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Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies
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Observational Constraints on the Influence of Active Galactic Nuclei on the Evolution of Galaxies

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. Leading theoretical models predict that AGN drive energetic winds into galaxies, regulating the formation of stars.
Painos
Softcover reprint of the original 1st ed. 2016
ISBN
9783319803579
Kieli
englanti
Paino
310 grammaa
Julkaisupäivä
30.3.2018
Sivumäärä
193