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Fig. 3

image

Left panel: relation between νmax and the mean frequency of the envelope for δ Scuti stars (green triangles). The black line points to the 1:1 relation. Blue dashed lines are the limits for a significant departure from the solar case (3σ, see text). Right panel: distribution of stars according to their asymmetry (black histogram). The blue (red) histogram denotes the proportion of stars whose νmax deviation from the mean frequency of the envelope towards lower (higher) frequencies is significantly higher than the solar case (see text).

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