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Published online by Cambridge University Press: 26 May 2016
An important aspects of the studies of giant radio sources is that they can constrain models of the cosmological evolution of radio sources (e.g. Condon 1984, ApJ, 287, 461; Dunlop & Peacock 1990, MNRAS, 247, 19) and their host galaxies, as well as the recent analytical models of time evolution of these sources (e.g. Kaiser, Dennett—Thorpe & Alexander 1997, MNRAS, 292, 723; Blundell et al. 1999, AJ, 117, 677). In order to achieve these goals, we undertook the following tasks: