A measured correlation between most massive core mass and bound gas mass, combined with an assumed 30% efficiency and a theoretical SFR-most massive star relation, reproduces the approximately linear Gao-Solomon law.
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Why is the Star Formation Rate Proportional to Dense Gas Mass?
A measured correlation between most massive core mass and bound gas mass, combined with an assumed 30% efficiency and a theoretical SFR-most massive star relation, reproduces the approximately linear Gao-Solomon law.