$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig1.ps}\end{figure}$ Figure 1: The evolutionary tracks in the HR diagram of a 8 $~M_\odot$ star for the sequences with and without rotation. The solid and dotted curves correspond to the tracks for the STD sequence and the ROT sequence, respectively.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig2.ps}\end{figure}$ Figure 2: The time dependent variation of the border of the burning core of the 8 $M_\odot$ star. The solid and dotted curves have the same meanings as in Fig. 1.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig3.ps}\end{figure}$ Figure 3: he evolution of the ratio $\langle g_{{\rm eff}} \rangle_i/g_i$ as a function of the mass fraction in the star. X(c) is the hydrogen composition at the center.
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In the text

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig1.ps}\end{figure}$	Figure 1: The evolutionary tracks in the HR diagram of a 8 $~M_\odot$ star for the sequences with and without rotation. The solid and dotted curves correspond to the tracks for the STD sequence and the ROT sequence, respectively.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig2.ps}\end{figure}$	Figure 2: The time dependent variation of the border of the burning core of the 8 $M_\odot$ star. The solid and dotted curves have the same meanings as in Fig. 1.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=270,width=8.8cm,clip]{0245fig3.ps}\end{figure}$	Figure 3: he evolution of the ratio $\langle g_{{\rm eff}} \rangle_i/g_i$ as a function of the mass fraction in the star. X(c) is the hydrogen composition at the center.
Open with DEXTER