Fig. 5
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Growth tracks of a single planet injected at r = 3 AU and t = 104 yr. In the irradiated case (left), this results in the formation of a super-Earth at the inner disc edge for all stellar masses and disc sizes. In the viscous heating case (right), the protoplanet grows into a giant planet for high stellar masses as well as for solar-mass stars with sufficiently large discs.
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