Galaxy cluster virial-shock sources in eROSITA catalogs
arXiv:2402.17822 · doi:10.1051/0004-6361/202449819
Abstract
Following the recent identification of discrete ROSAT and radio sources associated with the virial shocks of MCXC clusters and groups, we examine if the early eROSITA-DE data release (EDR) shows virial-shock X-ray sources within its deg field. EDR catalog sources are stacked and radially binned around EDR catalog clusters and groups. The properties of the excess virial-shock sources are inferred statistically by comparing the virial-shock region to the field. An excess of X-ray sources is found narrowly localized at the normalized radii, just inside the anticipated virial shocks, of the resolved 532 clusters, for samples of both extended ( for 534 sources) or bright ( for 5820 sources; excluding the low cluster-mass quartile) sources. The excess sources are on average extended ( kpc), luminous ( erg s), and hot (keV), consistent with infalling gaseous halos crossing the virial shock. The results agree with the stacked ROSAT-MCXC signal, showing the higher anticipated at EDR redshifts and a possible dependence upon host mass. Localized virial-shock spikes in the distributions of discrete radio, X-ray, and probably also -ray sources are new powerful probes of accretion from the cosmic web, with strong constraints anticipated with future all-sky catalogs such as by eROSITA.
4 pages, 5 figures + Appendices
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- The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups
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