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2018MNRAS.478.2074B - Mon. Not. R. Astron. Soc., 478, 2074-2085 (2018/August-1)
A laminar model for the magnetic field structure in bow-shock pulsar wind nebulae.
BUCCIANTINI N.
Abstract (from CDS):
Abstract Copyright: © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): MHD - polarization - radiation mechanisms: non-thermal - relativistic processes - ISM: supernova remnants
Simbad objects: 6
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