Evolution of random initial magnetic fields in stably stratified and barotropic stars

ABSTRACT Long-lived magnetic fields are known to exist in upper main-sequence stars, white dwarfs, and neutron stars. In order to explore possible equilibrium configurations of the magnetic field inside these stars, we have performed 3D magnetohydrodynamic simulations of the evolution of initially r...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2022-02, Vol.511 (1), p.732-745
Hauptverfasser: Becerra, Laura, Reisenegger, Andreas, Valdivia, Juan Alejandro, Gusakov, Mikhail E
Format: Artikel
Sprache:eng
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