Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations

Cinthia Ragone-Figueroa, Gian Luigi Granato, Massimiliano Parente +4

Context: Molecular hydrogen (${\mathrm{H}}_2$) is crucial in galaxy formation and evolution, serving as the main fuel for star formation (SF). In metal-enriched environments, ${\mathrm{H}}_2$…