Multi-transition CO observations reveal that the star formation-molecular gas relation becomes more linear for denser gas tracers, implying a volume density power-law index of approximately 1.5.
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COLIBRE calibrates supernova and AGN feedback parameters in multi-phase ISM cosmological simulations using emulator-based fitting to reproduce the z=0 galaxy stellar mass function and size-stellar mass relation at three resolutions.
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Constraining the Molecular Kennicutt-Schmidt Relation with Multi-Transition CO Observations of Nearby Galaxies
Multi-transition CO observations reveal that the star formation-molecular gas relation becomes more linear for denser gas tracers, implying a volume density power-law index of approximately 1.5.
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COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
COLIBRE calibrates supernova and AGN feedback parameters in multi-phase ISM cosmological simulations using emulator-based fitting to reproduce the z=0 galaxy stellar mass function and size-stellar mass relation at three resolutions.