All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{2410fig1.eps} \end{figure}$ Figure 1: HR diagram containing the whole sample of models considered in this work (filled circles) as well as the observational photometric error box. Dotted and dot-dashed lines correspond to non-rotating evolutionary tracks of 1.70 and $1.76~{M}_{\odot}$ models respectively. Continuous curves represent those of $1.70~{M}_{\odot}$ models with rotational velocities, from top to bottom, of 50, 100 and $150~\rm {km}~\rm {s}^{-1}$ respectively. Finally, dashed lines represent evolutionary tracks of $1.75~{M}_{\odot}$ models with rotational velocities varying, from top to bottom, of 50, 100 and $200~\rm{km}~\rm{s}^{-1}$ respectively.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{2410fig2.eps} \end{figure}$ Figure 2: Variation of the first overtone to fundamental radial period ratio as a function of the rotational velocity. For each mass considered, four curves are displayed, representing the results obtained modifying the effective temperature of models from ${T}_{{\rm eff}}=3.85$ ( bottom) to ${T}_{{\rm eff}}=3.88$ ( top) in steps of 0.01 dex.
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In the text

$\begin{figure} \par\includegraphics[width=7.7cm,clip]{2410fig3.eps} \end{figure}$ Figure 3: $\Pi _1/\Pi _0$ versus $\log\Pi_0$ . Three panels are displayed corresponding to the three masses considered in this work. For each panel, different lines represent the results obtained varying the rotational velocity from $\Omega=50~\rm {km}~\rm {s}^{-1}$ ( bottom, solid line) to $\Omega=250~\rm {km}~\rm {s}^{-1}$ ( top, dash-dotted line).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2410fig4.eps} \end{figure}$ Figure 4: Same as Fig. 2 but considering near degeneracy. $T_{\rm e,1}$ and $T_{\rm e,2}$ labels represent effective temperatures expressed in a logarithmic scale in K. The vertical thick solid line indicates the limit for which $\Pi _1/\Pi _0$ varies linearly with $\Omega$ in presence of near degeneracy (see details in text). The horizontal dashed thick line represents the observed $\Pi _1/\Pi _0$ . Finally, the shaded area represents the range of rotational velocities $\Omega$ (assuming i=90 deg).
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In the text

$\begin{figure} \par\includegraphics[width=6cm,clip]{2410fig5.eps}\hspace*{1cm} \includegraphics[width=6cm,clip]{2410fig6.eps} \end{figure}$ Figure 5: Variation of fundamental mode frequencies $\nu (\Pi _0)$ (in $\mu\mbox{Hz}$ ) with effective temperature for models with a rotational velocity of $\Omega=200~\rm {km}~\rm {s}^{-1}$ , representative of Altair. Left panel corresponds to frequencies not corrected for the effect of near degeneracy, and right panel to those corrected. Finally, the horizontal dashed line represents the frequency of the observed fundamental mode $f_0^{{\rm obs}}$ .
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{2410fig7.eps} \end{figure}$ Figure 6: HR diagram showing selected models given in Table 5. Labels correspond to model numbers. Square symbols represent models selected by the proximity to the fundamental radial mode; filled squares are used for those taking into account near degeneracy effects. Filled circles represent models selected by the minimum $\sigma ^2$ value. As a reference, observations (the cross symbol) and two evolutionary tracks are depicted: one corresponding to a $1.70~{M}_{\odot}$ and $\Omega_1=150~\rm{km}~\rm{s}^{-1}$ (solid line), and the other one, corresponding to a $1.75~{M}_{\odot}$ and $\Omega_2=200~\rm{km}~\rm{s}^{-1}$ (dashed line). For more details see the text.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{2410fig2.eps} \end{figure}$	Figure 2: Variation of the first overtone to fundamental radial period ratio as a function of the rotational velocity. For each mass considered, four curves are displayed, representing the results obtained modifying the effective temperature of models from ${T}_{{\rm eff}}=3.85$ ( bottom) to ${T}_{{\rm eff}}=3.88$ ( top) in steps of 0.01 dex.
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$\begin{figure} \par\includegraphics[width=7.7cm,clip]{2410fig3.eps} \end{figure}$	Figure 3: $\Pi _1/\Pi _0$ versus $\log\Pi_0$ . Three panels are displayed corresponding to the three masses considered in this work. For each panel, different lines represent the results obtained varying the rotational velocity from $\Omega=50~\rm {km}~\rm {s}^{-1}$ ( bottom, solid line) to $\Omega=250~\rm {km}~\rm {s}^{-1}$ ( top, dash-dotted line).
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