8-12 juin, 2014

Résumé

Galaxy Evolution in 3D

Lisa Kewley (Australian National University)

Throughout the history of the universe, shocks and large-scale gas flows have moulded the arms of spiral galaxies, formed the bulges of the most massive galaxies in the universe, fed supermassive black holes in the centres of galaxies, fuelled generation upon generation of new stars, and enriched the intergalactic medium with metals. I will discuss our current understanding of the relationship between galactic-scale outflows, star-formation, and active galactic nuclei. I will present the latest results from our large integral field surveys of nearby and high redshift galaxies which aim to reveal the relationship between galactic-scale outflows, star-formation, and active galactic nuclei in galaxies as a function of environment and redshift.
(doit être confirmé par le SOC)