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2019MNRAS.484.1475T - Mon. Not. R. Astron. Soc., 484, 1475-1486 (2019/April-1)
Modelling the bow shock Pulsar Wind Nebulae propagating through a non-uniform ISM.
TOROPINA O.D., ROMANOVA M.M. and LOVELACE R.V.E.
Abstract (from CDS):
Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal keyword(s): magnetic fields - MHD - stars: neutron - stars: pulsars
Simbad objects: 6
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