Seyfert Galaxies on milliarcsecond scales

dc.contributor.author	Lal, D. V
dc.contributor.author	Shastri, P
dc.contributor.author	Gabuzda, D. C
dc.date.accessioned	2010-01-25T12:14:51Z
dc.date.available	2010-01-25T12:14:51Z
dc.date.issued	2001-08
dc.identifier.citation	Astronomical and Astrophysical Transactions, Vol. 20, No. 2, pp. 311 – 313	en
dc.identifier.uri	http://hdl.handle.net/2248/5001
dc.description	Restricted Access
dc.description.abstract	We present our results from global VLBI observations of a sample of Seyfert galaxies at 5 GHz. Our goal was to test predictions of the Unified Scheme for Seyfert galaxies, in which observed differences between Seyferts of types I and II can be understood as effects of orientation alone. Our Seyferts of the two types were matched in their orientation-independent AGN and host-galaxy properties so that the Unified Scheme may be rigourously tested. We show that the compact radio structures of the two types of Seyferts are similar, supporting the simple Unified Scheme. The implications of our results are discussed	en
dc.language.iso	en	en
dc.publisher	Taylor and Francis	en
dc.relation.uri	http://www.informaworld.com/smpp/content~db=all?content=10.1080/10556790108229716	en
dc.rights	© Taylor and Francis	en
dc.subject	Seyfert Galaxies	en
dc.subject	VLBI-Observations	en
dc.subject	Radio Structure	en
dc.title	Seyfert Galaxies on milliarcsecond scales	en
dc.type	Article	en