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Fig. 14


Vertical velocities in z-direction for planets on fixed circular orbits in fully radiative discs with different disc masses (from top to bottom) in the disc’s midplane: MDisc = 0.005 M, MDisc = 0.015 M and MDisc = 0.04 M. The disruption in the velocity patterns for the higher mass discs are caused by convection inside the disc. A positive velocity simulates outward flows, while a negative velocity indicates a flow towards the disc’s midplane.

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