Pc-scale study of radio galaxies and BL Lacs

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3844

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DC Field	Value	Language
dc.contributor.author	Kharb, P	-
dc.contributor.author	Shastri, P	-
dc.contributor.author	Gabuzda, D. C	-
dc.date.accessioned	2008-09-23T14:42:09Z	-
dc.date.available	2008-09-23T14:42:09Z	-
dc.date.issued	2003-10	-
dc.identifier.citation	New Astronomy Reviews, Vol. 47, No. 6-7, pp. 431 - 434	en
dc.identifier.issn	1387 - 6473	-
dc.identifier.uri	http://hdl.handle.net/2248/3844	-
dc.description	Restricted Access	-
dc.description.abstract	We study two aspects of the differences between Active Galactic Nuclei (AGN) of the two Fanaroff-Riley types in order to investigate the causes of the F-R divide. We: (a) contrast the properties of the optical cores in beamed and unbeamed AGN of the two types, incorporating Hubble Space Telescope measurements of the unbeamed objects, and (b) contrast the nuclear magnetic field geometry of the beamed AGN of the two types using Very Long Baseline Polarimetry.	en
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/10.1016/S1387-6473(03)00065-4	en
dc.rights	© Elsevier B.V. All rights reserved.	-
dc.subject	Galaxies: Active	en
dc.subject	Galaxies: Nuclei	en
dc.subject	BL Lacertae Objects	en
dc.subject	Polarimetry	en
dc.title	Pc-scale study of radio galaxies and BL Lacs	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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