Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-03-11
Astronomy and Astrophysics
Astrophysics
9 pages, 8 figures. Accepted for publication in PASJ
Scientific paper
After 10 years of quiescence, HV Vir underwent a superoutburst in January 2002. We report time-series observations clearly revealing the period change of ordinary superhumps during the superoutburst. We derived a mean superhump period of 0.058260 d and a positive period derivative of $7 \times 10^{-5}$. These results are in good agreement with the value obtained from the 1992 superoutburst. We also detected early superhumps, which were not clearly recognized in the past outburst, and a possible rebrightening. Both of them are the common characteristics of WZ Sge-type stars.
Cook Lewis M.
Ishioka Ryoko
Kato Taichi
Kinugasa Kenzo
Kiyota Seiichiro
No associations
LandOfFree
Period change of Superhumps in the WZ Sge-Type Dwarf Nova, HV Virginis does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Period change of Superhumps in the WZ Sge-Type Dwarf Nova, HV Virginis, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Period change of Superhumps in the WZ Sge-Type Dwarf Nova, HV Virginis will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-131097