Interior dynamics of envelopes around disk-embedded planets

Open Access

Fig. 7

Same as Fig. 5 but for β=10² and 10³. The convective, radiative, and recycling layers are qualitatively indicated. The dashed red and yellow curves show Eq. (24), under the assumptions of fully and partially convective envelopes with l_m=R_B and l_m=0.2 R_B, respectively.

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