Hvězda | RA | Dec | Typ | Mo | P | M | m | Obor | D | d |
---|
- | h m s | ° \' | | 2400 000+ | d | mag | mag | | h | h |
CX Aqr |
22 35 44 |
-0 41.5 |
EA |
52500.4293 |
0.5559894 |
10.55 |
11.75 |
V |
2.3 |
0 |
V 346 Aql |
20 09 59 |
10 21.0 |
EA |
52500.7369 |
1.10636139 |
9.0 |
10.1 |
P |
5.0 |
0 |
UW Boo |
14 20 59 |
47 06.7 |
EA |
52500.0435 |
1.0047085 |
10.4 |
11.4 |
P |
3.4 |
|
TU Cnc |
8 52 17 |
9 05.3 |
EA |
52500.619 |
5.561406 |
9.9 |
12.4 |
P |
12 |
0 |
WW Cnc |
9 09 47 |
30 26.8 |
EA |
52500.451 |
1.1159515 |
10.5 |
11.6 |
P |
3.7 |
|
AK CMi |
7 40 16 |
3 57.2 |
EA |
52500.0824 |
0.5658971 |
10.1 |
11.5 |
P |
4.1 |
0 |
RZ Cas |
2 48 56 |
69 38.0 |
EA |
52500.5676 |
1.1952598 |
6.18 |
7.72 |
V |
4.9 |
0-0.5 |
AB Cas |
2 37 32 |
71 18.2 |
EA |
52501.3479 |
1.3668887 |
10.10 |
11.85 |
V |
5.9 |
0 |
U Cep |
1 02 18 |
81 52.5 |
EA |
52502.028 |
2.493096 |
6.75 |
9.24 |
V |
9.0 |
<2.4 |
EG Cep |
20 15 56 |
76 48.6 |
EB |
52500.5221 |
0.5446220 |
9.31 |
10.21 |
V |
2.0 |
0 |
EK Cep |
21 41 21 |
69 41.5 |
EA |
52503.0718 |
4.4277959 |
7.99 |
9.32 |
B |
6.4 |
|
SS Cet |
2 48 36 |
1 45.9 |
EA |
52500.404 |
2.973979 |
9.4 |
13.0 |
V |
9.3 |
1.8 |
V 456 Cyg |
20 28 50 |
39 09.2 |
EA |
52500.7818 |
0.8911956 |
10.8 |
11.9 |
P |
1.7 |
0 |
V 687 Cyg |
19 26 12 |
29 58.7 |
EA |
52500.209 |
1.707227 |
10.2 |
11.4 |
P |
4.1 |
0 |
TY Del |
21 04 22 |
13 13.0 |
EA |
52500.4195 |
1.191124 |
9.7 |
10.9 |
V |
5.7 |
0 |
FZ Del |
20 53 33 |
4 38.8 |
EA |
52500.7928 |
0.783211 |
10.2 |
11.3 |
P |
2.8 |
0 |
RZ Dra |
18 23 06 |
58 54.2 |
EB |
52500.1944 |
0.55087645 |
10.11 |
11.01 |
V |
B |
- |
TW Dra |
15 33 51 |
63 54.4 |
EA |
53558.91888 |
2.80683211 |
8.0 |
10.5 |
P |
11.5 |
1.3 |
AI Dra |
16 56 18 |
52 41.9 |
EA |
52500.9384 |
1.1988188 |
7.05 |
8.09 |
V |
5.2 |
0 |
WX Eri |
3 24 23 |
-0 42.2 |
EA |
52500.6696 |
0.8232720 |
9.38 |
10.28 |
V |
3.8 |
0 |
RW Gem |
6 01 28 |
23 08.4 |
EA |
52502.366 |
2.865505 |
9.53 |
11.76 |
V |
10.3 |
1.4 |
AF Gem |
6 50 34 |
21 22.6 |
EA |
52501.118 |
1.2434989 |
10.54 |
11.83 |
V |
6.0 |
0 |
SZ Her |
17 39 37 |
32 56.7 |
EA |
52500.3773 |
0.8181013 |
9.86 |
11.87 |
V |
