Polarisation of Accreting X-ray Pulsars. II. Hercules X-1

Abstract

We employ our new model for the polarised emission of accreting X-ray pulsars to describe the emission from the luminous X-ray pulsar Hercules X-1. In contrast with previous works, our model predicts the polarisation parameters independently of spectral formation, and considers the structure and dynamics of the accretion column, as well as the additional effects on propagation due to general relativity and quantum electrodynamics. We find that our model can describe the observed pulse fraction and the pulse shape of the main peak, as well as the modulation of the cyclotron line with phase. We pick two geometries, assuming a single accretion column or two columns at the magnetic poles, that can describe current observations of pulse shape and cyclotron modulation with phase. Both models predict a high polarisation fraction, between 60 and 80\% in the $1-10$ keV range, that is phase- and energy-dependent, and that peaks at the same phase as the intensity. The phase and energy dependence of the polarisation fraction and of the polarisation angle can help discern between the different geometries.

8 pages, 7 figures, submitted to MNRAS

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Cited by in corpus (6)

• Determination of X-ray pulsar geometry with IXPE polarimetry
• A polarimetrically oriented X-ray stare at the accreting pulsar EXO 2030+375
• Unbinned Likelihood Analysis for X-ray Polarization
• Vacuum polarization alters the spectra of accreting X-ray pulsars
• X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries
• Flux-resolved Spectropolarimetric Evolution of the X-Ray Pulsar Hercules X-1 Using IXPE