MRC 1925-296: a new WAT in a Poor Cluster

Details MRC 1925-296: a new WAT in a Poor Cluster MRC 1925-296: a new WAT in a Poor Cluster

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..427..353o&link_type=abstract

Accretion and Ejection in AGN: a Global View. Proceedings of a conference held June 22-26, 2009 in Como, Italy. Edited by Laura

Physics

Scientific paper

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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