Fig. 8
Measured mode amplitudes ( ∝ 
) versus L/M for the red giants (L/M > 5) and for the main-sequence stars (L/M < 5). The results of Barban et al. (in prep.) appear as filled squares. The result of Carrier et al. (2010) for HD181907 is hidden by other red-giant results. The dot-dash line indicates the global fit to red giants and main-sequence stars.
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