A new relativistic model for accretion-powered X-ray pulsars enables simultaneous computation of phase-averaged spectra and pulse profiles, applied to NuSTAR data for Her X-1 to extract physical parameters and beaming patterns.
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Scattering models predict generically higher linear polarization from magnetars than pulsars and show that single-component scattering cannot explain magnetar spectral shapes.
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A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra
A new relativistic model for accretion-powered X-ray pulsars enables simultaneous computation of phase-averaged spectra and pulse profiles, applied to NuSTAR data for Her X-1 to extract physical parameters and beaming patterns.
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X-ray polarization in magnetized neutron stars
Scattering models predict generically higher linear polarization from magnetars than pulsars and show that single-component scattering cannot explain magnetar spectral shapes.
- Vacuum polarization and cyclotron resonance effects on radiative transfer and plasma deceleration in subcritical X-ray pulsars