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Fig. 7
Solid line: the past 100 Myr in the evolution of the stellar radius as the star evolves to the tip of the RGB. The star is evolving under the Reimers mass-loss prescription with η = 0.6. The evolution of the initial orbits of planets TYC 14221614-1 b and c are shown as dashed lines asuming their Mpsini lowest masses.
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