Gaseous outflows in Seyferts and unification: The case of Mrk 533

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DC Field	Value	Language
dc.contributor.author	Shastri, P	-
dc.contributor.author	Murthy, J	-
dc.contributor.author	Hutchings, J	-
dc.contributor.author	Wills, B. J	-
dc.date.accessioned	2011-12-07T14:23:05Z	-
dc.date.available	2011-12-07T14:23:05Z	-
dc.date.issued	2004-11	-
dc.identifier.citation	International Astronomical Union Symposium, Vol. 222, pp. 291-294	en
dc.identifier.uri	http://hdl.handle.net/2248/5626	-
dc.description	Open Access	en
dc.description.abstract	We present our recent results from the observation of the O VI λ λ1032,1038 emission doublet in Seyfert galaxies of type 2 with the FUV spectrograph on the FUSE satellite. These observations are part of our investigation to contrast the properties of the OVI emission line and the absorbing outflows in a sample of rigorously matched Seyfert 1s and 2s, in the framework of the Unified Scheme. The OVI emission line is an excellent diagnostic of the outflowing hot gas at temperatures of [similar]106K. In the Unified Scheme, Seyferts of type 2 are those whose central regions are obscured by the ubiquitous dusty torus. We interpret our results in this framework.	en
dc.language.iso	en	en
dc.publisher	Cambridge University Press	en
dc.relation.uri	http://10.1017/S1743921304002297	en
dc.rights	© Cambridge University Press	en
dc.title	Gaseous outflows in Seyferts and unification: The case of Mrk 533	en
dc.type	Article	en
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