Different dust and gas radial extents in protoplanetary disks: consistent models of grain growth and CO emission

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Fig. 17

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Ratio derived for the models using the disk parametrisation of de Gregorio-Monsalvo et al. (2013), with a 0.52″ synthetic beam. The quantity is derived assuming a dynamic range of 30 for ¹²CO and a dynamic range of 10 for ¹³CO and C¹⁸O. For the continuum at 850 μm, the assumed dynamic range is 30. For all isotopologues, the ratio is a steep increasing function of disk turbulence.

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