Numerical model for the SNR DEM L316: Simulated X-ray emission

We present a two-component supernova remnant model for the case of Magellanic remnant DEM L316 obtained from two-dimensional, axisymmetric hydrodynamic simulations. We study different scenarios which consider a possible collision between the shells and also the effects of thermal conduction. Synthet...

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Detalles Bibliográficos
Autores principales:	Velázquez, Pablo Fabián, Reynoso, Estela Marta
Publicado:	2009
Materias:	Conduction Hydrodynamics Magellanic Clouds Methods: numerical Supernova remnants X-rays: individual: DEM L316
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v395_n1_p351_ToledoRoy http://hdl.handle.net/20.500.12110/paper_00358711_v395_n1_p351_ToledoRoy
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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