 1
144
14.90
43-5
8.8203
8.8515
Mittel aus den Yergleichsternbeobachtungen: 8.9859; 8.9726; 8.9597.
Zur Reduction benutzt: 8.9727.
