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A Cocoon Transparency and the 3C 345 Low Frequency Variability

Published online by Cambridge University Press:  25 May 2016

L.I. Matveenko*
Affiliation:
Space Research Institute of RAS, Profsojuznaja 84/32, 117810 Moscow, Russia

Abstract

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The structure of the quasar 3C 345 is studied at λ = 49cm. The core has a low-frequency cut off spectrum and α ≃ 3. The brightest knot is in the nearest part of the jet. The cocoon wall absorbs low-frequency emission and changes the polarization orientation, RM = 3500 rad m–2, B|| 100 μG at the core region.

Type
Radio Source Modelling and Emission Mechanisms
Copyright
Copyright © Kluwer 1996 

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