Magnetic field geometry of the broad line radio galaxy 3C111

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3687

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DC Field	Value	Language
dc.contributor.author	Kharb, P	-
dc.contributor.author	Gabuzda, D. C	-
dc.contributor.author	Alef, W	-
dc.contributor.author	Preuss, E	-
dc.contributor.author	Shastri, P	-
dc.date.accessioned	2008-09-17T10:26:41Z	-
dc.date.available	2008-09-17T10:26:41Z	-
dc.date.issued	2003-10	-
dc.identifier.citation	New Astronomy Reviews, Vol. 47, No. 6 - 7, pp. 621 - 624	en
dc.identifier.issn	1387 - 6473	-
dc.identifier.uri	http://hdl.handle.net/2248/3687	-
dc.description	Restricted Access	-
dc.description.abstract	Very Long Baseline Polarimetric observations of the Broad Line Radio galaxy 3C111 performed in July and September of 1996 at 8 and 43 GHz reveal rapidly evolving parsec-scale radio structure after a large millimetre outburst. The B-field geometry is not simple. We present a first analysis of possible Faraday and optical depth effects based on a comparison of the polarization images for the two frequencies.	en
dc.language.iso	en	en
dc.publisher	Elsevier	en
dc.relation.uri	http://dx.doi.org/10.1016/S1387-6473(03)00107-6	en
dc.rights	© Elsevier B.V. All rights reserved	-
dc.subject	Galaxies: Individual (3C111)	en
dc.subject	Polarimetry	en
dc.subject	Interferometry	en
dc.title	Magnetic field geometry of the broad line radio galaxy 3C111	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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