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Fig. 6

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Radius excess δ vs. rotational period (days) for the host stars of 103 planets for which mass and radius of star and planet are given in the “Extrasolar Planets Encyclopaedia”. Open diamonds: stars earlier than F5 with planets with null orbital eccentricity; filled diamonds: stars earlier than F5 with significantly eccentric planet orbits; open circles: stars later than F5 with planets with zero orbital eccentricity; filled circles stars later than F5 that host planets with significant eccentricities.

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