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

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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Bibliographic Details
Main Authors: Sumner Starrfield, Maitrayee Bose, Christian Iliadis, W. Raphael Hix, Charles E. Woodward, R. Mark Wagner
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Cataclysmic variable stars
Novae
Recurrent novae
Symbiotic novae
Galaxy abundances
Galaxy chemical evolution
Online Access:https://doi.org/10.3847/1538-4357/ad1836

Internet

https://doi.org/10.3847/1538-4357/ad1836

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