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Fig. D.2

image

Detailed structure examples for stellar models with an effective temperature near 25 000 K, for three different luminosities (cf. Fig. 2). The dashed line marks the point at which β falls below 0.15, i.e. the beginning of the inflated envelope. The square and the cross mark the temperatures TFe and TFe at which κ is maximum because of the iron and the helium opacity bumps respectively. The hatched regions show the convective zones.

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