X-Ray Polarimetry as a Tool to Constrain Orbital Parameters in X-Ray Binaries




Rankin, John; Kravtsov, Vadim; Muleri, Fabio; Poutanen, Juri; Marin, Frédéric; Capitanio, Fiamma; Matt, Giorgio; Costa, Enrico; Di Marco, Alessandro; Fabiani, Sergio; La Monaca, Fabio; Marra, Lorenzo; Soffitta, Paolo

PublisherThe American Astronomical Society

2024

 Astrophysical Journal

The Astrophysical Journal

34

962

1

1538-4357

DOIhttps://doi.org/10.3847/1538-4357/ad1991

https://iopscience.iop.org/article/10.3847/1538-4357/ad1991

https://research.utu.fi/converis/portal/detail/Publication/386840119

https://arxiv.org/abs/2312.16967



X-ray binary systems consist of a companion star and a compact object in close orbit. Thanks to their copious X-ray emission, these objects have been studied in detail using X-ray spectroscopy and timing. The inclination of these systems is a major uncertainty in the determination of the mass of the compact object using optical spectroscopic methods. In this paper, we present a new method to constrain the inclination of X-ray binaries, which is based on the modeling of the polarization of X-rays photons produced by a compact source and scattered off the companion star. We describe our method and explore the potential of this technique in the specific case of the low-mass X-ray binary GS 1826−238 observed by the Imaging X-ray Polarimetry Explorer observatory.

Last updated on 11/02/2026 11:20:07 AM