Open Access
Fig. 6.
Radial mode amplitude ⟨A0, bol⟩ computed from Eq. (13) as a function of νmax with the stellar mass colour-coded. The dashed lines are the fits presented in Table 3, shown in blue for low-mass stars (M ≤ 1.2 M⊙) and in red for high-mass stars (M ≥ 1.2 M⊙). The error bars are computed in the same way as in Fig. 5.
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