The implications of disc instabilities on cataclysmic variable structure and evolution

Details The implications of disc instabilities on cataclysmic variable structure and evolution The implications of disc instabilities on cataclysmic variable structure and evolution

2004-02-09

arxiv.org/abs/astro-ph/0402190v1

Astronomy and Astrophysics

Astrophysics

To appear in: Compact Binaries in the Galaxy and Beyond, IAU Coll. 194, editors E. Sion and G. Tovmassian

Scientific paper

Applications of the thermal-viscous disc instability model to various classes
of cataclysmic variable very often require the accretion disc to be truncated.
I argue that in most cases this inner truncation must be due to the white
dwarf's magnetic field.

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