On the Masses of the Secondary Stars in CVs
arXiv:astro-ph/0109440
Abstract
Recent theoretical efforts have made predictions for the masses of the secondary stars in cataclysmic variables. Accurate observational determinations for M are sparse and typically have uncertainties near 0.1M. How well do theory and observation agree?
To appear in the proceedings of The Physics of Cataclysmic Variables and Related Objects, Goettingen, Germany