Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of GalaxiesThis prize winning Ph. D. thesis by Chris Harrison adopts a multi faceted approach to address the lack of decisive observational evidence, utilising large observational data sets from several world leading telescopes. Developing several novel observational techniques, Harrison demonstrated that energetic winds driven by Active Galactic Nuclei (AGN) are found in a large number of galaxies, with properties in agreement with model predictions. One of the
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Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies