Outburst Properties of V1504 Cyg and V344 Lyr

Authors

  • J. K. Cannizzo 1CRESST, Dept. of Phys., UMBC, Baltimore, MD 21250, USA 2NASA/GSFC/Astroparticle Physics Lab., Greenbelt, MD 20771, USA

DOI:

https://doi.org/10.14311/APP.2015.02.0156

Abstract

I begin by reviewing dwarf novae and the disk instability theory, and then present an overview of three ideas for producing superoutbursts in the SU UMa stars − the thermal tidal instability, irradiation-induced secondary mass overflow, and the plain vanilla disk limit cycle instability. I discuss the properties of the outbursts in two SU UMa systems observed by Kepler in the context of the three theories. I conclude with a look beyond the SU UMa systems.

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Published

2015-02-23

Issue

Vol. 2 No. 1 (2015): THE GOLDEN AGE OF CATACLYSMIC VARIABLES AND RELATED OBJECTS - II

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Articles

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