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Orbital variability of polarized X-ray radiation reflected from a companion star in X-ray binaries




TekijätAhlberg, Varpu; Kravtsov, Vadim; Poutanen, Juri

KustantajaEDP SCIENCES S A

KustannuspaikkaLES ULIS CEDEX A

Julkaisuvuosi2024

JournalAstronomy and Astrophysics

Tietokannassa oleva lehden nimiASTRONOMY & ASTROPHYSICS

Lehden akronyymiASTRON ASTROPHYS

Artikkelin numero A220

Vuosikerta688

Sivujen määrä8

ISSN0004-6361

eISSN1432-0746

DOIhttps://doi.org/10.1051/0004-6361/202450131

Verkko-osoitehttps://doi.org/10.1051/0004-6361/202450131

Rinnakkaistallenteen osoitehttps://research.utu.fi/converis/portal/detail/Publication/457748026


Tiivistelmä
The reflection of X-ray radiation produced near a compact object from its stellar companion contributes to the orbital variability of polarization in X-ray binaries. The X-rays are reflected mainly via Thomson scattering resulting in a high polarization. The orbital variability of the polarization strongly depends on the inclination and the orbital parameters allowing us to constrain them. To explore this phenomenon, we present analytical single-scattering models for the polarized reflection. We find that while diluted by the direct emission, the reflection can produce a polarization degree of about 1% in the case of a large reflection albedo. We fitted the orbital variations of the X-ray polarization observed by the Imaging X-ray Polarimetry Explorer from an accreting weakly magnetized neutron star "clocked burster" GS 1826-238 and found that the amplitude of the variations is too large to be primarily caused by the companion star. The polarized reflection is more significant if the compact object is obscured from the observer, and thus it should be more easily observable in certain high-inclination targets.

Ladattava julkaisu

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Julkaisussa olevat rahoitustiedot
This research has been supported by the Academy of Finland grants 333112 (JP), 355672 (VA), and by Finnish Cultural Foundation (VK)


Last updated on 2025-27-01 at 19:40