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Low Frequency Observations of a Head-Tail Radio Source

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dc.contributor.author Vir Lal, D
dc.contributor.author Pramesh Rao, A
dc.date.accessioned 2008-06-25T09:29:15Z
dc.date.available 2008-06-25T09:29:15Z
dc.date.issued 2003
dc.identifier.citation BASI, Vol. 31, No. 3&4, pp. 427 - 428 en
dc.identifier.uri http://hdl.handle.net/2248/2501
dc.description.abstract We have mapped the head-tail radio galaxy, 3C 129 at 240 and 610 MHz using the GMRT and studied the detailed morphology and spectral index variations in this object. This is the first attempt to observe a sample of head-tail sources at low frequencies. We find weak spectral steepening as we go away from the head along the jet. The Crosspiece has a spectral index of 0.7 (Sv v-) and is flatter than the spectral index estimated by Lane et al. (2002). We also see a low surface brightness, diffuse feature at 240 MHz and could be a possible radio relic candidate (see Figure). en
dc.format.extent 228843 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2003BASI...31..427V en
dc.subject Galaxies:individual:3C 129 en
dc.subject Jets en
dc.subject Radio continuum en
dc.title Low Frequency Observations of a Head-Tail Radio Source en
dc.type Article en


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