Low frequency radio emission from seyfert galaxies

Singh, V; Shastri, P; Athreya, R

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dc.contributor.author	Singh, V
dc.contributor.author	Shastri, P
dc.contributor.author	Athreya, R
dc.date.accessioned	2010-02-09T13:35:46Z
dc.date.available	2010-02-09T13:35:46Z
dc.date.issued	2009-09
dc.identifier.citation	D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi., The Low-Frequency Radio Universe ASP Conference Series, Vol. 407, Proceedings of the conference held 8 - 12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India., pp. 173 - 175	en
dc.identifier.isbn	978-1-58381-694-3
dc.identifier.uri	http://hdl.handle.net/2248/5004
dc.description	Restricted Access
dc.description.abstract	Seyfert galaxies are low-luminosity, radio-quiet, nearby active galaxies. The high-frequency radio observations of several Seyfert galaxies show jet-like features, which tend to be confined within the host galaxy, whereas low frequency observations reported in the literature show more extended radio emission. We present our preliminary results on the low-frequency radio properties of Seyfert galaxies using GMRT observations.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.ispartofseries	Astronomical Society of the Pacific Conference Series; Vol. 407
dc.relation.uri	http://aspbooks.org/custom/publications/paper/407-0173.html	en
dc.rights	© Astronomical Society of the Pacific	en
dc.subject	Seyfert Galaxies	en
dc.subject	Active Galaxies	en
dc.subject	Radio Observations	en
dc.subject	Radio Emission	en
dc.subject	GMRT Observations	en
dc.title	Low frequency radio emission from seyfert galaxies	en
dc.type	Article	en