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GPS and CSS Sources — Theory and Modelling

Published online by Cambridge University Press:  05 March 2013

Geoffrey V. Bicknell ,
Curtis J. Saxton  and
Ralph S. Sutherland
Geoffrey V. Bicknell
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia. geoff@mso.anu.edu.au Department of Physics and Theoretical Physics, Australian National University, Canberra, ACT 0200, Australia
Curtis J. Saxton
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia. geoff@mso.anu.edu.au Department of Physics and Theoretical Physics, Australian National University, Canberra, ACT 0200, Australia
Ralph S. Sutherland
Affiliation:
Research School of Astronomy and Astrophysics, Australian National University, Mt Stromlo Observatory, Cotter Road, Weston, ACT 2611, Australia. geoff@mso.anu.edu.au
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Abstract

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We review theoretical ideas that seem to be currently important for the physics of GPS and CSS radio sources. These include models for their evolution, the production of emission lines, and the origin of the low frequency turnover. We also describe the initial phases of a program of simulations that is aimed at understanding the radiative interactions between jets, lobes, and dense clouds in the nuclei of these objects.

Keywords

galaxies: ISMgalaxies: jetsradio continuum: galaxies

Information

Type
GPS/CSS Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 1 , 2003 , pp. 102 - 109
Copyright
Copyright © Astronomical Society of Australia 2003

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