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Monthly Notices of the Royal Astronomical Society 474 (3) 3110 (2018)
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The Initial Conditions for Planet Formation: Turbulence Driven by Hydrodynamical Instabilities in Disks around Young Stars

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Suppression of atmospheric recycling of planets embedded in a protoplanetary disc by buoyancy barrier

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The Planetary Accretion Shock. II. Grid of Postshock Entropies and Radiative Shock Efficiencies for Nonequilibrium Radiation Transport

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Disk Evolution and the Fate of Water

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Zombie Vortex Instability. III. Persistence with Nonuniform Stratification and Radiative Damping

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Mapping the Conditions for Hydrodynamic Instability on Steady-State Accretion Models of Protoplanetary Disks

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From Protoplanetary Disks to Planet Formation

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Effect of Different Angular Momentum Transport Mechanisms on the Distribution of Water in Protoplanetary Disks

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