Structural Variability of 3C 111 on Parsec Scales

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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.accessioned2020-04-29T14:35:45Z
dc.date.available2020-04-29T14:35:45Z
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 and multiple trailing componentsen_US
dc.description.urihttps://ojs.cvut.cz/ojs/index.php/ap/article/view/1500en_US
dc.format.extent5 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2rvo8-22bd
dc.identifier.citationC. Grossberger, M. Kadler, J. Wilms, C. Müller, T. Beuchert, E. Ros, R. Ojha, M. Aller, H. Aller, E. Angelakis, L. Fuhrmann, I. Nestoras, R. Schmidt, J. A. Zensus, T. P. Krichbaum, H. Ungerechts, A. Sievers, D. Riquelme, Structural Variability of 3C 111 on Parsec Scales, Vol 52, No 1 (2012), https://ojs.cvut.cz/ojs/index.php/ap/article/view/1500en_US
dc.identifier.urihttp://hdl.handle.net/11603/18365
dc.language.isoen_USen_US
dc.publisherActa Polytechnicaen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsPublic Domain Mark 1.0*
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleStructural Variability of 3C 111 on Parsec Scalesen_US
dc.typeTexten_US

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