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$\begin{figure} \par {\includegraphics[width=8.2cm,clip]{hg282_f1.eps} } \end{figure}$ Figure 1: Horizontal component of the eigenfunction $\xi _{\rm h}$ (scaled such that $\xi _{\rm r} = 1$ at the surface) as a function of normalized radius (r/R) for a g₂₀¹ mode with a period of 1.5 d for a 4 $M_\odot$ SPB star of 94 Myr. The inset shows an enlargement of the region close to the edge of the convective core, where the eigenfunction displays strong oscillations due to the presence of a steep composition gradient.
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In the text

$\begin{figure} \par {\includegraphics[width=7.9cm]{hg282_f2.eps} } \end{figure}$ Figure 2: Same as in Fig. 1, but for the g₁₀¹ mode. The inset shows an enlargement of the region close to the convective core.
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In the text

$\begin{figure} \par {\includegraphics[width=7.9cm]{hg282_f2.eps} } \end{figure}$	Figure 2: Same as in Fig. 1, but for the g₁₀¹ mode. The inset shows an enlargement of the region close to the convective core.
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