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The Jets of Quasars 3C 345 and 1803+784

Published online by Cambridge University Press:  25 May 2016

L. I. Matveenko  and
A. I. Witzel
L. I. Matveenko
Affiliation:
Space Research Institute, Profsojuznaja 84/32, Moscow 117810 Russia, e-mail:lmatveen@mx.iki.rssi.ru
A. I. Witzel
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany, e-mail: p0103wzl@mpifr-bonn.mpg.de

Abstract

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We have studied the structures of AGN objects 3C345 and 1803+784. The objects have one sided jets with conic helix structure, determining step and diameter of the helix. The jets are surrounded by cocoon - thermal plasma, the transparency of which determines low frequency variability and absorption of the core emission.

Type
III. AGN Theory and Models
Information
Symposium - International Astronomical Union , Volume 194: Activity in Galaxies and Related Phenomena , 1999 , pp. 229 - 234
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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