Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5-1

0585714 - ASÚ 2025 RIV FR eng J - Článek v odborném periodiku
Fabiani, S. - Capitanio, F. - Iaria, R. - Svoboda, Jiří - Dovčiak, Michal - Karas, Vladimír … celkem 119 autorů
Discovery of a variable energy-dependent X-ray polarization in the accreting neutron star GX 5-1.
Astronomy & Astrophysics. Roč. 684, April (2024), č. článku A137. ISSN 0004-6361. E-ISSN 1432-0746
Grant CEP: GA ČR(CZ) GX21-06825X
Institucionální podpora: RVO:67985815
Klíčová slova: accretion * accretion disks * neutron stars
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 6.5, rok: 2022
Způsob publikování: Open access

We report on the coordinated observations of the neutron star low-mass X-ray binary (NS-LMXB) GX 5-1 in X-rays (IXPE, NICER, NuSTAR, and INTEGRAL), optical (REM and LCO), near-infrared (REM), mid-infrared (VLT VISIR), and radio (ATCA). This Z-source was observed by IXPE twice in March-April 2023 (Obs. 1 and 2). In the radio band the source was detected, but only upper limits to the linear polarization were obtained at a 3 sigma level of 6.1% at 5.5 GHz and 5.9% at 9 GHz in Obs. 1 and 12.5% at 5.5 GHz and 20% at 9 GHz in Obs. 2. The mid-IR, near-IR, and optical observations suggest the presence of a compact jet that peaks in the mid- or far-IR. The X-ray polarization degree was found to be 3.7%+/- 0.4% (at 90% confidence level) during Obs. 1 when the source was in the horizontal branch of the Z-track and 1.8%+/- 0.4% during Obs. 2 when the source was in the normal-flaring branch. These results confirm the variation in polarization degree as a function of the position of the source in the color-color diagram, as for previously observed Z-track sources (Cyg X-2 and XTE 1701-462). Evidence of a variation in the polarization angle of similar to 20(degrees) with energy is found in both observations, likely related to the different, nonorthogonal polarization angles of the disk and Comptonization components, which peak at different energies.
Trvalý link: https://hdl.handle.net/11104/0353908