Faraday rotation measures in 20 AGN jets at parsec scale

We present multi wavelength parsec-scale Faraday rotation measure properties of twenty active galactic nuclei, observed with the Very Long Baseline Array simultaneously at 1.4, 1.6, 2.2, 2.4, 4.6, 5.0, 8.1, 8.4 and 15.4 GHz in the full polarization mode. For the observed sources we construct Faraday...

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Main Authors: Kravchenko Evgeniya V., Kovalev Yuri Y., Sokolovsky Kirill V.
Format: Article
Language:English
Published: EDP Sciences 2013-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136107006
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author Kravchenko Evgeniya V.
Kovalev Yuri Y.
Sokolovsky Kirill V.
author_facet Kravchenko Evgeniya V.
Kovalev Yuri Y.
Sokolovsky Kirill V.
author_sort Kravchenko Evgeniya V.
collection DOAJ
description We present multi wavelength parsec-scale Faraday rotation measure properties of twenty active galactic nuclei, observed with the Very Long Baseline Array simultaneously at 1.4, 1.6, 2.2, 2.4, 4.6, 5.0, 8.1, 8.4 and 15.4 GHz in the full polarization mode. For the observed sources we construct Faraday rotation measure and Faraday-corrected linear polarization maps. Direction of electrical field in the optically thick core regions confirms bimodal distribution. No significant changes of a Faraday rotation measure transverse to the jet direction are found in any of the observed sources. We propose a new magnetic field spatial geometry reconstruction method based on core shift measurements. This technique is applied to the quasar 1004+141. Results indicate an existence of a large scale poloidal magnetic field in the jet of 1004+141.
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spelling doaj.art-399475ace40a4275a8d6ccc8324df5792022-12-21T21:04:27ZengEDP SciencesEPJ Web of Conferences2100-014X2013-12-01610700610.1051/epjconf/20136107006Faraday rotation measures in 20 AGN jets at parsec scaleKravchenko Evgeniya V.Kovalev Yuri Y.Sokolovsky Kirill V.We present multi wavelength parsec-scale Faraday rotation measure properties of twenty active galactic nuclei, observed with the Very Long Baseline Array simultaneously at 1.4, 1.6, 2.2, 2.4, 4.6, 5.0, 8.1, 8.4 and 15.4 GHz in the full polarization mode. For the observed sources we construct Faraday rotation measure and Faraday-corrected linear polarization maps. Direction of electrical field in the optically thick core regions confirms bimodal distribution. No significant changes of a Faraday rotation measure transverse to the jet direction are found in any of the observed sources. We propose a new magnetic field spatial geometry reconstruction method based on core shift measurements. This technique is applied to the quasar 1004+141. Results indicate an existence of a large scale poloidal magnetic field in the jet of 1004+141.http://dx.doi.org/10.1051/epjconf/20136107006
spellingShingle Kravchenko Evgeniya V.
Kovalev Yuri Y.
Sokolovsky Kirill V.
Faraday rotation measures in 20 AGN jets at parsec scale
EPJ Web of Conferences
title Faraday rotation measures in 20 AGN jets at parsec scale
title_full Faraday rotation measures in 20 AGN jets at parsec scale
title_fullStr Faraday rotation measures in 20 AGN jets at parsec scale
title_full_unstemmed Faraday rotation measures in 20 AGN jets at parsec scale
title_short Faraday rotation measures in 20 AGN jets at parsec scale
title_sort faraday rotation measures in 20 agn jets at parsec scale
url http://dx.doi.org/10.1051/epjconf/20136107006
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AT sokolovskykirillv faradayrotationmeasuresin20agnjetsatparsecscale