Low Frequency Radio Morphology of Head-tail Radio Sources in the Perseus Cluster

Details Low Frequency Radio Morphology of Head-tail Radio Sources in the Perseus Cluster Low Frequency Radio Morphology of Head-tail Radio Sources in the Perseus Cluster

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..345..294l&link_type=abstract

From Clark Lake to the Long Wavelength Array: Bill Erickson's Radio Science ASP Conference Series, Vol. 345, Proceedings of the

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We present radio maps of two head-tail radio galaxies, NGC 1265 (3C 83.1B) and IC 310 in the Perseus cluster at 240 and 610 MHz using the Giant Metrewave Radio Telescope. We have studied in detail the morphology of these sources and the distribution of spectral indices over these objects. We find large-scale spectral steepening along the jet away from the core in each of the two sources. We present preliminary morphological and spectral results for these sources.

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