Searching for Inverse Compton Emission in strong FRII Radio Galaxies
收藏ESA Earth Online2026-06-22 收录
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We propose relatively deep XMM observations of 3 high redshiftradiogalaxies in order to study the origin of their Xray emission.In particular we want to test if a hot thermal gas possibly associatedwith high redshift cluster is present or if a Invers Compton emissionof the nuclear photons off the relativistic electrons in the radio lobesis responsible of the weak Xray fluxes observed by ROSAT.
