Speaker
Peter Creasey
(University of California at Riverside (UCR))
Description
The mechanisms of feedback in which Milky-Way and smaller galaxies are regulated by
events on scales of parsecs and below is still poorly understood. In this talk I will
look at hydrodynamical simulations on cosmological and interstellar medium scales and
tease out some of the dynamical and chemical indicators at small and large (galaxy
population) scales that can be used to identify the culprits of the low efficiency of
star formation.
Primary author
Peter Creasey
(University of California at Riverside (UCR))
