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2017MNRAS.466.4851V - Mon. Not. R. Astron. Soc., 466, 4851-4857 (2017/April-3)
A 3D MHD simulation of SN 1006: a polarized emission study for the turbulent case.
VELAZQUEZ P.F., SCHNEITER E.M., REYNOSO E.M., ESQUIVEL A., DE COLLE F., TOLEDO-ROY J.C., GOMEZ D.O., SIEYRA M.V. and MORANCHEL-BASURTO A.
Abstract (from CDS):
Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): MHD - polarization - radiation mechanisms: general - methods: numerical - supernovae: individual: SN 1006 - ISM: supernova remnants - ISM: supernova remnants
Simbad objects: 2
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