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Fig. 1.

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Upper panel: HR diagram of different evolutionary tracks for the different radiative acceleration methods – the default method (gray line), models with DT, Fe (blue line), and the SVP method (red line). Lower panels: Difference for the 1.4 M models for the different methods, for effective temperature (middle panel) and luminosity (bottom panel) as a function of the central hydrogen mass fraction. The black circles are the differences between the default method and the DT, Fe, the purple squares the differences between the default method and the SVP method, and the orange diamonds the differences between DT, Fe and the SVP method.

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