A 3D numerical model for Kepler's supernova remnant

We present new 3D numerical simulations for Kepler's supernova remnant. In this work we revisit the possibility that the asymmetric shape of the remnant in X-rays is the product of a Type Ia supernova explosion which occurs inside the wind bubble previously created by an AGB companion star. Due...

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Detalles Bibliográficos
Autores principales:	Velázquez, Pablo Fabián, Reynoso, Estela Marta
Publicado:	2014
Materias:	Hydrodynamics ISM: supernova remnants Methods: numerical Radiation mechanisms: thermal X-rays: ISM
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v442_n1_p229_ToledoRoy http://hdl.handle.net/20.500.12110/paper_00358711_v442_n1_p229_ToledoRoy
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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