Large gaps and high accretion rates in photoevaporative transition disks with a dead zone

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Fig. 12

Effective turbulence profile for different X-ray luminosities, derived using the MRI model described in Delage et al. (in prep.). The solid and dashed lines correspond to the steady-state scenario and the Lynden-Bell & Pringle (1974) scenario, respectively. See Sect. 6.3.

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