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Extreme Superluminal motion in CTA102 ?
Department of Astronomy/Astrophysics, Chalmers University of Technology, Gothenburg, Sweden.
Onsala Space Observatory, Chalmers University of Technology, Gothenburg, Sweden.ORCID iD: 0000-0002-4826-019X
1993 (English)In: Sub-arcsecond Radio Astronomy: Proceedings of the Nuffield Radio Astronomy Laboratories' conference, held in Manchester, July 20–24, 1992 / [ed] R. J. Davis & R. S. Booth, Cambridge: Cambridge University Press, 1993, p. 197-198Chapter in book (Refereed)
Abstract [en]

We present observations of proper motion in five epoches of VLBI observations of CTA102. The highest observed proper motion was μ=0.64 mas/year, corresponding to a transverse velocity of v = 18.0 ± 4 c.
Place, publisher, year, edition, pages
Cambridge: Cambridge University Press, 1993. p. 197-198
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:hh:diva-22849ISI: A1993BC51K00065Libris ID: 5020268ISBN: 0-521-43472-6 OAI: oai:DiVA.org:hh-22849DiVA, id: diva2:630079
Available from: 2013-06-18 Created: 2013-06-17 Last updated: 2015-08-24Bibliographically approved

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Bååth, L.B.

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