The Dynamics of Radio Galaxies and Double–Double Radio Galaxies

dc.contributor.author	Konar, C.
dc.contributor.author	Jamrozy, M.
dc.contributor.author	Hardcastle, M. J.
dc.contributor.author	Croston, J. H.
dc.contributor.author	Nandi, S.
dc.contributor.author	Saikia, D. J.
dc.contributor.author	Machalski, J
dc.date.accessioned	2015-04-30T04:51:27Z
dc.date.available	2015-04-30T04:51:27Z
dc.date.issued	2011
dc.identifier.uri	http://hdl.handle.net/123456789/1024
dc.description.abstract	Relativistic and magnetized plasma ejected by radio loud AGNs through jets form the diffuse lobes of radio galaxies. The radiating particles (electron/electron–positron) in lobes emit in radio via the synchrotron process and X-ray via inverse-Compton scattering of cosmic microwave background photons. The thermal environment around radio galaxies emits X-rays via the thermal bremsstrahlung process. By combining information from these processes we can measure physical conditions in and around the radio lobes and thus study the dynamics of radio galaxies, including double–double radio galaxies.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	jaa32-477
dc.subject	Galaxies: active—galaxies: jets—galaxies: nuclei—radio continuum: galaxies—galaxies: individual: 3C457, J0041+3224.	en_US
dc.title	The Dynamics of Radio Galaxies and Double–Double Radio Galaxies	en_US
dc.type	Article	en_US