Three-dimensional hydrodynamical simulations of the large-scale structure of W50-SS433

We present 3D hydrodynamical simulations of a precessing jet propagating inside a supernova remnant (SNR) shell, particularly applied to the W50-SS433 system in a search for the origin of its peculiar elongated morphology. Several runs were carried out with different values for the mass-loss rate of...

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Detalles Bibliográficos
Publicado:	2008
Materias:	ISM: jets and outflows Methods: numerical Shock waves Supernova remnants
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v387_n2_p839_Zavala http://hdl.handle.net/20.500.12110/paper_00358711_v387_n2_p839_Zavala
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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