The CO-to-H2 conversion factor in high-z dusty star-forming galaxies is not required to be 0.8; intermediate to near-Galactic values (median ~4-5) remain dynamically viable.
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Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension
The CO-to-H2 conversion factor in high-z dusty star-forming galaxies is not required to be 0.8; intermediate to near-Galactic values (median ~4-5) remain dynamically viable.