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Diffuse, non-thermal extended emission not associated with the AGNphenomenon, found in many clusters of galaxies hosted by an AGN, are related tothe acceleration of cosmic rays. In the current work we present preliminaryevidence of absence of such formations in clusters of galaxies hosted byoptically identified cD galaxies. Our subsample consists of three powerful lowredshift radiogalaxies, centered in poor clusters of galaxies. We have searchedfor radio relics and (mini)halos which could be forming as a result of theconfinement of cosmic rays by bubbles creayed by the AGN. We report on the workin progress.

Extended reagions of radio emission not associated with the AGN phenomenon as sources of acceleration of cosmic rays: The case of cD galaxies