Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/994
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dc.contributor.authorLal, D. V-
dc.contributor.authorShastri, P-
dc.contributor.authorGabuzda, D. C-
dc.date.accessioned2006-06-13T11:15:28Z-
dc.date.available2006-06-13T11:15:28Z-
dc.date.issued2004-10-
dc.identifier.citationAstronomy and Astrophysics, Vol. 425, No. 1, 99 - 108en
dc.identifier.urihttp://hdl.handle.net/2248/994-
dc.description.abstractWe have obtained mas-scale resolution very long baseline interferometry (VLBI) images of a sample of Seyfert 1 and Seyfert 2 galaxies at 5 GHz (wavelength, lamda = 6 cm). The Seyferts of the two types were chosen to be matched in several orientation-independent properties, primarily in order to rigorously test predictions of the unified scheme. We detected all the 15 objects that we observed. In this paper we describe the observations and data reduction procedures, and present the VLBI radio images as well as simultaneous Very Large Array images that we obtained for these 15 Seyfertsen
dc.format.extent1119855 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEDP Sciences-
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361:20040486-
dc.rights© ESO-
dc.subjectSeyferten
dc.subjectRadio continuumen
dc.subjectGalaxiesen
dc.titleMilliarcsec-scale radio structure of a matched sample of Seyfert 1 and Seyfert 2 galaxiesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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