Fig. 9.
Relation of dust mass to X-ray luminosity. This figure shows the variation of the dust-to-stellar mass ratio as a function of the X-ray photon rate per dust grain, for the sample of Table 4. This is a subset of the reference run (Sect. 3.2). The color convention is similar to Fig. 8. The Bayesian correlation coefficient of this relation is 
, with CR95%(ρ) = [−0.62, −0.56].
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