Evolution of Superhumps in V466 And: A New WZ Sge-Type Object

Details Evolution of Superhumps in V466 And: A New WZ Sge-Type Object Evolution of Superhumps in V466 And: A New WZ Sge-Type Object

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1314..208c&link_type=abstract

INTERNATIONAL CONFERENCE ON BINARIES: In celebration of Ron Webbink's 65th Birthday. AIP Conference Proceedings, Volume 1314, p

Other

Photometry, White Dwarfs, Novae, Brightness, Photometric, Polarimetric, And Spectroscopic Instrumentation, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification

Scientific paper

Time series analysis of multicolour CCD photometry of a new WZ Sge-type dwarf nova V466 And, discovered during its superoutburst in September 2008, revealed the early superhumps, with the period 0.056383 d in the first 11 days, the ordinary superhumps with the period 0.05713 d in the days 13-23 and late superhumps, with unstable period of about 0.056 d in the days 24-33 of the superoutburst. Thereafter, the dwarf nova returned to its pre-outburst state.

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