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Fig. 1

image

Stellar evolution tracks in the gTeff diagram for the labelled masses. The region enclosed by the thick black boundary is the gTeff range covered by the RHD simulations. Thick solid lines denote fully consistent calculations with the RHD calibrated variable αml and T(τ) relationships. The lower panel displays the evolution of αml along each track. The dotted portion of each sequence denotes the region where the αml values are extrapolated. Dashed lines in the upper panel represent tracks calculated with a constant αml = αml, ⊙ and the RHD T(τ) relationships.

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