Kavli Affiliate: Roberto Maiolino | First 5 Authors: , , , , | Summary: Stars in galaxies form when baryons radiatively cool down and fall into gravitational wells whose mass is dominated by dark matter. Eventually, star formation quenches as gas is depleted and/or perturbed by feedback processes, no longer being able to collapse and […]
Continue.. Accelerated quenching and chemical enhancement of massive galaxies in a $zsim4$ gas-rich halo