Radio and X-ray Emission from Low-Luminosity AGNs: Testing Unification Hypothesis

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5564

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DC Field	Value	Language
dc.contributor.author	Singh, V	-
dc.contributor.author	Shastri, P	-
dc.contributor.author	Risaliti, G	-
dc.contributor.author	Athreya, R	-
dc.date.accessioned	2011-09-09T16:26:20Z	-
dc.date.available	2011-09-09T16:26:20Z	-
dc.date.issued	2010-10	-
dc.identifier.citation	ASP Conference Series, Vol. 427, pp. 391-392	en
dc.identifier.uri	http://hdl.handle.net/2248/5564	-
dc.description	Restricted Access	en
dc.description.abstract	We investigate the low-frequency radio properties and the X-ray spectral properties of a sample of Seyfert galaxies in order to compare the two subtypes of Seyferts and rigorously test the predictions of Seyfert unification.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://aspbooks.org/custom/publications/paper/427-0391.html	en
dc.rights	© Astronomical Society of the Pacific	en
dc.title	Radio and X-ray Emission from Low-Luminosity AGNs: Testing Unification Hypothesis	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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