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Fig. 12
Visibility of the ℓ = 1, 2 and 3 modes (from top to bottom), as a function of the effective temperature. Same color code as in Fig. 11. Dashed lines are the fits derived from Ballot et al. (2011). Blue and red solid lines are the fits for RGB and clump stars, respectively.
This figure is made of several images, please see below:
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