Modeling the High-brightness State of the Recurrent Nova T CrB as an Enhanced Mass-transfer Event

T Coronae Borealis is the nearest symbiotic recurrent nova. Twice in the last two centuries, in 1866 and 1946, the accreted material ignited on the surface of the white dwarf via runaway thermonuclear fusion reactions and produced a nova eruption. Both eruptions occurred approximately midway through...

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Detalhes bibliográficos

Principais autores:	Wagner Schlindwein, Raymundo Baptista, Gerardo Juan Manuel Luna
Formato:	Artigo
Idioma:	Inglês
Publicado em:	IOP Publishing 2025-01-01
coleção:	The Astrophysical Journal
Assuntos:	Stellar accretion disks Symbiotic binary stars Recurrent novae Astronomical simulations Interacting binary stars
Acesso em linha:	https://doi.org/10.3847/1538-4357/ade98c
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