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2004MNRAS.349.1505B - Mon. Not. R. Astron. Soc., 349, 1505-1508 (2004/April-3)
Mass-transfer bursts and the superhumps in cataclysmic variables.
BATH G.T.
Abstract (from CDS):
It is suggested that the superhumps in SU UMa stars are generated by a bright region on the red component that rotates asynchronously with the binary period. The bright region would be produced by mass-transfer instability by the red component. A simple experimental illustration of dynamical instability is presented, together with estimates of cooling times after instability.
Abstract Copyright: 2004 RAS
Journal keyword(s): instabilities - binaries: close - stars: dwarf novae - stars: mass-loss - novae, cataclysmic variables
Simbad objects: 4
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