Stellar evolution models with overshooting based on 3-equation non-local theories - II. Main-sequence models of A- and B-type stars

Open Access

Fig. B.1.

Comparison of the TKE as a function of fractional mass on a logarithmic scale for different values for the parameter c₄ in a 3-equation non-local 5 M_⊙ main-sequence model with limited dissipation length scale, Λ.

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