Seyfert Galaxies: Radio Continuum Emission Properties and the Unification Scheme

Shastri, Prajval; ATHREYA, RAMANA; Singh, Veeresh

Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5136

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DC Field	Value	Language
dc.contributor.author	Singh, Veeresh	en_US
dc.contributor.author	Shastri, Prajval	en_US
dc.contributor.author	ATHREYA, RAMANA	en_US
dc.date.accessioned	2020-10-19T04:06:23Z	-
dc.date.available	2020-10-19T04:06:23Z	-
dc.date.issued	2011-12	en_US
dc.identifier.citation	Journal of Astrophysics and Astronomy, 32(4), 497-500.	en_US
dc.identifier.issn	0250-6335	en_US
dc.identifier.uri	http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5136	-
dc.identifier.uri	https://doi.org/10.1007/s12036-011-9096-2	en_US
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_US
dc.language.iso	en	en_US
dc.publisher	Springer Nature	en_US
dc.subject	Galaxies: Seyfert	en_US
dc.subject	Galaxies: active	en_US
dc.subject	Radio continuum: galaxies	en_US
dc.subject	2011	en_US
dc.title	Seyfert Galaxies: Radio Continuum Emission Properties and the Unification Scheme	en_US
dc.type	Article	en_US
dc.contributor.department	Dept. of Physics	en_US
dc.identifier.sourcetitle	Journal of Astrophysics and Astronomy	en_US
dc.publication.originofpublisher	Foreign	en_US
Appears in Collections:	JOURNAL ARTICLES

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