Theoretical Modeling of the Thermal State of Accreting White Dwarfs Undergoing Classical Nova Cycles
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Date
2004-01-01
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binaries: close — novae, cataclysmic variables — nuclear reactions, nucleosynthesis, abundances — stars: dwarf novae — white dwarfs
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).