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DC Field | Value | Language |
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dc.contributor.author | Kale, Ruta | - |
dc.contributor.author | Dwarakanath, K.S. | - |
dc.date.accessioned | 2012-04-27T04:28:17Z | - |
dc.date.available | 2012-04-27T04:28:17Z | - |
dc.date.issued | 2011-12 | - |
dc.identifier.citation | Journal of Astrophysics and Astronomy, 2011, Vol.32, p537. | en |
dc.identifier.issn | 0250-6335 | - |
dc.identifier.issn | 0973-7758(online) | - |
dc.identifier.uri | http://hdl.handle.net/2289/4420 | - |
dc.description | Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations) | en |
dc.description.abstract | Radio relics in galaxy clusters can be electrons accelerated at cluster merger shocks or adiabatically compressed fossil radio cocoons or dying radio galaxies. The spectral evolution of radio relics is affected by the surrounding thermal plasma. We present a low frequency study of three radio relics representing environments of dense cluster core (A4038), cluster outskirts (A1664) and filaments (A786). The properties of the relics are found to be consistent with the effect of confinement by external medium if the effects of projection are ignored. | en |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/2011JApA...32..537K | en |
dc.relation.uri | http://dx.doi.org/10.1007/s12036-011-9098-0 | en |
dc.rights | 2011 Indian Academy of Sciences, Bangalore, India | en |
dc.title | Zoo of radio relics: cluster cores to filaments | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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2011_JAA_V32_p537.pdf Restricted Access | Restricted Access | 192.38 kB | Adobe PDF | View/Open Request a copy |
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