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2019MNRAS.488.2466B - Mon. Not. R. Astron. Soc., 488, 2466-2472 (2019/September-2)
Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification.
BELL A.R., MATTHEWS J.H. and BLUNDELL K.M.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): acceleration of particles - magnetic fields - shock waves - cosmic rays
Simbad objects: 3
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