Spine-sheath polarization structures in four active galactic nuclei jets
dc.contributor.author | Pushkarev, A. B. | |
dc.contributor.author | Gabuzda, Denise | |
dc.contributor.author | Vetukhnovskaya, Y. N. | |
dc.contributor.author | Yakimov, V. E. | |
dc.contributor.funder | Russian Foundation for Basic Research | |
dc.contributor.funder | International Association for the Promotion of Cooperation with Scientists from the New Independent States | |
dc.date.accessioned | 2017-11-07T09:38:58Z | |
dc.date.available | 2017-11-07T09:38:58Z | |
dc.date.issued | 2005 | |
dc.description.abstract | We present the results of multifrequency (15 + 8 + 5 GHz) polarization Very Long Baseline Array (VLBA) observations of the three BL Lacertae objects 0745 + 241, 1418 + 546 and 1652 + 398 together with 5-GHz VLBI Space Observatory Programme (VSOP) observations of 1418 + 546 and 1.6- and 5-GHz VSOP observations of the blazar 1055 + 018. The jets of all these sources have polarization structure transverse to the jet axis, with the polarization E vectors aligned with the jet along the jet spine and 'sheaths' of orthogonal E vectors at one or both edges of the jet. The presence of polarization aligned with the jet near the 'spine' may indicate that the jets are associated with helical B fields that propogate outward with the jet flow; the presence of orthogonal polarization near the edges of the jet may likewise be a consequence of a helical jet B field, or may be owing to an interaction with the ambient medium on parsec scales. We have tentatively detected interknot polarization in 1055 + 018 with E aligned with the local jet direction, consistent with the possibility that the jet of this source is associated with a helical B field. | en |
dc.description.sponsorship | Russian Foundation for Basic Research (project code No. 02-02-16305); International Association for the Promotion of Cooperation with Scientists from the New Independent States (Grant No. 2001–0669) | |
dc.description.status | Peer reviewed | en |
dc.description.version | Published Version | en |
dc.format.mimetype | application/pdf | en |
dc.identifier.citation | Pushkarev, A. B., Gabuzda, D. C., Vetukhnovskaya, Y. N. and Yakimov, V. E. (2005) 'Spine–sheath polarization structures in four active galactic nuclei jets', Monthly Notices of the Royal Astronomical Society, 356(3), pp. 859-871. doi: 10.1111/j.1365-2966.2004.08535.x | en |
dc.identifier.doi | 10.1111/j.1365-2966.2004.08535.x | |
dc.identifier.endpage | 871 | |
dc.identifier.issn | 0035-8711 | |
dc.identifier.issued | 3 | |
dc.identifier.journaltitle | Monthly Notices of the Royal Astronomical Society | en |
dc.identifier.startpage | 859 | |
dc.identifier.uri | https://hdl.handle.net/10468/4986 | |
dc.identifier.volume | 356 | |
dc.language.iso | en | en |
dc.publisher | Oxford University Press | en |
dc.relation.uri | https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2004.08535.x | |
dc.rights | © 2004, Royal Astronomical Society | en |
dc.subject | Magnetic fields | en |
dc.subject | Polarization | en |
dc.subject | BL Lacertae objects | en |
dc.subject | General | en |
dc.title | Spine-sheath polarization structures in four active galactic nuclei jets | en |
dc.type | Article (peer-reviewed) | en |
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