Fig. 10
Hertzprung-Russell diagram showing all the core-hydrogen burning inflated models, i.e with Δr/rcore> 0. Models with Δr/rcore> 5 are coloured yellow. Below the solid black line we do not find any inflated models and above the dotted black line we do not find any non-inflated models in our grid. The hot part of the S Dor instability strip is also marked (Smith et al. 2004).
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