Molecular clouds across eight galaxies are in pressure-balanced virial equilibrium, and turbulence-regulated star formation models overpredict star formation in high-pressure environments by about two orders of magnitude.
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How Galactic Environment affects the Dynamical State of Molecular Clouds and their Star Formation Efficiency
Molecular clouds across eight galaxies are in pressure-balanced virial equilibrium, and turbulence-regulated star formation models overpredict star formation in high-pressure environments by about two orders of magnitude.