Fig. 9
Hill-normalized accretion rates for a planet of thermal mass 
and η∕hgas = 0.1. Data points give kabs obtained from hydrodynamical laminar (2D), ideal MRI (ID), and resistive (ambipolar diffusion) MRI (AD) simulations reported by Xu et al. (2017). Solid lines give our fits, where we adopt σ from the same simulations. Data kindly provided by Ziyan Xu.
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