Magnetic Field Geometry of the Broad Line Radio Galaxy 3C111

3); Bangalore; (2) University College Cork; (3) Astro Space Center; Bonn); D. Gabuzda (2; E. Preuss (4); Moscow; (4) MPIfR; P. Kharb (1); P. Shastri (1) ((1) IIA; W. Alef (4)

arxiv: astro-ph/0301065 · v1 · submitted 2003-01-06 · 🌌 astro-ph

Magnetic Field Geometry of the Broad Line Radio Galaxy 3C111

P. Kharb (1) , D. Gabuzda (2 , 3) , W. Alef (4) , E. Preuss (4) , P. Shastri (1) ((1) IIA , Bangalore; (2) University College Cork; (3) Astro Space Center , Moscow; (4) MPIfR

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keywords radiobroadc111galaxygeometrylineanalysisb-field

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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.

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Magnetic Field Geometry of the Broad Line Radio Galaxy 3C111

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