086441

Galaxy clusters grow hierarchically through the merger-accretion of smaller substructures along filaments. The dynamically young cluster A1367 is one of the best examples to study the cluster evolution because of its proximity and with abundant multi-wavelength data. Additional to the main merger along the NW-SE direction and a merger shock-radio relic at the NW comma we also find evidences of another counter-shock at the SE and the accretion of group-filament along the Coma-A1367 supercluster. We propose XMM observations to complete a coverage of the R500 radius of A1367 to 1closePar explore the unique case of an extended shock radio-tail interaction 2closePar study the dynamics of the cluster-filament transition region and 3closePar search for X-ray tails-clumps associated with Halpha emission.