344 
Müller und Kempf, Photometrische Durchmusterung 
344 
B.D. 
Sternzeit 
I 
II 
III 
IV 
/ 
z 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
IQ° 
2 ig8 
7 Ъ 
i 9 m 
1488 
I 2?6 
1584 
1385 
14808 
3988 
8.7722 
8.7963 
0.1265 
4 0.32 
7.27 
IO 
1818 
7 
21 
20.4 
17.6 
18.4 
15-5 
17.98 
44.0 
8.9791 
9.0114 
9 
2239 
7 
24 
14-5 
12.8 
14-5 
13-5 
13.82 
51-5 
8.7563 
8.8094 
i 7 
2078 
7 
26 
23-5 
19-7 
20.5 
22.0 
21.42 
41.8 
9-1251 
9.1528 
0.2300 
— 0.58 
6-37 
i 7 
2065 
7 
28 
15-5 
14.0 
16.0 
14.4 
14.98 
41.i 
8.8249 
8.8513 
0.0715 
0 .18 
7-13 
i 5 
2027 
7 
29 
18.5 
1 5 -i 
18.2 
15.0 
16.70 
42.2 
8.9169 
8.9454 
0.0226 
— 0.06 
6.89 
i 3 
2074 
7 
31 
19.6 
18.0 
18.2 
17.7 
18.38 
44.0 
8.9975 
9.0298 
0.1070 
— 0.27 
6.68 
12 
2009 
7 
33 
20.2 
17-5 
19-5 
18.4 
18.90 
45 -o 
9.0209 
9-0555 
0.1327 
— 0-33 
6.62 
IO 
1972 
7 
34 
15-5 
12.8 
14-5 
14.0 
14.20 
46.7 
8.7794 
8.8182 
0.1046 
-f- 0.26 
7.21 
IO 
1818 
7 Зб 
19.9 
17-5 
18.0 
16.5 
17.98 
43 -i 
8.9791 
9.0094 
9 
2239 
7 
38 
14.2 
13.6 
14.8 
13-9 
14.12 
50.1 
8.7746 
8.8231 
Mittel aus den 
Vcrglcichsternbcobachtungen: 8.9417; 8.9104; 8.9162. Zur Reduction benutzt: 8.9228. 
Zone 550. 1892 März 17. 
Beobachter: Müller. Photometer: D 
. Yergleichsterne: Nr. 20 und Nr. 22. Luft: 2 
3 - 
9 ° 
2239 
7 h 
42 ю 
I 5?2 
1389 
14?o 
1383 
14810 
4987 
8.7734 
8.8207 
9 
2374 
7 
45 
26.2 
22.0 
23.1 
22.3 
2340 
54-4 
9.1979 
9.2620 
13 
2237 
7 
48 
13.6 
12.7 
14-5 
ii -5 
13.08 
48.7 
8.7094 
8-7537 
0.2950 
4- 0.74 
7-30 
18 
2338 
7 
50 
I 7.0 
16.4 
17.6 
16.0 
16.75 
43-7 
8.9194 
8-95 ю 
0.0977 
4 0.24 
6.80 
18 
2345 
7 
5 i 
15-7 
14.2 
16.5 
13.8 
1 5-°5 
44.0 
8.8288 
8.8611 
0.1876 
4 0.47 
7-°3 
18 
2352 
7 
52 
11.9 
8.7 
10.6 
10. i 
ю.32 
44.4 
8.5064 
8.5396 
0.5091 
4 1.27 
7-83 
i 7 
2224 
7 
54 
12.4 
11.8 
14.0 
13.0 
12.80 
45 -o 
8.6909 
8-7255 
0.3232 
+ 0.81 
7-37 
16 
2122 
7 
56 
11.8 
7.8 
10.4 
9.0 
9-75 
46.1 
8.4576 
8.4949 
0.5538 
4 1.38 
7-94 
9 
2374 
7 
58 
26.3 
21.5 
23-7 
22.8 
23-58 
52-9 
9.2042 
9.2624 
9 
2239 
8 
о 
15-5 
13-3 
14-5 
12.6 
13.98 
48.0 
8.7662 
8.8085 
16 
2098 
8 
3 
15-4 
12.7 
144 
13.6 
14.02 
43-5 
8.7686 
8.7998 
0.2489 
-|- 0.62 
7.18 
i 5 
2 I92 
8 
6 
22.6 
21.6 
21.4 
19.8 
2 i -35 
44.9 
9.1224 
9.1568 
0.1081 
— 0.27 
6.2g 
16 
2Il6 
8 
7 
13-9 
12.i 
12.i 
11.7 
12.45 
44.6 
8.6673 
8.7010 
0-3477 
—f- 0.87 
7-43 
11 
2217 
8 
9 
17.4 
14.8 
1 7-5 
144 
16.02 
48.9 
8.8817 
8.9266 
0.1221 
4 0.31 
6.87 
12 
22 I I 
8 
11 
17.6 
15-3 
17-5 
16.0 
16.60 
48-3 
8.9118 
8.9550 
0.0937 
4 0.23 
6.79 
IO 
2152 
8 
13 
23.8 
23.0 
22.3 
22.0 
22.78 
49-5 
9-1759 
9.2226 
O.I 739 
— 0.43 
6.13 
9 
2374 
8 
15 
24.7 
25.6 
26.5 
24.6 
25-35 
51.0 
9.2632 
9.3146 
9 
2239 
8 
18 
14.6 
1 3 -1 
1 5-9 
13.6 
14.30 
46.5 
8.7854 
8.8237 
Mittel aus den 
Vergleichsternbeobachtungen: 9.0414; 9.0354; 9.0692. 
