Fig. 10
Absolute obliquity as a function of orbital distance, for the 68 exoplanets with a measure of the spin-orbit angle. The size of each disk corresponds to the planet mass, while its color is related to v sin i⋆ (color is black when the value is unknown). KOI-12b, which orbits a fast rotator at more than 0.1 au, is located with an arrow.
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