Fig. 10

Solid lines show the evolution tracks for αcgm = 0.62 and αmlt = 1.68 and a mass of 2.65 M⊙. The dotted lines correspond to the same mass but αcgm = 0.77 and αmlt = 1.98. The solar-calibrated models for convection do not fit the observations. Dashed line and dot-dashed lines are 1.85 M⊙ models, respectively, for αcgm = 0.77 and αcgm = 0.62. The smaller radius object is ξ Hya and the larger one ϵ Oph.
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