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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3629

Title: Dynamical friction of radio galaxies in galaxy clusters
Authors: Nath, Biman B.
Keywords: galaxies: active
galaxies: clusters
radio continuum: galaxies
Issue Date: Jun-2008
Publisher: Blackwell Publishing for the RAS
Citation: Monthly Notices of the Royal Astronomical Society, 2008, Vol.387, pL50
Abstract: The distribution of luminous radio galaxies in galaxy clusters has been observed to be concentrated in the inner region. We consider the role of dynamical friction of massive galaxies (M ~ 1012.5Msolar), assuming them to be hosts of luminous radio galaxies, and show that beginning with a Navarro-Frenk-White density profile of a cluster of mass Mcl ~ 1015Msolar of concentration c ~ 5 and collapsing at z ~ 1, the density profile of radio galaxies evolves to a profile of concentration c ~ 25, as observed, in a time-scale of t ~ 3-5 Gyr.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)
URI: http://hdl.handle.net/2289/3629
ISSN: E-ISSN: 1365-2966
P-ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/abs/2008MNRAS.387L..50N
http://arxiv.org/abs/0804.3468
http://dx.doi.org/10.1111/j.1745-3933.2008.00483.x
Copyright: 2008 The Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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