Hydrodynamic Simulations of Oxygen–Neon Classical Novae as Galactic 7Li Producers and Potential Accretion-induced Collapse Progenitors

We report on studies of classical nova (CN) explosions where we follow the evolution of thermonuclear runaways (TNRs) on oxygen–neon (ONe) white dwarfs (WDs). Using NOVA, a 1D hydrodynamic computer code, we accrete solar matter until the TNR is ongoing and then switch to a mixed composition. This ap...

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Váldodahkkit:	Sumner Starrfield, Maitrayee Bose, Christian Iliadis, W. Raphael Hix, Charles E. Woodward, R. Mark Wagner
Materiálatiipa:	Artigo
Giella:	Inglês
Almmustuhtton:	IOP Publishing 2024-01-01
Ráidu:	The Astrophysical Journal
Fáttát:	Cataclysmic variable stars Novae Recurrent novae Symbiotic novae Galaxy abundances Galaxy chemical evolution
Liŋkkat:	https://doi.org/10.3847/1538-4357/ad1836
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