A memory-timescale prescription for the dynamical corotation torque lets 1D models reproduce 2D hydrodynamic migration of low-mass planets in low-viscosity discs.
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The importance of the dynamical corotation torque for the migration of low-mass planets -- 1D analytical prescriptions verified by 2D hydrodynamical simulations
A memory-timescale prescription for the dynamical corotation torque lets 1D models reproduce 2D hydrodynamic migration of low-mass planets in low-viscosity discs.