Is WX CEN a possible type Ia supernova progenitor with wind-driven mass transfer?

WX Cen is one of a few compact binary supersoft X-ray sources (CBSS) in the Galaxy that is a possible Type Ia supernova (SN Ia) progenitor. The supersoft X-ray radiation is explained as hydrostatic nuclear burning on the surface of the white dwarf component that is accreting hydrogen from a stellar...

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Detalles Bibliográficos
Autores principales:	Qian, S.-B., Shi, G., Fernández Lajús, Eduardo, Di Sisto, Romina Paula, Zhu, L.-Y., Liu, L., Zhao, E.-G., Li, L.-J.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2013
Materias:	Ciencias Astronómicas binaries: eclipsing close stars: evolution stars: individual (WX Cen) stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85592
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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