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Fig. 1.

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Schematic view of the mass fluxes in a multi-phase gas particle. Gas cooling moves mass from the hot to the cold phase at a rate cool. Within the cold phase, an H2 reservoir begins to grow. M ˙ form H 2 $ \dot{M}_\mathrm{{form\, H_2}} $ is the H2 formation rate determined by the particle dust content and the number density of atomic hydrogen, which in turn is computed from the cold phase mass. M ˙ dest H 2 $ \dot{M}_\mathrm{{dest\,H_2}} $ is the H2 destruction rate by LW photons, which transports mass from the molecular reservoir back to the cold phase. sf is the rate at which molecular gas creates a virtual stellar phase, which is contained within the gas particle until a stellar particle is stochastically spawned. Further destruction of the molecular mass occurs due to the action of massive stars and AGN, at rates ev and f H 2 M ˙ AGN $ \mathrm{f_{H2}}\ \dot{M}_\mathrm{{AGN}} $, respectively, where fH2 represents the fraction of H2 in the cold phase. AGN also moves material from the cold to the hot phase at a rate AGN

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