Time Series Photometry of the Cataclysmic Variable Systems VY Aquarii and V2491 Cygni

Details Time Series Photometry of the Cataclysmic Variable Systems VY Aquarii and V2491 Cygni Time Series Photometry of the Cataclysmic Variable Systems VY Aquarii and V2491 Cygni

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jsara...3...11p&link_type=abstract

Journal of the Southeastern Association for Research in Astronomy, Vol. 3, p. 11-14

Astronomy and Astrophysics

Astronomy

Cataclysmic Variables, Stars: Cataclysmic Variables

Scientific paper

We present an analysis of time-series photometry of the cataclysmic variable systems VY Aquarii and V2491 Cygni. We produced a lightcurve for VY Aquarii during its superoutburst and calculated a superhump period of 92.81 minutes. The decline of the superoutburst was also examined in VY Aquarii. The new classical nova V2491 Cygni was examined. A Fourier analysis revealed no significant periodicity.

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