The multiple routes of galaxy transformation across the cosmic epochs
In the local universe most of the stellar mass is in passive galaxies, where star formation is
absent or at very low levels. Understanding what are the mechanisms that have been
responsible for quenching star formation in galaxies, and transforming them into passive,
quiescent systems, is one of the main observational and theoretical challenges of extragalactic
astrophysics. I will give a brief overview of the several possible quenching causes and physical
processes that have been proposed so far, ranging from feedback from black hole accretion and
starburst activity, to effects associated with the large scale environment in which galaxies live.
Although most of these mechanisms and causes play a role in different classes of galaxies and
at different epochs, multi-band observations are providing growing evidences that just a few of
them play the key, dominant role.
I will conclude by providing prospects for further investigating these aspects and tackling open
questions with the next generation of observing facilities.
About the talk
turbulence, shock waves, radiative transfer, molecular gas, hydrodynamics, gravitation, black holes, accretion, accretion discs, supermassive black hole, SMBH, stellar content, starburst galaxies, star forming galaxies, quasars, Morphologies, massive galaxies, late-type galaxies, intergalactic medium, galaxy evolution, galactic nuclei, galactic formation, galactic classification, elliptical galaxies, early-type galaxies, cooling flows, active galaxies, SDSS, science