CORALIE radial velocity search for companions around evolved stars (CASCADES) - II. Seismic masses for three red giants orbited by long-period massive planets

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Fig. 9.

Impact of a change in orbital distance (blue solid lines) for HD 64121b, for a host-star initial surface rotation of Ω_in = 5 × Ω_⊙. The magenta area shows extension of the stellar convective envelope, while the cyan area represents the extension of the stellar core.

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