First giant molecular cloud simulation for star formation that includes jets, radiation, winds, supernovae

Star formation is arguably the most important process in the universe. Over their lifetimes, and then with their deaths, stars produce of all the chemical elements except for hydrogen and helium (produced in the big bang). In their youth, stars nurture the birth of planets and smaller bodies, and their demise results in supernovae, super-dense bodies like black holes, neutron stars or white dwarfs, and nebulae.