0586062 - ASÚ 2025 RIV US eng J - Článek v odborném periodiku
Svoboda, Jiří - Dovčiak, Michal - Steiner, J.F. - Kaaret, P. - Podgorný, Jakub - Brigitte, Maimouna - Datta, Sudeb Ranjan … celkem 37 autorů
Dramatic drop in the X-ray polarization of Swift J1727.8-1613 in the soft spectral state.
Astrophysical Journal Letters. Roč. 966, č. 2 (2024), č. článku L35. ISSN 2041-8205. E-ISSN 2041-8213
Grant CEP: GA ČR(CZ) GX21-06825X
Institucionální podpora: RVO:67985815
Klíčová slova: black hole physics * X-ray astronomy * polarimetry
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 8.8, rok: 2023
Způsob publikování: Open access
DOI: https://doi.org/10.3847/2041-8213/ad402e

Black hole X-ray binaries exhibit different spectral and timing properties in different accretion states. The X-ray outburst of a recently discovered and extraordinarily bright source, Swift J1727.8-1613, has enabled the first investigation of how the X-ray polarization properties of a source evolve with spectral state. The 2-8 keV polarization degree was previously measured by the Imaging X-ray Polarimetry Explorer (IXPE) to be approximate to 4% in the hard and hard intermediate states. Here we present new IXPE results taken in the soft state, with the X-ray flux dominated by the thermal accretion disk emission. We find that the polarization degree has dropped dramatically to less than or similar to 1%. This result indicates that the measured X-ray polarization is largely sensitive to the accretion state and the polarization fraction is significantly higher in the hard state when the X-ray emission is dominated by upscattered radiation in the X-ray corona. The combined polarization measurements in the soft and hard states disfavor a very high or low inclination of the system.

Trvalý link: https://hdl.handle.net/11104/0353686