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Fig. 1


Main sequence showing the Geneva stellar evolution tracks for solar metallicity as presented in Mowlavi et al. (2011) and plotted using R   (in R) as a function of Teff. Tracks are labelled in units of M. Dashed line show the 2 Gyr isochrone. Overplotted are the systems for which we have Rossiter-McLaughlin measurements. Aligned systems are red circles, misaligned systems are blue triangles. Higher metallicities will move the tracks to the right. Data obtained from Exoplanet.eu.

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