Fig. 4.

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Correlations between CO luminosity concentration (CCO) and molecular gas mass concentration (Cmol). Top panel:Cmol(αCO[R]) derived based on αCO(R), which is a function of radius and is set the same for all the galaxies (Eq. (6)). Bottom panel:Cmol(αCO[Z, Σ⋆]) computed based on αCO[Z, Σ⋆], which is a function of Z and Σ⋆ and varies from galaxy to galaxy (Eq. (8)). The dashed lines mark the 1 : 1 relations.
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