THE IMPACT of STELLAR FEEDBACK on the STRUCTURE, SIZE, and MORPHOLOGY of GALAXIES in MILKY-WAY-SIZED DARK MATTER HALOS
We use cosmological zoom-in simulations of galaxy formation in a Milky-Way-sized halo started from identical initial conditions to investigate the evolution of galaxy sizes, baryon fractions, morphologies, and angular momenta in runs with different parameters of the star formation-feedback cycle. Our fiducial model with a high local star formation efficiency, which results in efficient feedback, p
