152 153 Zone o° bis -j- 20° Declination. 153 
Grösse 
BD. 
Sternzeit 
! 
I 
II 
III 
IV 
J 
z 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
Diff. in 
Grössen 
Grösse 
ii° 
1588 
7 11 54 ,n 
20?8 
20?4 
2 2?5 
ig?o 
2 o 968 
4 i?8 
9.0959 
9.1236 
5 
1380 
7 56 
13-5 
13-9 
I7.7 
14.7 
14-95 
49.1 
8.8232 
8.8687 
0.3682 
+ o.g2 
7-39 
4 
1414 
7 57 
27.4 
30.0 
27*5 
25.0 
27.48 
5 1-1 
9.3282 
9-3799 
0.1430 
— 0.36 
6.11 
9 
i 37 6 
7 59 
18.2 
17.0 
20.5 
17-3 
18.25 
45-5 
8.9915 
9.0273 
o.2og6 
+ 0.52 
6.99 
7-75 
8 
i486 
8 0 
27-3 
25-5 
27.7 
26.2 
26.68 
46.6 
9-3045 
9-3431 
0.1062 
— 0.27 
6.20 
7.67 
9 
1393 
8 2 
1 7.6 
15-4 
I7.6 
16.4 
i 6.75 
4 Ó -3 
8 .gig 4 
8.9572 
o- 2 7 g 7 
+ 0.70 
7.17 
8.02 
1 
1 53 1 
8 3 
23.2 
24.4 
24.2 
22.3 
23-52 
53-9 
g.2021 
g.2642 
0.0273 
— 0.07 
6.40 
6.70 
10 
1149 
8 5 
27.6 
24-3 
26.3 
24.2 
25.60 
46.8 
g.2711 
9.3102 
7.00 
11 
1588 
8 7 
21.5 
20.4 
21.1 
20.5 
20.88 
42.3 
9.1039 
9.1326 
6.40 
Mittel aus den Vcrgleichsternbeobachtungen: 9.2658; 9.2234; 9.2214. Zur Keduction benutzt: 9.2369. 
*) 9 0 1345 dupl. Zuerst die hellere, südlich folgende Componente gemessen. Messungen 
sehr unsicher. 
Zone 70 
. 1887 Februar i. 
7.41 
Beobachter: Kempf. 
Photometer: 
D. Vergleichsterne: Nr. 10 und Nr. 12. Luft: 
3 - 
6.41 
11° 
632 
3^3 2 m 
2 2?I 
23-5 
23% 
2 2?0 
2 2?8o 
4288 
g.i 766 
g.2063 
7-85 
IO 
818 
3 35 
43-5 
47.6 
404 
37-9 
42.38 
48.1 
9-6574 
g.7000 
7.24 
qqa( 
3 39 
25-5 
23-5 
30.0 
21.3 
25.08 
53-4 
9-2545 
9 - 3 I 47 
0.1161 
+ 0.2g 
6-74 
6.68 
) 1 
3 41 
15-0 
14.9 
15.2 
13-1 
14-55 
53-3 
8.8001 
8.85gg 
0.5709 
+ i -43 
7.88 
8.18 
7 
778 
3 47 
23.0 
21.8 
21.5 
20.0 
21.58 
47.2 
9-1312 
9 -i 7 i 3 
0.2595 
+ 0.65 
7.10 
6 
81g 
3 49 
16.4 
16.5 
16.2 
15.2 
16.08 
48.0 
8.884g 
8^272 
0.5036 
+ 1.26 
7.71 
7 
787 
3 51 
20.3 
18.4 
18.8 
18.6 
ig.02 
46.7 
g.0262 
g.0650 
0.3658 
+ 0.91 
7-36 
8 
852 
3 53 
16.6 
17-5 
18.7 
17.0 
17-45 
45-6 
8-9539 
8.g8gg 
0.440g 
-f- 1.10 
7-55 
**) 0 
939 
3 55 
40.0 
344 
35 -o 
31.2 
35-15 
53-2 
9.5204 
9-5798 
o.i4go 
— 0.37 
6.08 
11 
632 
3 57 
24.7 
23-5 
25.0 
22.5 
23.92 
41.7 
9.2159 
9.2434 
IO 
818 
3 59 
38.5 
42.4 
40.4 
40.4 
40.42 
45-9 
9.6237 
g.6605 
9 
736 
4 i 
28.6 
2g.6 
314 
28.2 
29-45 
44.8 
9-3834 
9-4175 
0.0133 
+ 0.03 
6.48 
9 
743 
4 3 
42.6 
41-3 
47-5 
40-5 
42.g8 
44.4 
9.6673 
9.7005 
o.26g7 
— 0.67 
5.78 
c (Sö 
7 
812 
4 4 
26.4 
24.2 
25.0 
24-5 
25.02 
46.2 
9-2525 
g.2goo 
0.1408 
+ 0.35 
6.80 
6 
3 
785 
4 7 
23.1 
22.1 
25.6 
25.0 
23-95 
50.6 
g.2i6g 
g.2670 
0.1638 
+ 0.41 
6.86 
U.Uj 
6 
864 
4 9 
15.6 
15-5 
15.6 
15-5 
15-55 
47.2 
8.8565 
8.8g66 
0.5342 
+ i -34 
7-79 
6 78 
0 
975 
4 IO 
40.0 
34 -o 
33-9 
33 -o 
35-22 
52.8 
9.5219 
9-5798 
0. i4go 
— 0.37 
6.08 
11 
632 
4 12 
23-5 
22.6 
22.g 
21.0 
22.50 
41-3 
9 -i 657 
9.1925 
0.7g 
IO 
818 
4 15 
33 -i 
36.5 
374 
38.8 
3645 
44.8 
9-5478 
9.5819 
Mittel aus den Vergleichsternbeobachtungen: 9.4532; 9.4519; 9.3872. 
