Different Angles on Active Galaxies: Where are We with Regard to Unification?

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2143

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DC Field	Value	Language
dc.contributor.author	Shastri, P	-
dc.date.accessioned	2008-03-07T09:01:57Z	-
dc.date.available	2008-03-07T09:01:57Z	-
dc.date.issued	2007-10	-
dc.identifier.citation	Astronomical Society of the Pacific Conference Series, Vol. 373, pp. 435 - 438	en
dc.identifier.uri	http://hdl.handle.net/2248/2143	-
dc.description	Restricted Access	en
dc.description.abstract	With the realization that orientation plays a dominant role in the appearance of active galaxies, much of AGN research has been worked into the operating framework of the �unified scheme,� wherein active galaxies are broadly classified into three physically distinct classes: radio-quiet, radio-loud Fanaroff-Riley I and radio-loud Fanaroff-Riley II, with the appearance in each of the three cases being dominated by orientation alone. The following is a brief summary of the current understanding on the domain of validity of the scheme.	en
dc.format.extent	130201 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://aspbooks.org/custom/publications/paper/373-0435.html	en
dc.subject	Active Galaxies	en
dc.title	Different Angles on Active Galaxies: Where are We with Regard to Unification?	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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