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. 8.

Surface angular velocity evolution for HD 64121 (TIC 264770836) in the case of fast rotator (Ω_in = 18 × Ω_⊙, black solid line), a medium rotator (Ω_in = 5 × Ω_⊙, blue solid line) and a slow rotator (Ω_in = 3.2 × Ω_⊙). The red dashed line represents the critical velocity limit. The black dotted vertical line indicates the age of the system.

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