Zoo of radio relics: cluster cores to filaments

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4420

Full metadata record

DC Field	Value	Language
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
2011_JAA_V32_p537.pdf Restricted Access	Restricted Access	192.38 kB	Adobe PDF	View/Open Request a copy