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- W2019958609 abstract "Classical novae are violent stellar events at the crossroads of astrophysics, nuclear physics, and cosmochemistry. They are powered by thermonuclear runaways (hereafter, TNR) that take place at the base of an accreted envelope, transferred from a Main Sequence (or a more evolved) stellar companion onto a compact white dwarf in a close binary system. The number of nova explosions expected in our galaxy is 30± 10yr−1 [1 Shafter, A.W., Hernanz, M. and José, J., eds. 2002. “Classical Nova Explosions”. In AIP Conference Proceedings, Vol. 637, 462New York: AIP. [Google Scholar]]. Contrary to type Ia supernovae, for which the white dwarf is fully disrupted by the violence of the explosion, all classical novae are expected to recur, with periodicities of the order of 104–105 years (in contrast, X-ray bursts recur on timescales from hours to days)." @default.
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- W2019958609 date "2005-10-01" @default.
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- W2019958609 title "Feature Article: Nucleosynthesis in Classical Nova Explosions: Modeling and Nuclear Uncertainties" @default.
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