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Variability of X-ray polarization of Cyg X-1

Lookup NU author(s): Dr Adam IngramORCiD

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This work is licensed under a Creative Commons Attribution 4.0 International License (CC BY 4.0).


Abstract

c The Authors 2025.We present the results of a three-year X-ray, optical, and radio polarimetric monitoring campaign of the prototypical black hole X-ray binary Cyg X-1, conducted from 2022 to 2024. The X-ray polarization of Cyg X-1 was measured 13 times with the Imaging X-ray Polarimetry Explorer (IXPE), covering both hard and soft spectral states. The X-ray polarization degree (PD) in the hard state was found to be ≈4.0%, roughly twice as high as in the soft state, where it was around 2.2%. In both states, a statistically significant increase in PD with the energy was found. Moreover, a linear relation between PD and spectral hardness suggests a gradual and continuous evolution of the polarization properties, rather than an abrupt change of polarization production mechanism between states. The polarization angle (PA) was independent of the spectral state and showed no trend with the photon energy. The X-ray PA is well aligned with the orientation of the radio jet, as well as the optical and radio PAs. We find significant orbital changes of PA in the hard state, which we attribute to scattering of X-ray emission at the intrabinary structure. No significant superorbital variability in PD or PA was found at the period Pso = 294 d. We detect, for the first time in this source, polarization of the radio emission, with the PA aligned with the jet, and a strong increase of the PD at a transition to the soft state. We also find no correlation between the X-ray and optical polarization; if any, there is a long-term anti-correlation between the X-ray PD and the radio PD.


Publication metadata

Author(s): Kravtsov V, Bocharova A, Veledina A, Poutanen J, Hughes AK, Dovciak M, Egron E, Muleri F, Podgorny J, Svoboda J, Forsblom SV, Berdyugin AV, Blinov D, Bright JS, Carotenuto F, Green DA, Ingram A, Liodakis I, Mandarakas N, Nitindala AP, Rhodes L, Trushkin SA, Tsygankov SS, Brigitte M, Marco AD, Iacolina N, Krawczynski H, Monaca FL, Loktev V, Mastroserio G, Petrucci P-O, Pilia M, Tombesi F, Zdziarski AA

Publication type: Article

Publication status: Published

Journal: Astronomy and Astrophysics

Year: 2025

Volume: 701

Print publication date: 01/09/2025

Online publication date: 05/09/2025

Acceptance date: 24/07/2025

Date deposited: 30/09/2025

ISSN (print): 0004-6361

ISSN (electronic): 1432-0746

Publisher: EDP Sciences

URL: https://doi.org/10.1051/0004-6361/202555411

DOI: 10.1051/0004-6361/202555411


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Funding

Funder referenceFunder name
ASI-INAF-2022-14-HH.0
ASI-OHBI-2022-13-I.0
ASI-INAF-2022-19-HH.0
ASI-INFN 2021-43-HH.0
ASI-INFN-2017.13-H0
Istituto Nazionale di Astrofisica (INAF)
Istituto Nazionale di Fisica Nucleare (INFN)
Italian Space Agency (Agenzia Spaziale Italiana, ASI)
National Aeronautics and Space Administration (NASA)
Royal Society

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