Seyfert Galaxies: Radio Continuum Emission Properties and the Unification Scheme

dc.contributor.author	Singh, V
dc.contributor.author	Shastri, P
dc.contributor.author	Athreya, R
dc.date.accessioned	2012-02-24T10:31:29Z
dc.date.available	2012-02-24T10:31:29Z
dc.date.issued	2011-12
dc.identifier.citation	Journal of Astrophysics and Astronomy, Vol. 32, No. 4, pp. 497-500	en
dc.identifier.uri	http://hdl.handle.net/2248/5703
dc.description.abstract	Seyfert galaxies are classified mainly into type 1 and type 2 depending on the presence and absence of broad permitted emission lines in their optical spectra, respectively. Unification scheme hypothesizes that the observed similarities and differences between the two Seyfert subtypes can be understood as due to the differing orientations of anisotropically distributed obscuring material having a torus-like geometry around the AGN. We investigate the radio continuum emission properties of a sample of Seyfert galaxies in the framework of the unification scheme	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://dx.doi.org/10.1007/s12036-011-9096-2	en
dc.rights	© Indian Academy of Sciences	en
dc.subject	Galaxies: Seyfert—galaxies	en
dc.subject	Active—radio continuum: galaxies	en
dc.title	Seyfert Galaxies: Radio Continuum Emission Properties and the Unification Scheme	en
dc.type	Article	en