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Abstract: The distribution of luminous radio galaxies in galaxy clusters has beenobserved to be concentrated in the inner region. We consider the role ofdynamical friction of massive galaxies $M\sim 10^{12.5}$ M$ {\odot}$,assuming them to be hosts of luminous radio galaxies, and show that beginningwith a Navarro-Frenk-White density profile of a cluster of mass $M {cl}\sim10^{15}$ M$ {\odot}$ of concentration $c\sim 5$ and collapsing at $z\sim 1$,the density profile of radio galaxies evolve to a profile of concentration $c\sim 25$, as observed, in a time scale of $t\sim 3\hbox{-}5$ Gyr.



Author: Biman B. Nath Raman Research Institute, India

Source: https://arxiv.org/







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