Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer

0584791 - ASÚ 2025 RIV GB eng J - Journal Article
Errando, M. - Liodakis, I. - Marscher, A.P. - Karas, Vladimír - Dovčiak, Michal … Total 145 authors
Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer.
Astrophysical Journal. Roč. 963, č. 1 (2024), č. článku 5. ISSN 0004-637X. E-ISSN 1538-4357
Institutional support: RVO:67985815
Keywords : stochastic particle-acceleration * active galactic nuclei * parsec-scale jets
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 4.9, year: 2022
Method of publishing: Open access

Observations of linear polarization in the 2-8 keV energy range with the Imaging X-ray Polarimetry Explorer (IXPE) explore the magnetic field geometry and dynamics of the regions generating nonthermal radiation in relativistic jets of blazars. These jets, particularly in blazars whose spectral energy distribution peaks at X-ray energies, emit X-rays via synchrotron radiation from high-energy particles within the jet. IXPE observations of the X-ray-selected BL Lac-type blazar 1ES 1959+650 on 2022 May 3-4 showed a significant linear polarization degree of pi x = 8.0% +/- 2.3% at an electric-vector position angle psi x = 123 degrees +/- 8 degrees. However, on 2022 June 9-12, only an upper limit of pi x <= 5.1% could be derived (at the 99% confidence level). The degree of optical polarization at that time, pi O similar to 5%, is comparable to the X-ray measurement. We investigate possible scenarios for these findings, including temporal and geometrical depolarization effects. Unlike some other X-ray-selected BL Lac objects, there is no significant chromatic dependence of the measured polarization in 1ES 1959+650, and its low X-ray polarization may be attributed to turbulence in the jet flow with dynamical timescales shorter than 1 day.
Permanent Link: https://hdl.handle.net/11104/0353184