LYRA. III. The Smallest Reionization Survivors

The dividing line between galaxies that are quenched by reionization (relics) and galaxies that survive reionization (i.e., continue forming stars) is commonly discussed in terms of a halo mass threshold. We probe this threshold in a physically more complete and accurate way than has been possible to date, using five extremely high resolution (M (target) = 4 M (circle dot)) cosmological zoom-in simulations of dwarf galaxies within the halo mass range (1-4) x 10(9) M (circle dot). The employed LYRA simulation model features resolved interstellar medium physics and individual, resolved supernova explosions. Interestingly, two out of five of the simulated dwarf galaxies lie close to the threshold mass but are neither full reionization relics nor full reionization survivors. These galaxies initially quench at the time of reionization but merely remain quiescent for similar to 500 Myr. At z similar to 5 they recommence star formation in a synchronous way and remain star-forming until the present day. The parallel timing indicates consistent sound-crossing and cooling times between the halos. While the star formation histories we find are diverse, we show that they are directly related to the ability of a given halo to retain and cool gas. Whereas the latter is most strongly dependent on the mass (or virial temperature) of the host halo at the time of reionization, it also depends on its growth history, the UV background (and its decrease at late times), and the amount of metals retained within the halo.

Automated summary

The ability of galaxies to continue forming stars after reionization is related to their host halo's mass, growth history, UV background, and retained metals.