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Fig. 7
Frequency of the dominant mode as a function of vsini for δ Sct stars from the catalogues of Rodríguez et al. (2000, top and Uytterhoeven et al. (2011, bottom. The solid line represents a linear function fit to the shown data points. Detailed information on individual stars is provided in Table A.1.
This figure is made of several images, please see below:
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