All Tables

Table 1: Altair observed frequencies (from Paper I). From left to right, columns provide frequencies in cd^-1, in $\mu\mbox{Hz}$ , amplitudes in ppm, and finally, f₁/f_j=2,...,7 frequency ratios.
Table 2: Table containing the main characteristics of $M=1.70~{M}_{\odot}$ computed models. From left to right, $\Omega$ represents the rotational velocity in $\rm{km}~\rm{s}^{-1}$ ; ${T}_{{\rm eff}}$ the effective temperature (on a logarithmic scale); $L/L_{\odot }$ the luminosity in solar luminosities (on a logarithmic scale); $R/{R}_{\odot }$ the stellar radius in solar radii; g the surface gravity in cgs (on a logarithmic scale); the age in Myr; $\nu (\Pi _0)$ the frequency of the fundamental radial mode (in $\mu\mbox{Hz}$ ) and finally, $\Pi _1/\Pi _0$ represents the ratio between periods of the first overtone and the fundamental radial mode. Variables indexed with a d represent the same quantities obtained when including near-degeneracy effects.
Table 3: Idem Table 2 for $M=1.75~{M}_{\odot}$ models.
Table 4: Idem Table 2 for $M=1.76~{M}_{\odot}$ models.
Table 5: Table containing a proposed mode identification for the observed frequencies given in Table 1, using the oscillations computed from different models. Values in parentheses correspond to the mode identification numbers ( $n,\ell ,m$ ). The first five models corresponds to those chosen by their proximity to the fundamental radial mode. The last five, corresponds to those chosen by minimum $\sigma ^2$ value. $\nu _i$ represent the theoretical frequencies closest to the observed ones.