Fits of a magnetized plasma radiative-transfer model to bright magnetar bursts favor heavy nuclei (effective charge Z≈37) over light ions, suggesting neutron-star crust material enters the emitting fireball.
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2026 3representative citing papers
Force-free simulations confirm that fast magnetosonic waves undergo efficient parametric decay into secondary FMS and Alfvén waves, producing a broad spectrum and continued energy drain even after equipartition.
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Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
Fits of a magnetized plasma radiative-transfer model to bright magnetar bursts favor heavy nuclei (effective charge Z≈37) over light ions, suggesting neutron-star crust material enters the emitting fireball.