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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) |
Files in This Item:
File | Description | Size | Format | |
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2008 MNRAS V387 L50.pdf Restricted Access | Restricted Access | 479.48 kB | Adobe PDF | View/Open Request a copy |
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