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. 5.

Evolutionary tracks in the Hertzsprung-Russell diagram of a 5 M_⊙ model computed with MLT (yellow line), ad hoc overshooting (black line), the 3-equation, non-local model (blue line) and the 1-equation, non-local model (red line). The black dot marks the model selected at a central hydrogen abundance of X_c = 0.6.

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