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Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE

Veledina, Alexandra; Muleri, Fabio; Poutanen, Juri; Podgorný, Jakub; Dovčiak, Michal; Capitanio, Fiamma; Churazov, Eugene; ... Zane, Silvia; + view all (2024) Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE. Nature Astronomy , 8 pp. 1031-1046. 10.1038/s41550-024-02294-9. Green open access

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Abstract

The accretion of matter by compact objects can be inhibited by radiation pressure if the luminosity exceeds a critical value known as the Eddington limit. The discovery of ultraluminous X-ray sources has shown that accretion can proceed even when the apparent luminosity considerably exceeds this limit. A high apparent luminosity might be produced due to the geometric beaming of radiation by an outflow. The outflow half-opening angle, which determines the amplification due to beaming, has never been robustly constrained. Using the Imaging X-ray Polarimetry Explorer, we measured the X-ray polarization in the Galactic X-ray binary Cygnus X-3 (Cyg X-3). We found high, >20%, nearly energy-independent linear polarization orthogonal to the direction of the radio ejections. These properties unambiguously indicate the presence of a collimating outflow from the X-ray binary Cyg X-3 and constrain its half-opening angle to ≲15°. Thus, the source can be used as a laboratory for studying the supercritical accretion regime. This finding underscores the importance of X-ray polarimetry in advancing our understanding of accreting sources.

Type: Article
Title: Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE
Open access status: An open access version is available from UCL Discovery
DOI: 10.1038/s41550-024-02294-9
Publisher version: https://doi.org/10.1038/s41550-024-02294-9
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: Compact astrophysical objects, High-energy astrophysics
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10196156
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