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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2162
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dc.contributor.authorLal, D. V-
dc.contributor.authorShastri, P-
dc.contributor.authorGabuzda, D-
dc.date.accessioned2008-03-15T11:29:32Z-
dc.date.available2008-03-15T11:29:32Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 403 - 405en
dc.identifier.urihttp://hdl.handle.net/2248/2162-
dc.description.abstractWe have observed a sample of Seyfert galaxies using Global Very Long Baseline Interferometry at 5 GHz. Our goal is to investigate the systematics of their nuclear radio morphology on milli-arcsecond scales. We have chosen our objects so as to be able to test the predictions of the Unified Schemes for Seyfert galaxies. We present preliminary results of the VLBI observations.en
dc.format.extent207733 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..403Len
dc.subjectSeyfert galaxiesen
dc.subjectActive galactic nucleien
dc.subjectVLB Interferometryen
dc.titleSeyferts at milli-arcsec scalesen
dc.typeArticleen
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