Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Nova Cycles

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dc.contributor.author Townsley, Dean M.
dc.contributor.author Bildsten, Lars
dc.date 2004-01-01
dc.date.accessioned 2018-08-22T20:38:48Z
dc.date.available 2018-08-22T20:38:48Z
dc.date.issued 2004-01-01
dc.identifier.citation Townsley, D., Bildsten, L. (2004): Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Nova Cycles. The Astrophysical Journal, 600(1). en_US
dc.identifier.uri http://ir.ua.edu/handle/123456789/3746
dc.format.mimetype application/pdf en_US
dc.subject binaries: close — novae en_US
dc.subject cataclysmic variables — nuclear reactions en_US
dc.subject nucleosynthesis en_US
dc.subject abundances — stars: dwarf novae — white dwarfs en_US
dc.title Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Nova Cycles en_US
dc.type text en_US


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