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2017MNRAS.470.4066B - Mon. Not. R. Astron. Soc., 470, 4066-4074 (2017/October-1)
Modeling the effect of small-scale magnetic turbulence on the X-ray properties of Pulsar Wind Nebulae.
BUCCIANTINI N., BANDIERA R., OLMI B. and DEL ZANNA L.
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: non-thermal - relativistic processes - ISM: individual objects: Crab nebula - ISM: supernova remnants - ISM: supernova remnants
Simbad objects: 2
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