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dc.contributor.authorGrossberger , C.
dc.contributor.authorKadler , M.
dc.contributor.authorWilms , J.
dc.contributor.authorMüller , C.
dc.contributor.authorBeuchert , T.
dc.contributor.authorRos , E.
dc.contributor.authorOjha , R.
dc.contributor.authorAller , M.
dc.contributor.authorAller , H.
dc.contributor.authorAngelakis , E.
dc.contributor.authorFuhrmann , L.
dc.contributor.authorNestoras , I.
dc.contributor.authorSchmidt , R.
dc.contributor.authorZensus , J. A.
dc.contributor.authorKrichbaum , T. P.
dc.contributor.authorUngerechts , H.
dc.contributor.authorSievers , A.
dc.contributor.authorRiquelme , D.
dc.date.accessioned2017-02-03T11:17:23Z
dc.date.available2017-02-03T11:17:23Z
dc.date.issued2012
dc.identifier.citationActa Polytechnica. 2012, vol. 52, no. 1.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/66903
dc.description.abstractWe discuss the parsec-scale structural variability of the extragalactic jet 3C111 related to a major radio flux density outburst in 2007. The data analyzed were taken within the scope of the MOJAVE, UMRAO, and F-GAMMA programs, which monitor a large sample of the radio brightest compact extragalactic jets with the VLBA, the University of Michigan 26 m, the Effelsberg 100 m, and the IRAM 30m radio telescopes. The analysis of the VLBA data is performed by fitting Gaussian model components in the visibility domain. We associate the ejection of bright features in the radio jet with a major flux-density outburst in 2007. The evolution of these features suggests the formation of a leading component andmultiple trailing componentsen
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/ap/article/view/1500
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectgalaxiesen
dc.subjectindividualen
dc.subject3C111 – galaxiesen
dc.subjectactive – galaxiesen
dc.subjectjets– galaxiesen
dc.subjectnucleien
dc.titleStructural Variability of 3C 111 on Parsec Scales
dc.typearticleen
dc.date.updated2017-02-03T11:17:24Z
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License