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Radio Source Evolution & Unified Schemes

C A Jackson1

Department of Astrophysics, School of Physics, University of Sydney, NSW 2006
cjackson@physics.usyd.edu.au

Abstract:

Powerful extragalactic radio sources are characterised by kpc-scale synchrotron emission associated with highly-collimated outflows of relativistic plasma. It is hypothesized that this outflowing plasma is powered by accretion processes concomitant with a central massive black hole. The radio morphologies of these sources comprise jets, lobes and for the most powerful sources, hotspots. At first sight, powerful extragalactic radio sources are a mixed group of objects, with the result that only some gross property delineates them further (e.g. steep-spectrum or flat-spectrum). However, there is accumulating observational evidence which suggests that it is the orientation of the radio axis to our line-of-sight which dictates their observed characteristics. This orientation-dependence has been incorporated into `unified schemes', which physically-link apparently disparate radio source types via the random orientation of a `parent' population on the plane of the sky. This paper summarises the `dual-population unified scheme' paradigm investigated by and discusses some of its implications with respect to radio source cosmology.

Keywords:galaxies:evolution, galaxies:jets, quasars:general, radio continuum:galaxies





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Next: Extragalactic radio sources: What

Amelia Ortiz-Gil
1999-04-12
ASKAP
Public