VLBI Observations of the Gigahertz-Peaked Spectrum Galaxy PKS 1934−638

dc.contributor.authorOjha, Roopesh
dc.contributor.authorFey, Alan L.
dc.contributor.authorJohnston, Kenneth J.
dc.contributor.authorTzioumis, Anastasios K.
dc.contributor.authorReynolds, John E.
dc.date.accessioned2020-05-11T12:22:59Z
dc.date.available2020-05-11T12:22:59Z
dc.date.issued2004-04-01
dc.description.abstractWe present 8.4 GHz VLBI observations of the gigahertz-peaked spectrum source PKS 1934-638 made with the Australian Long Baseline Array. Our observations confirm the compact double nature of the source and yield measured separations of 42.7 ± 0.4 mas at epoch 2002 July and 42.6 ± 0.3 mas at epoch 2002 November, which, when combined with previous observations, yield a rate of separation of 23 ± 10 μas yr⁻¹. This result suggests that over a timescale of 32.1 yr, the separation of the two components has changed marginally. Nominally, this provides support to the emerging consensus that compact symmetric objects (CSOs) are young sources. Our measurement of hot spot separation has, to our knowledge, the longest temporal coverage for a CSO reported in the literature.en_US
dc.description.sponsorshipThis research has made use of NASA’s Astrophysics Data System Abstract Service.en_US
dc.description.urihttps://iopscience.iop.org/article/10.1086/382724en_US
dc.format.extent5 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2m6oj-rjsm
dc.identifier.citationRoopesh Ojha et al., VLBI Observations of the Gigahertz-Peaked Spectrum Galaxy PKS 1934−638, The Astronomical Journal, Volume 127, Number 4, doi: https://doi.org/10.1086%2F382724en_US
dc.identifier.urihttps://doi.org/10.1086%2F382724
dc.identifier.urihttp://hdl.handle.net/11603/18534
dc.identifier.urihttp://simbad.u-strasbg.fr/simbad/sim-ref?querymethod=bib&simbo=on&submit=submit+bibcode&bibcode=2004AJ....127.1977O
dc.identifier.urihttps://ned.ipac.caltech.edu/cgi-bin/objsearch?search_type=Search&refcode=2004AJ....127.1977O
dc.language.isoen_USen_US
dc.publisherIOPen_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.titleVLBI Observations of the Gigahertz-Peaked Spectrum Galaxy PKS 1934−638en_US
dc.typeTexten_US

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