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Altamirano, D · 2010 · DOI 10.1088/2041-8205/712/1/l58

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astro-ph.HE 1

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2024 1

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CONDITIONAL 1

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Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

astro-ph.HE · 2024-11-25 · conditional · novelty 7.0

GRMHD simulations with relativistic ray tracing show that realistic accretion hotspots are crescent- or band-shaped, not circular, and produce X-ray pulse amplitudes consistent with accreting millisecond pulsars.

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  • Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations astro-ph.HE · 2024-11-25 · conditional · none · ref 4

    GRMHD simulations with relativistic ray tracing show that realistic accretion hotspots are crescent- or band-shaped, not circular, and produce X-ray pulse amplitudes consistent with accreting millisecond pulsars.