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Studies of the 3c 345 Quasar Structure at Dm-Wavelengths
Space Research Institute, Russian Academy of Sciences, Moscow, Russia.
Max-Planck-Institute für Radio Astronomie, Bonn, Germany.
Max-Planck-Institute für Radio Astronomie, Bonn, Germany.
Onsala Space Observatory, Chalmers University of Technology, Gothenburg, Sweden.ORCID iD: 0000-0002-4826-019X
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1987 (English)In: Observational evidence of activity in galaxies: proceedings of the 121st Symposium of the International Astronomical Union, held in Byurakan, Armenia, U.S.S.R., June 3-7, 1986 / [ed] E. Ye. Khachikian, K.J. Fricke & J. Melnick, Dordrecht: D. Reidel Publishing Group, 1987, Vol. 121, no 121, p. 301-304Conference paper, Published paper (Refereed)
Abstract [en]

The structure of the quasar 3C 345 has been studied at 18 and 49 cm wavelengths by VLBI method. The structure has a nucleus and a jet, which changes direction with distance from the nucleus. The continuum emission of the nucleus and the jet regions correspond to a source with a large optical depth, the cut frequence goes down with increasing distance from nucleus.

Place, publisher, year, edition, pages
Dordrecht: D. Reidel Publishing Group, 1987. Vol. 121, no 121, p. 301-304
Series
Symposium / International Astronomical Union, ISSN 0074-1809 ; 121
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:hh:diva-22801ISI: A1987J075300043Libris ID: 7389660ISBN: 90-277-2473-3 ISBN: 90-277-2474-1 OAI: oai:DiVA.org:hh-22801DiVA, id: diva2:629848
Conference
121st Symposium of the International Astronomical Union, Byurakan, Armenia, U.S.S.R., June 3-7, 1986
Available from: 2013-06-17 Created: 2013-06-17 Last updated: 2015-08-18Bibliographically approved

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Bååth, L.B.

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CiteExportLink to record
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