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Fig. 10
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Growth and migration of individual protoplanets at different disk locations around stars of M⋆ = 0.1 M⊙ in a pure stellar irradiation disk with L⋆ = 0.01 L⊙ (top) and in a viscously heated and stellar irradiated disk with L⋆ = 0.1 L⊙ (bottom). The model parameters are similar to that in Fig. 2f (see Table 2).
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