Asymmetries in the expansion and emission from young supernova remnants

We present two-dimensional and three-dimensional numerical simulations of asymmetric young supernova remnants (SNRs) carried out with the hydrodynamical code Yguazú, aiming to quantitatively assess the role of different factors that may give origin to such asymmetries in their expansion. In particul...

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Detalles Bibliográficos
Publicado: 2011
Materias:
Hydrodynamics
ISM: supernova remnants
Methods: numerical
Shock waves
Supernovae: individual (Tycho)
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v727_n1_p_Vigh
http://hdl.handle.net/20.500.12110/paper_0004637X_v727_n1_p_Vigh
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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