Radio Galaxy Spectra

Abstract

Radio spectra of radio galaxies are often ascribed a simple power law form (Sν να) with the spectral index, α, being of order -0.7. However, all radio galaxies deviate from this simple power law behaviour. In this paper we derive simple expressions for the average rest-frame spectra of FRI and FRII radio galaxies. These will be used to describe the spectral curvature of the parent (FRI and FRII) populations in models of radio source evolution.

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