Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
We present a suite of cosmological radiation-hydrodynamical simulations of the assembly of galaxies driving the reionization of the intergalactic medium (IGM) at z ≳ 6. The simulations account for the hydrodynamical feedback from photoionization heating and the explosion of massive stars as supernovae (SNe). Our reference simulation, which was
Pawlik, A. H. et al.
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2015