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An Asymmetric Relativistic Model for FRII Radio Sources

Published online by Cambridge University Press:  25 May 2016

T. G. Arshakian
Affiliation:
Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE
M. S. Longair
Affiliation:
Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE

Abstract

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An asymmetric relativistic model for FRII radio sources is described which takes account of both relativistic effects and intrinsic/environmental asymmetries to explain the observed structural asymmetry of their radio lobes. A key feature of the model is jet-sidedness, which can now be determined for about 80% of the FRII sources in the 3CRR complete sample. It is shown that a simple asymmetric relativistic model can account for a wide range of observational data, and that the relativistic and intrinsic asymmetry effects are of comparable importance. The mean translational speed of the lobes is . The results are in agreement with an orientation-based unified scheme in which the critical angle separating the radio galaxies from the radio quasars is about 50°.

Type
III. AGN Theory and Models
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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