2009/03/16 by Samuel J. George, S. J. George, George, S. J. +3
Physics and Astronomy · #Galaxies: Formation, Evolution, Phenomena #Pulsars and Gravitational Waves Research #Radio Astronomy Observations and Technology #astro-ph.CO
paper · pdf · doi:10.48550/arxiv.0903.2726
4 pages, 2 figures, Proceedings of The Low Frequency Radio Universe, ASP Conference Series, Vol LFRU, 2009, Eds: D.J. Saikia, Dave Green, Y.Gupta and Tiziana Venturi
arxiv created 2009/03/16 · arxiv updated 2009/12/01
We present results of deep 150 MHz observations with the GMRT which show several extended radio sources with a range of morphologies. These sources have then further followed up at higher frequencies (610 and 1400 MHz) with the GMRT. GMRT J0137+4121 was a candidate double--double radio galaxy for which we have also used the VLA-A array at C band to resolve the core. These observations have allowed us to determine that this source is a normal radio galaxy with a core and a one sided jet. Prominent amongst the other extended sources is the giant radio galaxy, 4C39.04.