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1995BaltA...4..413O - Baltic Astronomy, 4, 413-421 (1995/November-0)
The AM CVn trial: the case for superhumps.
O'DONOGHUE D.
Abstract (from CDS):
The AM CVn stars are hydrogen deficient stars which are explained by an interacting binary white dwarf model. In this model, a low mass white dwarf fills its Roche lobe and transfers He-rich material to another white dwarf via an accretion disk. This paper advances a superhump mechanism to explain the photometric oscillations seen in the light curves of these stars.
Abstract Copyright: ∼
Journal keyword(s): stars: cataclysmic variables - stars: individual: AM CVn
Simbad objects: 6
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