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dc.contributor.author Britzen S.
dc.contributor.author Fendt C.
dc.contributor.author Witzel G.
dc.contributor.author Qian S.J.
dc.contributor.author Pashchenko I.N.
dc.contributor.author Kurtanidze O.
dc.contributor.author Zajacek M.
dc.contributor.author Martinez G.
dc.contributor.author Karas V.
dc.contributor.author Aller M.
dc.contributor.author Aller H.
dc.contributor.author Eckart A.
dc.contributor.author Nilsson K.
dc.contributor.author Arévalo P.
dc.contributor.author Cuadra J.
dc.contributor.author Subroweit M.
dc.contributor.author Witzel A.
dc.date.accessioned 2021-02-25T20:46:18Z
dc.date.available 2021-02-25T20:46:18Z
dc.date.issued 2020
dc.identifier.issn 1743-9213
dc.identifier.uri https://dspace.kpfu.ru/xmlui/handle/net/162382
dc.description.abstract © International Astronomical Union 2020. We re-analyzed OJ287 in 120 Very Long Baseline Array (VLBA, MOJAVE) observations (at 15 GHz) covering the time span between Apr. 1995 and Apr. 2017. We find that the radio jet motion over the sky is consistent with a precessing and nutating jet source. The variability of the radio flux-density can be explained by Doppler beaming due to a change in the viewing angle. We suggest that part of the optical emission is due to synchrotron emission related to the jet radiation. We find a strikingly similar scaling for the timescales for precession and nutation as indicated for SS433 with a factor of roughly 50 times longer in OJ287.
dc.relation.ispartofseries Proceedings of the International Astronomical Union
dc.subject BL Lacertae objects: Individual (OJ 287)
dc.subject galaxies: Jets
dc.subject techniques: Interferometric
dc.title A precessing and nutating jet in OJ287
dc.type Article
dc.collection Публикации сотрудников КФУ
dc.relation.startpage 250
dc.source.id SCOPUS17439213-2020-SID85083422319


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  • Публикации сотрудников КФУ Scopus [24551]
    Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.

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