SILCC: Evolution of a supernova driven ISM including chemical evolution, stellar winds and radiation transfer  (Peters, Naab, el al. 2017)

Evolution of a dwarf galaxy with a supernovae driven interstellar medium with molecule formation, feedback from individual massive stars and varying interstellar radiation field (Hu, Naab, et al. 2017).

Evolution of a dwarf galaxy with a supernovae driven interstellar medium. From left to right: Column density of hydrogen, molecular hydrogen, and ionized hydrogen (Hu, Naab et al. 2016).