Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres

Waves launched from the neutron star surface or inner magnetosphere propagate through the magnetosphere as small perturbations, but can grow relative to the background magnetic field and steepen into “monster shocks”—ultrarelativistic magnetized shocks that can power high-energy emission. Such shock...

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Autors principals:	Michael P. Grehan, Bart Ripperda, Andrei M. Beloborodov, Christopher Thompson, Elias R. Most
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Magnetars Plasma astrophysics High energy astrophysics Shocks X-ray transient sources Magnetohydrodynamical simulations
Accés en línia:	https://doi.org/10.3847/1538-4357/ae633a
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