On the Masses of the Secondary Stars in CVs

Details On the Masses of the Secondary Stars in CVs On the Masses of the Secondary Stars in CVs

2001-09-25

arxiv.org/abs/astro-ph/0109440v1

Astronomy and Astrophysics

Astrophysics

To appear in the proceedings of The Physics of Cataclysmic Variables and Related Objects, Goettingen, Germany

Scientific paper

Recent theoretical efforts have made predictions for the masses of the
secondary stars in cataclysmic variables. Accurate observational determinations
for M$_2$ are sparse and typically have uncertainties near $\pm$0.1M$_{\odot}$.
How well do theory and observation agree?

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