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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5004
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dc.contributor.authorSingh, V-
dc.contributor.authorShastri, P-
dc.contributor.authorAthreya, R-
dc.date.accessioned2010-02-09T13:35:46Z-
dc.date.available2010-02-09T13:35:46Z-
dc.date.issued2009-09-
dc.identifier.citationD. 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 - 175en
dc.identifier.isbn978-1-58381-694-3-
dc.identifier.urihttp://hdl.handle.net/2248/5004-
dc.descriptionRestricted Access-
dc.description.abstractSeyfert 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.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.ispartofseriesAstronomical Society of the Pacific Conference Series; Vol. 407-
dc.relation.urihttp://aspbooks.org/custom/publications/paper/407-0173.htmlen
dc.rights© Astronomical Society of the Pacificen
dc.subjectSeyfert Galaxiesen
dc.subjectActive Galaxiesen
dc.subjectRadio Observationsen
dc.subjectRadio Emissionen
dc.subjectGMRT Observationsen
dc.titleLow frequency radio emission from seyfert galaxiesen
dc.typeArticleen
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