Fig. 9
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Gaia DR3 measurements of vbroad versus each of the five covariates as indicated for the 1775 γ Dor (grey triangles) and 190 SPB (cyan squares) stars having these quantities available. The lower right panel shows the standard deviation of vbroad as a function of the dominant ɡ-mode amplitude. When invisible, the errors are smaller than the symbol sizes.
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