Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 433, Issue 3, Pages 1910-1929Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stt851
Keywords
galaxies: evolution; galaxies: high-redshift; galaxies: ISM; galaxies: star formation
Categories
Funding
- NASA [HF-51304.01-A, NAS 5-26555]
- Space Telescope Science Institute
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Observations show that star formation in galaxies is closely correlated with the abundance of molecular hydrogen. Modelling this empirical relation from first principles proves challenging, however, and many questions regarding its properties remain open. For instance, the exact functional form of the relation is still debated and it is also unknown whether it applies at z > 4, where carbon monoxide observations are sparse. Here, we analyse how the shape of the star formation-gas relation affects the cosmic star formation history and global galaxy properties using an analytic model that follows the average evolution of galaxies in dark matter haloes across cosmic time. We show that a linear relation with an H-2 depletion time of similar to 2.5 Gyr, as found in studies of nearby galaxies, results in good agreement with current observations of galaxies at both low and high redshift. These observations include the evolution of the cosmic star formation rate density, the z similar to 4-9 UV luminosity function, the evolution of the mass-metallicity relation, the relation between stellar and halo mass, and the gas-to-stellar mass ratios of galaxies. In contrast, the short depletion times that result from adopting a highly super-linear star formation-gas relation lead to large star formation rates, substantial metal enrichment (similar to 0.1 Z(circle dot)) and low gas-to-stellar mass ratios already at z greater than or similar to 10, in disagreement with observations. These results can be understood in terms of an equilibrium picture of galaxy evolution in which gas inflows, outflows and star formation drive the metallicities and gas fractions towards equilibrium values that are determined by the ratio of the accretion time to the gas-depletion time. In this picture, the cosmic modulation of the accretion rate is the primary process that drives the evolution of stellar masses, gas masses and metallicities of galaxies from high redshift until today.
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