Modelling of Low-Accretion Rate Polars

Details Modelling of Low-Accretion Rate Polars Modelling of Low-Accretion Rate Polars

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..330..411f&link_type=abstract

The Astrophysics of Cataclysmic Variables and Related Objects, Proceedings of ASP Conference Vol. 330. Edited by J.-M. Hameury a

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Observations of recently discovered AM Herculis systems through the Sloan Digital Sky Survey have uncovered a new class of objects characterized by an extremely low mass transfer rate. In addition, these systems show unusual phase dependent flux and circular polarization variations which are not explicable in terms of the standard cyclotron emission model.

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