Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

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Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

The pulsed X-ray emission from the neutron star surface acts as a window to study the state of matter in the neutron star interior. For accreting millisecond pulsars, the surface X-ray emission is generated from the “hotspots” formed due to the magnetically channeled accretion flow hitting the stell...

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Bibliographic Details
Main Authors:	Pushpita Das, Tuomo Salmi, Jordy Davelaar, Oliver Porth, Anna Watts
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal
Subjects:	Neutron stars Pulsars Compact objects Accretion Low-mass x-ray binary stars Magnetohydrodynamics
Online Access:	https://doi.org/10.3847/1538-4357/add472
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