Zur Keduction benutzt: 9.4308. 
*) x°886 dupl. Zuerst die südlich vorangehende Componente gemessen. 
6.go 
**) o° 939 . 
Die röthliche Farbe erschwert die Messungen. 
7.28 
Zone 71. 
1887 Februar 5. 
7.07 
Beobachter: 
Müller. 
Photometer: 
D. Vergleichsterne: Nr. 6 und Nr. 8. Luft: 2. 
7.07 
8 ( 
385 
3 h 57 m 
3086 
2588 
2 8?7 
24?6 
27842 
4782 
9-3265 
g .3666 
7.02 
9 
472 
4 0 
18.3 
16.3 
I 7.0 
15.0 
16.65 
43 -o 
8 .gi 44 
8-9445 
6.13 
1 ' 
11 
335 
4 2 
1 5 -1 
13.6 
16.4 
13-1 
14-55 
45-8 
8.8001 
8.8366 
0.3226 
+ 0.81 
7.67 
16 
293 
4 4 
17.4 
* 5 -i 
16.6 
15-7 
16.20 
41.6 
8.8gi2 
8.9185 
0.2407 
+ 0.60 
7.46 
J 9 
365 
4 6 
25-9 
27-5 
28.8 
25-5 
26.g2 
38.5 
9 - 3 ii 7 
9-3336 
0.1744 
— 0.44 
642 
17 
380 
4 8 
27.4 
254 
27.1 
234 
25.82 
40.6 
g.2780 
9-3035 
0.1443 
— 0.36 
6.50 
14 
419 
4 9 
32-5 
25-7 
2 8.6 
28.3 
28.78 
42.9 
9-3651 
9-3950 
0.2358 
— 0.59 
6.27 
18 
325 
4 n 
19-3 
18.3 
20.4 
17.2 
18.80 
39-6 
g.0164 
g.0401 
0.1 igi 
+ 0.30 
7.16 
8 
385 
4 13 
26.7 
24.6 
254 
26.7 
25-85 
48.6 
g.27go 
9.3230 
9 
4 T» 2 
4 15 
17.4 
16.5 
19.4 
174 
17.68 
43-4 
8.gÓ4g 
8-9959 
11 
354 
4 17 
14.2 
14.9 
16.7 
134 
14.80 
46.2 
8.8146 
8.8521 
0.3071 
+ 0.77 
7-63 
7.2 2 
IO 
340 
4 18 
19-5 
17-3 
18.8 
16.0 
17.90 
46.9 
8-9753 
g.0146 
0.1446 
0.36 
7.22 
8-37 
13 
411 
4 20 
16.7 
154 
17.6 
15.6 
16.32 
44.8 
8 . 8 g 74 
8.9315 
0.2277 
+ 0.57 
7-43 
6.01 
11 
365 
4 22 
13-7 
12.6 
15.8 
13-7 
13-95 
46.2 
8.7643 
8.8018 
0-3574 
-j- 0.8g 
7-75 
6.67 
19 
394 
4 24 
18.0 
16.7 
19.4 
17-3 
17-85 
39-7 
8.9730 
8.gg6g 
0.1623 
+ 0.41 
7.27 
7-°3 
14 
439 
4 26 
17.6 
15.6 
20.3 
194 
18.20 
44.1 
8.g8g2 
g.0217 
0-1375 
+ 0.34 
7.20 
7-45 
8 
385 
4 28 
28.7 
274 
27.7 
26.1 
27.48 
50.1 
9.3282 
9.3767 
6.36 
9 
472 
4 30 
17.1 
15.6 
17.4 
16.6 
16.68 
44.1 
8.9159 
8^484 
Mittel aus den Vergleichsternbeobachtungen: 9.1556; 9.1594; 9.1626. 
Zur Keduction benutzt: 9.1592.