All Tables

Table 1: Adopted constraints for our models of Procyon A: mass $M_\star$ , effective temperature $T_{\rm eff}$ , radius $R_\star$ , surface metallicity ${\rm [{Fe/ H}]_s}$ , and galactic enhancement ${\Delta Y/\Delta Z}$ .
Table 2: Global parameters of models differing by the way diffusion is treated varying the additional mixing parameter: (a) MS model of mass M = 1.46 $M_\odot$ , (b) PoMS model of mass M = 1.38 $M_\odot$ .
Table 3: Global parameters of models differing by the way convection is treated: the Canuto & Mazitelli theory and $\lambda = 1.$ , and the classical mixing length theory with $\lambda = 1.9, 1.7$ . (a) MS models $M_\star = 1.46~M_\odot$ , (b) PoMS models $M_\star = 1.38~M_\odot$ ).