Mixed-mode coupling in the red clump - I. Standard single star models

Open Access

Fig. 12.

Power-law exponents $β_{\tilde{S}}$ $\beta_{\tilde{S}}$ and $β_{\tilde{N}}$ $\beta_{\tilde{N}}$ as a function of s of model C are shown as solid blue and orange lines respectively. The values of $β_{\tilde{S}}$ $\beta_{\tilde{S}}$ and $β_{\tilde{N}}$ $\beta_{\tilde{N}}$ used in the power-laws are shown as the horizontal dashed blue and orange lines respectively. The vertical grey dashed lines show the boundaries of the evanescent zone, ±s₀.

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