380
Müller und Kempf, Photometrische Durchmusterung
380
B.D.
Sternzeit
I
II
III
IV
/
z
log sin 2 /
corrig. J
für Ext.
Diff.
in log.
Diff. in
Grössen
Grösse
Zusatz-Zone 6.
1803 Januar
II.
Beobachter: Kempf.
Photometer: Ol. Vergleichsterne: Nr. i und Nr. 3.
Luft: 1-
2.
i o°
8
I h 54 m
15-5
I 6?2
1581
i6?4
1 5?8o
4783
8.8700
8.9104
11
96
I 56
14-7
16.2
! 5-7
19.2
16.45
43-7
8.9041
8-9357
IO
5004
1 59
16.0
l6. 5
17.6
17.4
16.88
49.8
8.9259
8-9735
0.036 1
— 0.09
5-63
6
5216
2 1
13-5
II.6
12.0
12.6
12.42
53-2
8.6652
8.7246
0.2 128
+ O.53
6.25
8
5164
2 4
11.2
10.5
10.5
9-5
10.42
5 i-i
8-5147
8.5664
0.3710
+ O.93
6.65
7
5 121
2 6
14.2
144
14.2
15.6
14.60
51-7
8.8030
8.8568
0.0806
+• 0.20
5-92
7
2 7
2 15
ii -5
12.8
11.6
13-5
12-35
51-5
8.6604
8-7135
0.2239
4“ O.56
6.28
o
28
2 20
11.6
11.6
12.5
12.6
12.08
57.8
8.6415
8.7213
0.2 l6l
4~ O.54
6.26
IO
8
2 22
16.4
15-5
16.4
17-5
16.45
50.1
8.9041
8.9526
11
96
2 24
15-5
17.0
16.8
18.5
16.95
45-9
8.9294
8.9662
IO
2 5
2 28
13-5
11.8
13.0
14.4
13.18
49-9
8-7159
8.7638
O.1736
+ 0.43
6.15
7
36
2 3 °
20.0
18.5
17-5
18.3
18.58
52.6
9.0066
9.0637
O.I263
— O.32
5-40
I 2
2 5
2 32
134
11.6
1 1-7
12.0
12.18
47-8
8.6485
8.6903
O.247 I
4 ~ O.Ó 2
6-34
I
57
2 35
14.0
154
16.2
14-3
14.98
58.3
8.8249
8.9073
O.O3OI
4“ O.08
5.80
15
59
2 38
9-5
10.0
9-5
10.0
9-75
45-7
8.4576
8.4939
0.4435
4-I.ii
6.83
18
5 1
2 42
10.6
12.1
10.7
1 1-5
11.22
43-2
8.5782
8.6087
O.3287
4~ 0.82
6-54
IO
8
2 44
154
15-2
16.0
17.2
15-95
52-7
8.8781
8-9356
11
96
2 46
14-5
16.6
15 5
17-5
16.02
48.0
8.8817
8.9240
Mittel aus den Vergleiehsternbe obachtungen: 8.9231; 8.9594; 8.9298.
Zur Reduction benutzt: 8.9374.
Zusatz
-Zone 7.
18Q3 Januar
II.
Beobachter : Müller.
Photometer: Ci. Vergleichsterne: Nr. 5
und Nr. 7
Luft : i
—2.
IO°
252
2 h 59“
i 4?4
i4?o
I4?2
1383
13898
4485
8.7662
8.7996
8
455
3 i
24.8
2 3-7
22.4
21.7
23-15
43-9
9.1891
9.2212
14
419
3 3
134
12.3
12.4
12.4
12.62
38.5
8.6788
8.7007
O.3138
4~ O.78
6-35
6
39 2
3 5
1 5 * 1
134
12.4
134
13-58
46.0
8.7414
8.7784
O.2361
+ 0.59
6.16
6
398
3 7
14-5
13-3
16.0
16.4
15-05
46.7
8.8288
8.8676
O.1469
+ 0.37
5-94
7
402
3 8
12.7
13.0
13-7
13-7
13.28
45-8
8.7223
8.7588
0.2557
+ O.64
6.21
2
406
3 10
11.6
11.2
11.1
10.5
I I.IO
50.0
8.5690
8.6172
0-3973
4 - 0.99
6.56
5
374
3 12
11.6
10.8
10.6
11 -5
11.12
47-3
8-5705
8.6109
0.4036
4- 1.01
6.58
IO
252
3 14
15-3
13.0
12.7
15.0
14.00
45-6
8.7674
8.8034
8
455
3 18
24.1
23-3
22.3
25.2
23.72
44.2
9.2090
9.2418
14
457
3 19
15-5
14.0
13-7
15-3
14.62
38.3
8.8042
8.8258
0.1887
4 - 0.47
6.04
4
437
3 21
10.8
10.9
11.1
11.9
11.18
48.8
8-575 2
8.6198
0-3947
4- 0.99
6.56
17
44 2
3 23
144
12.4
144
15.0
14.05
35-4
8.7704
8.7878
0.2267
4- 0.57
6.14
14
480
3 24
18.0
17.0
14-3
154
16.18
38.5
8.8901
8.9120
0.1025
4- 0.26
5-83
17
457
3 27
13-3
13-7
14.4
14-3
13.92
35-2
8.7624
8.7796
O.2349
+ 0.59
6.16
1 7
458
3 28
16.1
16.1
16.4
16.9
16.38
35-6
8.9005
8.9182
0.0963
4- 0.24
5.81
IO
252
3 30
134
14-5
13-7
12.6
13-55
46.9
8.7396
8.7789
8
455
3 32
22.3
24.0
234
25-1
23.70
44.6
9.2083
9.2420
Mittel aus den Vergleichsternbeobachtungen: 9.0104; 9.0226; 9.0105.
Zur Reduction benutzt: 9.0145
Zusatz-Zone 8.
1893 Januar
II.
Beobachter : Kempf.
Photometer: Ci. Vergleichsterne: Nr. 7 und Nr. 9
Luft : i
-2.
8 C
455
3 u 38 m
2384
2 I?2
2 2 ? I
2485
2 2?8o
4488
9.1766
9.2 107
8
652
3 41
234
24.O
23.O
24.1
23.62
43-7
9.2056
9.2372
7
450
3 43
134
12-5
I 2.4
14-5
13.20
45-7
8.7172
8-7535
0.4483
4- 1.12
6.12
3
410
3 45
134
I3.O
I2.4
12.4
12.80
49.6
8.6909
8-7379
0.4639
4- i. 16
6.16
IO
401
3 47
13.8
12.6
I3.8
16.5
14.18
43-2
8.7782
8.8087
0.3931
4- 0.98
5-98
4
485
3 50
12.0
12.0
IO.5
12.9
11.85
48.8
8.6250
8.6696
0.5322
4 - 1.33
6-33
3
420
3 52
14.6
154
I4.O
16.4
15.10
49.8
8.8316
8.8792
0.3226
4- 0.81
5.81
i
534
3 54
13.2
12.5
13.O
12.5
12.80
52.2
8.6909
8.7465
0.4553
4 - i-14
6.14
