Fig. 7

Measured mode linewidths versus Teff for the red giants (Teff < 5000 K) and for the main-sequence stars (Teff > 5000 K). Note the measured width for HD181907 (Teff = 4760 K) from Carrier et al. (2010). The dot-dashed line indicates the fit to the red-giant width, and the triple-dot-dashed line shows the fit to main-sequence stars.
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