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Fig. 11

image

CO underabundance vs. R90, gas/R90, dust. Middle panel: models with Rc = 20 AU. Bottom panel: models with Rc = 50 AU. The observed range of R90, gas/R90, dust from Ansdell et al. (2018) is shown in grey. Top panel: histogram of the gas-to-dust ratios measured in Lupus (Ansdell et al. 2016; Miotello et al. 2017). These have been converted into an effective CO underabundance using δC,O, eff = Δgd/100, where Δgd is the gas-to-dust mass ratio.

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