3.5 |
|
CM Lac |
22 00 04 |
44 33.1 |
EA |
52500.7920 |
1.60469143 |
8.18 |
9.15 |
V |
4.2 |
0 |
SX Lyn |
8 13 58 |
57 15.9 |
EA |
52501.887 |
2.022475 |
10.0 |
11.4 |
P |
4.9 |
0 |
TZ Lyr |
18 15 50 |
41 06.7 |
EB |
52500.5252 |
0.52882709 |
10.87 |
11.85 |
V |
B |
- |
RW Mon |
6 34 46 |
8 49.6 |
EA |
52501.1776 |
1.9060769 |
9.26 |
11.51 |
V |
6.9 |
1.2 |
BO Mon |
7 59 49 |
-3 28.3 |
EA |
52501.866 |
2.225235 |
10.0 |
12.1 |
V |
8.0 |
0 |
RV Oph |
17 34 35 |
7 14.8 |
EA |
52502.517 |
3.6871194 |
9.42 |
11.44 |
V |
8.8 |
1.3 |
UX Peg |
22 28 36 |
18 01.6 |
EA |
52501.292 |
1.544619 |
10.7 |
12.0 |
P |
5.2 |
0 |
BG Peg |
22 52 47 |
15 39.2 |
EA |
52500.237 |
1.952441 |
10.5 |
11.6 |
V |
5 |
0.5 |
DI Peg |
23 32 15 |
14 58.1 |
EA |
52500.4219 |
0.7118150 |
9.38 |
10.48 |
V |
3.6 |
0 |
RT Per |
3 23 40 |
46 34.5 |
EA |
52500.3551 |
0.84940480 |
10.46 |
11.74 |
V |
3.3 |
0 |
IU Per |
2 59 37 |
43 55.3 |
EA |
52500.215 |
0.857023 |
10.5 |
11.6 |
P |
3.9 |
0 |
β Per |
3 08 10 |
40 57.4 |
EA |
52500.155 |
2.867353 |
2.12 |
3.39 |
V |
9.6 |
0 |
U Sge |
19 18 48 |
19 36.6 |
EA |
52501.8178 |
3.3806091 |
6.45 |
9.28 |
V |
13.8 |
1.5 |
RW Tau |
4 03 54 |
28 07.7 |
EA |
52500.9031 |
2.768752 |
7.98 |
11.59 |
V |
9.3 |
1.3 |
X Tri |
2 00 34 |
27 53.3 |
EA |
52500.7395 |
0.9715224 |
8.55 |
11.27 |
V |
4.2 |
0.3 |
W UMa |
9 43 45 |
55 57.2 |
EW |
52500.1693 |
0.3336347 |
7.75 |
8.48 |
V |
W |
0.3 |
TX UMa |
10 45 20 |
45 34.0 |
EA |
52500.184 |
3.063279 |
7.06 |
8.80 |
V |
8.8 |
0 |
XZ UMa |
9 31 25 |
49 28.1 |
EA |
52501.2009 |
1.2223040 |
10.1 |
11.7 |
P |
2.9 |
0 |
BH Vir |
13 58 25 |
-1 39.7 |
EA |
52500.4626 |
0.8168712 |
9.60 |
10.56 |
V |
3.1 |
0 |
AW Vul |
20 29 00 |
24 48.0 |
EA |
52500.784 |
0.8064507 |
10.8 |
11.9 |
V |
3.9 |
0.4 |
Poznámky k tabulce
U několika hvězd uvedených tabulce byly zaznamenány drobné změny na světelné křivce. Pulsace jedné ze složek jsou dobře patrné u AB Cas. Podobné drobné oscilace, ale zatím nejasného původu jsou u TW Dra. RZ Cas může kromě oscilací, jejichž amplituda se navíc mění, zaujmout i změnami tvaru světelné křivky.
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