eROSITA view of Abell 3391/95 field : J/A+A/681/A108

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Authors : Veronica A. orcid , Reiprich T.H., Pacaud F. (hide) , Reiprich T.H., Pacaud F. et..al

VizieR DOI : 10.26093/cds/vizier.36810108
Bibcode : 2024A&A...681A.108V (ADS) (Simbad) (Objects)
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CDS Keywords : Clusters, galaxy; Spectroscopy; X-ray sources
UAT : Galaxy clusters, Spectroscopy, X-ray sources

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Inserted into VizieR : 25-Jan-2024
Last modification : 06-Nov-2024

The eROSITA view of the Abell 3391/95 field. Cluster outskirts and filaments. (2024)

Keywords : galaxies clusters: individual: Abell 3391 - galaxies: clusters: individual: Abell 3395 - galaxies: groups: general - large-scale structure of Universe - X-rays: galaxies - X-rays: galaxies: clusters

Abstract:Many of the "missing" baryons are expected to reside in the warm-hot intergalactic medium (WHIM) in the Cosmic-Web filaments, that connect clusters of galaxies. SRG/eROSITA performance verification (PV) observations covered about 15 square degrees of the A3391/95 system and have revealed a ~15Mpc continuous soft emission, connecting several galaxy groups and clusters. Aim. We aim to characterize the gas properties in cluster outskirts (R500<r ...(more)
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Astronomy and Astrophysics policies
eROSITA Performance Verification data of the A3391/95 system. eROSITA PIB-subtracted, exposure- and Galactic-absorption-corrected image in the 0.3-2.0keV band image.
Angie Veronica, averonica(at)astro.uni-bonn.de

                


                

                    

                


                

                    

                


                

                    
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