Spectral structure of X-shaped radio sources

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DC Field	Value	Language
dc.contributor.author	Vir Lal, D	-
dc.contributor.author	Pramesh Rao, A	-
dc.date.accessioned	2006-03-13T10:48:37Z	-
dc.date.available	2006-03-13T10:48:37Z	-
dc.date.issued	2004-09	-
dc.identifier.citation	BASI, Vol. 32, No. 3, pp. 247-255	en
dc.identifier.uri	http://hdl.handle.net/2248/738	-
dc.description.abstract	Analysis of Giant Metrewave Radio Telescope low frequency data for an X-shaped source, 3C 223.1 has revealed an unusual result as discussed earlier by Lal & Rao (2004). The radio morphologies of it at 240 and 610 MHz show a well-denfied X-shaped structure with a pair of active jets along the north-south axis and a pair of wings along the east-west axis, that pass symmetrically through the undetected radio core. The wings (or low surface brightness jet) seem to have flatter spectral index with respect to the high surface brightness jet. This clearly shows the value of mapping the sample of X-shaped sources at low frequencies. Here we present our preliminary results for two more such sources	en
dc.format.extent	826657 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	galaxies	en
dc.subject	active - galaxies	en
dc.subject	individual: (B1059+169, 3C 136.1, 3C 223.1) - galaxies	en
dc.subject	formation - radio continuum	en
dc.subject	galaxies	en
dc.title	Spectral structure of X-shaped radio sources	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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