144 
Müller und Kempf, Photometrische Durchmusterung 
144 
B.D. 
Sternzeit 
1 
II 
! HI 
IV 
/ 
1 
2 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
1 log. 
Diff. in 
Grössen 
Grösse 
ii° 
632 
5t 0 m 
I 7 °I 
i6?o 
1787 
I 6?2 
1 687 5 
458 o 
8.9194 
8.9540 
IO 
818 
6 
2 
2 Ó.O 
28.0 
29.2 
28.3 
27.88 
42.8 
9-3398 
9-3695 
o 
893 
6 
4 
19.7 
21.3 
24-5 
21.1 
21.65 
54-4 
9-1339 
9.1981 
0.0279 
— 0.07 
6.38 
5 
769 
6 
6 
16.5 
16.5 
18.0 
154 
16.60 
49-7 
8.9118 
8 - 959 1 
0.2111 
+ O.53 
6.98 
7 
759 
6 
7 
18.5 
17-5 
20.6 
20.0 
19-15 
! 47-4 
9.0319 
9.0726 
0.0976 
— J— 0.24 
6.69 
i 
857 
6 
9 
13.6 
I 4-7 
15-0 
16.O 
14.82 
53-6 
8.8157 
8.8766 
0.2936 
+ 0.73 
7.18 
3 
736 
6 
12 
I4.O 
12.7 
12.6 
12.7 
13.00 
51-4 
8.7042 
8.7570 
0.4132 
4 - 1.03 
7.48 
3 
737 
6 
13 
15.6 
15-7 
16.9 
15-3 
15.88 
51-5 
8.8743 
8.9274 
0.2428 
+ 0.61 
7.06 
4 
811 
6 
14 
l6.2 
16.0 
18.2 
16.5 
16.72 
50.7 
8 - 9 1 79 
8.9683 
0.2019 
+ 0.50 
6-95 
o 
923 
6 
16 
23-4 
24.1 
244 
234 
23.82 
54-4 
9.2125 
9.2767 
0.1065 
— 0.27 
6.18 
11 
632 
6 
19 
I5.6 
16.3 
16.7 
17.0 
16.40 
46.7 
8.9015 
8.9403 
IO 
818 
6 
20 
31-3 
28.5 
28.4 
27-5 
28.92 
1 43-5 
9.3689 
9.4001 
Mittel aus den Vergleich sternbeobachtun "e 
n: 9.1786; 9.1618; 9.1702. 
Zur Reduction benutzt: 9.1702. 
Zone 47 
. 1887 Januar 16. 
Beobachter: 
Kempf. 
Photometer 
D. Vergleichsterne: Nr. 6 
und Nr. 
8. Luft: 
2. 
8° 
385 
2 1 
l 4 Ó m 
2785 
30? 6 
3284 
3389 
3i?io 
4385 
9.4262 
9-4574 
9 
472 
2 
50 
19.6 
19.O 
21-5 
19.5 
19.90 
43-7 
9.0639 
9-0955 
5 
420 
2 
52 
18.2 
194 
2 I .O 
18.0 
I 9 -I 5 
46.7 
9.0319 
9.0707 
O.1944 
+ 0.49 
7-35 
7 
450 
2 
54 
324 
32.5 
30.0 
2 9-5 
31.10 
44-5 
9.4262 
9.4596 
O.1945 
— 0.49 
6-37 
o 
D 
410 
2 
57 
28.4 
29-5 
334 
34 -o 
31-32 
48.4 
9-4317 
9-4752 
0.2 IOI 
— 0.53 
6-33 
i 
517 
2 
59 
17.0 
16.2 
20.0 
17-3 
1 7.62 
50.7 
8.9620 
9.0124 
O.2527 
+ 0.63 
7-49 
4 
485 
3 
2 
28.7 
27-5 
30.1 
28.7 
28.75 
47-5 
9-3643 
9.4052 
O.I4OI 
— 0.35 
6.51 
3 
420 
3 
5 
35-9 
34-0 
394 
37-5 
36.70 
48.5 
9-5529 
9.5966 
0.3315 
— 0.83 
6.03 
8 
385 
3 
8 
29-5 
28.5 
31.6 
33 -o 
30.65 
44-3 
9.4148 
9.4478 
9 
472 
3 
IO 
18.0 
20.0 
21.0 
18.5 
19.38 
42.9 
9.0418 
9.0717 
5 
443 
3 
14 
23.1 
20.2 
23.6 
25.0 
22.98 
46.7 
9 -! 83 1 
9.2219 
O.O432 
+ 0.11 
6.97 
i 
534 
3 
16 
324 
35-9 
31-3 
30.5 
32.52 
5 1 - 1 
9.4609 
9.5126 
O.2475 
— 0.62 
6.24 
9 
397 
3 
18 
14.4 
13-9 
134 
13.0 
13.68 
43 -o 
8-7477 
8.7778 
O.4873 
+ 1.22 
8.08 
7 
478 
3 
21 
28.2 
26.3 
27.2 
27.6 
27.32 
44-5 
9.3236 
9 - 357 ° 
O.O919 
— 0.23 
6.63 
9 
408 
3 
23 
21.8 
22.6 
21.0 
21.7 
21.78 
42.9 
9- 1 388 
9.1687 
O.O964 
+ 0.24 
7.10 
i 
561 
3 
26 
234 
19.0 
24.0 
20.7 
21.78 
50.7 
9 -Ì 388 
9.1892 
0.0759 
+ 0.19 
7-05 
8 
385 
3 
32 
33-8 
3 1 *5 
36.0 
31.8 
33-28 
45-5 
9.4787 
9-5145 
9 
472 
3 
34 
18.6 
17.0 
19.4 
16.5 
17.88 
42.7 
8-9744 
9.0039 
Mittel aus den Vergleichsternbeobachtungen: 9.2765; 9.2597; 9.2592. 
