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