Discovery of inverse-Compton X-ray emission and estimate of the volume-averaged magnetic field in a galaxy group

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Authors

MERNIER F. WERNER Norbert BAGCHI J. GENDRON-MARSOLAIS M.-L. GOPAL-KRISHNA Gopal-Krishna GUAINAZZI M. RICHARD-LAFERRIERE A. SHIMWELL T. W. SIMIONESCU A.

Year of publication 2023
Type Article in Periodical
Magazine / Source Monthly Notices of the Royal Astronomical Society
MU Faculty or unit

Faculty of Science

Citation
Web
Doi http://dx.doi.org/10.1093/mnras/stad2093
Keywords magnetic fields; galaxies: clusters: individual: MRC0116+111; galaxies: clusters: intracluster medium; X-rays: galaxies: clusters
Description Observed in a significant fraction of clusters and groups of galaxies, diffuse radio synchrotron emission reveals the presence of relativistic electrons and magnetic fields permeating large scale systems of galaxies. Although, these non-thermal electrons are expected to upscatter cosmic microwave background photons up to hard X-ray energies, such inverse-Compton (IC) X-ray emission has so far not been unambiguously detected on cluster/group scales. Using deep, new proprietary XMM–Newton observations (~200 ks of clean exposure), we report a 4.6?? detection of extended IC X-ray emission in MRC 0116?+111, an extraordinary group of galaxies at z = 0.131. Assuming a spectral slope derived from low frequency radio data, the detection remains robust to systematic uncertainties. Together with low frequency radio data from the Giant Metrewave Radio Telescope (GMRT), this detection provides an estimate for the volume-averaged magnetic field of (1.9 ± 0.3) µG within the central part of the group. This value can serve as an anchor for studies of magnetic fields in the largest gravitationally bound systems in the Universe.
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