Magnetic field geometry of the broad line radio galaxy 3C111

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