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Fig. 3

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a) The distribution of projected rotational velocities vsini is shown for those stars for which measurements could be obtained from the analysis of the zeros of the Fourier transform of the overall broadening profile. Mesurements with upper limits on vsini are omitted. The grey-shaded area represents the distribution of the sample of the previous work (Reiners et al.), the hashed area the sample of the present work. The white area shows the distribution of the combined sample. b) The distribution of measurements of is shown for the stars with resolved rotational profiles. The layout follows a).

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