Studies of the 3c 345 Quasar Structure at Dm-WavelengthsVisa övriga samt affilieringar
1987 (Engelska)Ingår i: 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, nr 121, s. 301-304Konferensbidrag, Publicerat paper (Refereegranskat)
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.
Ort, förlag, år, upplaga, sidor
Dordrecht: D. Reidel Publishing Group, 1987. Vol. 121, nr 121, s. 301-304
Serie
Symposium / International Astronomical Union, ISSN 0074-1809 ; 121
Nationell ämneskategori
Astronomi, astrofysik och kosmologi
Identifikatorer
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
Konferens
121st Symposium of the International Astronomical Union, Byurakan, Armenia, U.S.S.R., June 3-7, 1986
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