All Tables

Table 1: Observed periods in G 185-32.
Table 2: Impact of $T_{\rm eff}$ variation on the $\ell =2$ , k=1 and $\ell =2$ , k=10 modes.
Table 3: Potential solutions in the $\log q$ (H) vs. $M_{\star }$ plane derived from the reference mode with $T_{\rm eff}$ and q(He) constant.
Table 4: Structural parameters for the best fitting model.
Table 5: $\ell =1$ modes for the best fitting model.
Table 6: $\ell =2$ modes for the best fitting model.
Table 7: Preliminary identification of the modes observed in G 185-32. The first column gives the observed periods, the second one the spherical degree ( $\ell$ ) of the mode, the third its radial order (k), the fourth gives the value of the corresponding period computed from the best-fit model, the fifth gives the absolute difference between the two periods, and the sixth their relative difference.
Table 8: Full identification of the observed modes in G 185-32.