Fig. 7.
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Properties of the exoplanets with known mass around stars with 0.6 ≤ M ≤ 2.5 M⊙ and R ≥ 4 ≤ R R⊙. Mass of the host star as a function of the semi-major axis of the planet. The color code represents the decimal logarithm of the mass of the planet, in Jupiter masses. The horizontal dashed lines indicate a mass of M = 1.5 M⊙. Green and magenta lines and dots indicate the radius at TAMS and TRGB, respectively, for models of M = {1, 1.3, 1.6, 1.9, 2.2, 2.5}M⊙. The vertical continuous line indicates a radius of R = 15 R⊙.
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