Rayleigh-Taylor instability in magnetohydrodynamic simulations of the Crab nebula

Porth, O, Komissarov, SS and Keppens, R (2014) Rayleigh-Taylor instability in magnetohydrodynamic simulations of the Crab nebula. Monthly Notices of the Royal Astronomical Society, 443 (1). pp. 547-558. ISSN 0035-8711



  • Porth, O
  • Komissarov, SS
  • Keppens, R
Copyright, Publisher and Additional Information: © The Author 2014. Published by Oxford University Press on behalf of the Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/3.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited.
Keywords: instabilities; MHD; relativistic processes; shock waves; pulsars: general; pulsars: individual: Crab; ISM: supernova remnants
  • Published (online): 12 July 2014
  • Published: 1 September 2014
Institution: The University of Leeds
Academic Units: The University of Leeds > Faculty of Engineering & Physical Sciences (Leeds) > School of Mathematics (Leeds) > Applied Mathematics (Leeds)
Depositing User: Symplectic Publications
Date Deposited: 29 Jun 2016 14:55
Last Modified: 11 Apr 2018 13:25
Published Version: https://dx.doi.org/10.1093/mnras/stu1082
Status: Published
Publisher: Oxford University Press
Identification Number: https://doi.org/10.1093/mnras/stu1082
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