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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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Bibliografski detalji
Glavni autori: Michael P. Grehan, Bart Ripperda, Andrei M. Beloborodov, Christopher Thompson, Elias R. Most
Format: Artigo
Jezik:Inglês
Izdano: IOP Publishing 2026-01-01
Serija:The Astrophysical Journal
Teme:
Online pristup:https://doi.org/10.3847/1538-4357/ae633a
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