2013PASJ...65...50O


Query : 2013PASJ...65...50O

2013PASJ...65...50O - Publ. Astron. Soc. Jap., 65, 50-50 (2013)

The cause of the superoutburst in SU UMa stars is finally revealed by Kepler light curve of V1504 Cygni.

OSAKI Y. and KATO T.

Journal keyword(s):

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 V* VW Hyi CV* 04 09 11.3967378648 -71 17 41.554528260   12.786 12.543 14.160   DQ 661 0
2 V* SU UMa CV* 08 12 28.2695986944 +62 36 22.427676396           B2 516 0
3 V* ER UMa CV* 09 47 11.9410111200 +51 54 08.950092804 14.351 14.03 13.91 14.909 14.629 ~ 161 0
4 V* OY Car CV* 10 06 22.0793274312 -70 14 04.584660540           ~ 586 0
5 V* V436 Cen CV* 11 14 00.0568720872 -37 40 47.763655572           ~ 148 0
6 V* QZ Vir CV* 11 38 26.8241432424 +03 22 07.110298596     15.81     ~ 269 1
7 V* V344 Lyr CV* 18 44 39.1748179896 +43 22 28.051269960           sdB 114 0
8 V* V1504 Cyg CV* 19 28 56.4508657536 +43 05 37.081595940           ~ 122 0
9 V* V503 Cyg CV* 20 27 17.3992939944 +43 41 22.504607556           ~ 138 0

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