EDGE: from quiescent to gas-rich to star-forming low-mass dwarf galaxies
We study how star formation is regulated in low-mass field dwarf galaxies (105≤M⋆≤106M⊙), using cosmological high-resolution (3pc) hydrodynamical simulations. Cosmic reionization quenches star formation in all our simulated dwarfs, but three galaxies with final dynamical masses of 3×109M⊙ are subsequently able to replenish their interstellar medium by slowly accreting gas. Two of these galaxie
