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Paper: MRC 1925-296: a new WAT in a Poor Cluster
Volume: 427, Accretion and Ejection in AGN: a Global View
Page: 353
Authors: Oozeer, N.; Somanah, R.
Abstract: We have observed MRC 1925-296 using the Giant Metre Wave Radio Telescope (GMRT) at 618 MHz. We classify MRC 1925-296 as a Wide Angle Tail (WAT) source with a rather asymmetric morphology in extent with respect to the radio core. The host galaxy of MRC 1925-296 is coincident with an E+4 galaxy (ESO460-004) of r magnitude 13.83, with a redshift of 0.02442. Using multi-wavelength data, we derive physical properties of the source.
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