On the Masses of the Secondary Stars in CVs

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dc.creatorHowell, S. B.
dc.date2001-09-25
dc.date.accessioned2026-07-07T02:00:16Z
dc.date.available2026-07-07T02:00:16Z
dc.descriptionRecent 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?
dc.descriptionTo appear in the proceedings of The Physics of Cataclysmic Variables and Related Objects, Goettingen, Germany
dc.identifierhttps://arxiv.org/abs/astro-ph/0109440
dc.identifierhttp://arxiv.org/abs/astro-ph/0109440
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3387
dc.subjectAstrophysics
dc.titleOn the Masses of the Secondary Stars in CVs
dc.typetext

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