Post-outburst rebrightening in WZ Sge stars

Details Post-outburst rebrightening in WZ Sge stars Post-outburst rebrightening in WZ Sge stars

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..521o&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

1

Scientific paper

WZ Sge-type dwarf novae often exhibit reflares after the end of the main outbursts. In particular, one of WZ Sge stars, EG Cnc, exhibited six consecutive mini-outbursts. Most unusual was that the star abruptly entered into a deep faint minimum after such frantic activities. We propose that this peculiar phenomenon may be understood in terms of viscosity decay in the cold disk.

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