Zur Reduction benutzt: 9.0487. 
Zone 551. 1892 März 17. 
Beobachter: Müller. 
Photometer: 
D. Yergleichsterne : Nr. 22 
und Nr. 24. Luft: 
2. 
9 ‘ 
2374 
9 
40 m 
3183 
2986 
2988 
2684 
29828 
4483 
9.3788 
9.4118 
11 
2372 
9 
43 
18.3 
16.8 
19.8 
16.6 
17.88 
46.0 
8.9744 
9.0114 
2 
2387 
9 
45 
27.7 
27.0 
28.4 
26.5 
27.40 
52.2 
9-3259 
9 - 38 I 5 
0.1502 
— 0.38 
6.02 
3 
2475 
9 
48 
18.1 
15.0 
16.4 
1 5-7 
16.30 
52.2 
8.8964 
8.9520 
0.2793 
4 0.70 
7.10 
2 
2411 
9 
50 
254 
26.0 
25-1 
25-8 
25-58 
53 -o 
9.2705 
9.3291 
0.0978 
— 0.24 
6.16 
О 
2782 
9 
52 
24-5 
24.1 
23.1 
22.3 
23 - 5 ° 
54-7 
9.2014 
9.2668 
0.0355 
— 0.09 
6.31 
2 
2418 
9 
54 
30-7 
З ь 5 
31-7 
29.0 
30.72 
53-4 
9.4166 
9.4767 
0.2454 
— 0.61 
5-79 
4 
2461 
9 
56 
17.9 
14.9 
15.О 
14.4 
1 5 - 5 5 
51-5 
8.8565 
8.9096 
0.3217 
+ 0.80 
7.20 
4 
2463 
9 
58 
21.0 
21.2 
2 1.0 
20.6 
20.95 
50.8 
9.1067 
9- I 574 
0.0739 
4- 0.18 
6.58 
9 
2374 
10 
0 
30.5 
27.4 
28.3 
26.6 
28.20 
43-6 
9.3489 
9.3803 
11 
2372 
10 
2 
19.0 
17.9 
19.6 
17.8 
18.58 
44.4 
9.0066 
9.0398 
11 
2376 
IO 
3 
18.9 
18.0 
20-4 
18.4 
18.92 
44.2 
9.0218 
9.0546 
0.1767 
40.44 
6.84 
8 
2476 
IO 
6 
29.8 
27.8 
26.6 
26.2 
27.60 
45-6 
9-3317 
9.3677 
0.1364 
— 0.34 
6.06 
7 
2440 
IO 
9 
19.7 
16.4 
I9.2 
16.8 
18.02 
47.2 
8.9809 
9.0210 
0.2103 
4 0.53 
6-93 
7 
2443 
IO 
10 
17.9 
16.1 
18.5 
16.2 
17.18 
47-3 
8.9407 
8.9811 
0.2502 
40.63 
7-03 
9 
2482 
IO 
12 
20.6 
16.8 
20.0 
18.9 
19.08 
44-5 
9.0288 
9.0622 
0.1691 
■— |— О.42 
6.82 
9 
2494 
IO 
4 
2 1.1 
18.7 
18.7 
19.7 
19-55 
45-2 
9.0492 
9.0843 
0.1470 
40.37 
6-77 
9 
2374 
IO 
*5 
32.0 
30.1 
З2.3 
29.4 
30-95 
43-3 
9.4225 
9-4533 
11 
2372 
IO 
18 
21.4 
18.5 
20-4 
19.0 
19.82 
43-2 
9.0605 
9.0910 
Mittel aus den Yergleichsternbeobachtungen: 9.2116; 9.2101; 9.2721. Zur Reduction benutzt: 9.2313.