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Paper: On the masses of the secondary stars in CVs
Volume: 261, The Physics of Cataclysmic Variables and Related Objects
Page: 59
Authors: Howell, S. B.
Abstract: Recent theoretical efforts have made predictions for the masses of the secondary stars in cataclysmic variables. Accurate observational determinations for M2 are sparse and typically have uncertainties near +/- 0.1 Modot. How well do theory and observation agree? SBH acknowledges partial support for this research from NSF grant AST 98-19770 and NASA Theory grant NAG5-8500.
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