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Fig. 14

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Evolution of the semi-major axis of a planet embedded in an isothermal disk for different locations of the disk’s inner boundary. The graph in red corresponds to the standard model with an open inner boundary at 0.25 AU. The graph in blue represents a model with a closed inner boundary at 0.25 AU, and the graph in green is for a disk with an open inner boundary at 0.22 AU.

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