Binary Interaction Dominates Mass Ejection in Classical Novae

Recent observations suggest our understanding of mass loss in classical novae is incomplete, motivating a new theoretical examination of the physical processes responsible for nova mass ejection. In this paper, we perform hydrodynamical simulations of classical nova outflows using the stellar evolut...

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Veröffentlicht in:	The Astrophysical journal 2022-10, Vol.938 (1), p.31
Hauptverfasser:	Shen, Ken J., Quataert, Eliot
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Binary stars Cataclysmic variable stars Cataclysmic variables Classical novae Companion stars Dwarf novae Ejecta Novae Outflow Radiation Stellar evolution White dwarf stars Wind
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