Molecular clouds and the origins of feedback in galaxies
Room: 100
Department of Physics and Astronomy
PHYSICS & ASTRONOMY COLLOQUIUM
Dr. Brian McNamara
Department of Physics & Astronomy
University of Waterloo
“Molecular clouds and the origins of feedback in galaxies”
ABSTRACT
Galaxies owe much of their structure and appearance to physical processes resulting from energetic feedback from supernovae, starburst winds, and massive black holes. In the largest galaxies, nuclear supermassive black holes are the dominant energy source. I will discuss recent progress in understanding how feedback from active galactic nuclei both sustains and regulates itself by heating the hot atmospheres surrounding galaxies and by inducing thermally-unstable, cooling gas that fuels star formation and the feedback engine itself.