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The role of velocity dispersion in the Kennicutt-Schmidt relation
The resolved Kennicutt-Schmidt (KS) relation is a power-law relation between the surface densities of the star formation rate ($Σ_\mathrm{SFR}$) and molecular gas ($Σ_\mathrm{mol}$) in star-forming galaxies on kiloparsec scales. Despite its apparent simplicity, it exhibits substantial scatter, sugge
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