The goal of IAU Symposium 359 on 'Galaxy Evolution and Feedback
across Different Environments' (GALFEED) was to bring together the
active galactic nuclei (AGN) and galaxy evolution scientific
communities. The AGN phase occurs in most galaxies and critically
influences their evolution, so it is important to study the two
processes together and for researchers, in both topics, to learn
from one another. They ask key questions such as: How do galaxies
acquire their gas and how efficiently is it transformed into stars?
How is the supermassive black hole in a galaxy center fuelled to
become an AGN? What is the main physical mechanism that quenches
star formation? How powerful are the stellar and AGN feedback
processes in regulating galaxy evolution? And what is the role of
the environment on galaxy evolution and AGN triggering? Astronomers
engage in these discussions spanning from early galaxies to the
present day.
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