An MHD study of SN 1006 and determination of the ambient magnetic field direction

In this work, we employ a magnetohydrodynamic (MHD) numerical code to reproduce the morphology observed for SN 1006 in radio synchrotron and thermal X-ray emission. We introduce a density discontinuity, in the form of a flat cloud parallel to the Galactic plane, in order to explain the NW filament o...

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Detalles Bibliográficos
Autores principales:	Schneiter, E.M., Velázquez, P.F., Reynoso, E.M., De Colle, F.
Formato:	JOUR
Materias:	ISM: supernova remnants Methods: numerical MHD Radiation mechanisms: general Supernovae: individual: SN 1006
Acceso en línea:	http://hdl.handle.net/20.500.12110/paper_00358711_v408_n1_p430_Schneiter
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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