Zur Reduction benutzt: 9.2651 
Zone 48 
1887 Januar 16. 
Beobachter: 
Müller. 
Photometer : 
D. Vergleichsterne: Nr. 6 
und Nr. 8. Luft: 3. 
9 ° 
472 
3 11 
39 m 
1385 
I 2?6 
1387 
I 2?4 
13805 
4287 
8.7075 
8.7370 
8 
385 
3 
43 
24.6 
26.6 
23.8 
26.9 
25.48 
46.4 
9.2674 
9 - 3°54 
6 
496 
3 
45 
32.7 
33*8 
31-5 
34-3 
33 -o 8 
46.8 
9.4740 
9 - 5 i 3 i 
O.4567 
— 1.14 
5.72 
6 
508 
3 
48 
144 
17.7 
16.4 
16.4 
16.22 
46.6 
8.8922 
8.9308 
O.I256 
+ 0.31 
7.17 
7 
493 
3 
51 
11.0 
10.9 
il.6 
14.2 
11.92 
45-9 
8.6300 
8.6668 
O.3896 
+ 0.97 
7-83 
3 
461 
3 
56 
28.9 
28.6 
29.6 
28.6 
28.92 
49.9 
9.3689 
9.4168 
O.3604 
— 0.90 
5-96 
o 
581 
3 
58 
18.0 
21.1 
20.7 
20.6 
20.10 
52.6 
9.0723 
9.1294 
O.O73O 
— 0.18 
6.68 
i 
597 
4 
1 
10.5 
14-3 
12.6 
12.6 
12.50 
51-2 
8.6707 
8.7228 
0.3336 
+ 0.83 
7.69 
8 
385 
4 
3 
24.7 
26.4 
24.4 
27.6 
25-78 
47-9 
9.2768 
9.3188 
9 
472 
4 
6 
11.7 
16.0 
14-3 
14-5 
14.12 
43 -i 
8.7746 
8.8049 
5 
495 
4 
8 
154 
16.8 
14.4 
15.8 
15.60 
47.8 
8.8592 
8.9010 
0.1554 
+ 0.39 
7-25 
2 
552 
4 
IO 
19.2 
20.5 
18.4 
22.6 
20.18 
50.4 
9.0756 
9.1251 
O.0687 
— 0.17 
6.69 
9 
447 
4 
12 
16.4 
16.3 
18.3 
15-7 
16.68 
43-4 
8.9159 
8.9469 
O.IO95 
+ 0.27 
7-13 
5 
502 
4 
13 i 
26.2 
28.6 
31-5 
28.3 
28.65 
47.6 
9-3615 
9.4027 
0.3463 
— 0.87 
5-99 
8 
528 
4 
15 
32.2 
29.9 
28.5 
32.1 
30.68 
44-5 
9.4156 
9.4490 
O.3926 
— 0.98 
5-88 
5 
5 11 
4 
16 
20.1 
21.3 
19.0 
21-5 
20.48 
47-3 
9.0879 
9.1283 
O.O719 
— 0.18 
6.68 
8 
385 
4 
18 
254 
25.6 
25-9 
274 
26.08 
49.2 
9.2862 
9.3320 
9 
472 
4 
2! 
14.6 
14.0 
14.2 
16.0 
14.70 
43-7 
8.8088 
8.8404 
Mittel aus den Vergleichsternbeobachtungen: 9.0212; 9.06x9; 9.0862. Zur Reduction benutzt: 9.0564. 
Beobachtungen erschwert durch ausserordentliche Unruhe der Luft.