Table 2: Model parameters (L*, \ensuremath {T_{{\rm eff}}} and P) of both constant-opacity models (prefix "R'') and Planck mean models (prefix "P''). Columns 5 and 6 give the stellar radius, calculated from L* and \ensuremath {T_{{\rm eff}}} (Eq. (8)), and the gravitational acceleration at the location of the photosphere. The last column shows the fraction of the stellar mass contained in the model domain of the initial model for constant-opacity models and Planck mean models (the latter averaged over the carbon/oxygen ratios used), respectively. The stellar mass M* is set to $1.0~M_{\odot}$ in all models. The remaining two (out of totally six) model parameters, the carbon/oxygen ratio \ensuremath {\varepsilon _{{\rm C}}/\varepsilon _{{\rm O}}} and the piston velocity amplitude $\Delta {u}_{\rm p}$ are specified in Tables 4-6 (Sects. 4 and 5.1).
Model L* \ensuremath {T_{{\rm eff}}} P   R* $\log g_*$ $M_{{\rm e}}/M_*$
R-/P- $[L_{\odot}]$ $[\mbox{K}]$ $[\mbox{d}]$   $[R_{\odot}]$   [%]
               
07F $7.0\times10^3$ 2880 390   336 -0.61 13; 0.16
10F $1.0\times10^4$ 2790 525   428 -0.82 17; 0.16
10G $1.0\times10^4$ 2790 653   428 -0.82 17; 0.16
13F $1.3\times10^4$ 2700 650   521 -0.99 20; 0.19
13G $1.3\times10^4$ 2700 841   521 -0.99 20; 0.19


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