Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{Fg163_f1.ps} \end{figure}$ Figure 1: Critical period as a function of the differential rotation parameter. The two curves refer to different values of $R_{\rm c}$ , with the solid parts corresponding to a $\alpha ^{2}$ -dynamo and the dashed parts to a $\alpha \Omega$ -dynamo.
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In the text

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{Fg163_f2.ps} \end{figure}$ Figure 2: Toroidal ( $B_{\phi }$ ) and the poloidal ( $B_{\rm p}$ ) magnetic field lines. Solid and dashed contours correspond to positive and negative values, respectively. The dot-dashed line marks the position of $R_{\rm c} = 0.6~R$ .
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In the text

$\begin{figure} \par\includegraphics[width=7.4cm,clip]{Fg163_f1.ps} \end{figure}$	Figure 1: Critical period as a function of the differential rotation parameter. The two curves refer to different values of $R_{\rm c}$ , with the solid parts corresponding to a $\alpha ^{2}$ -dynamo and the dashed parts to a $\alpha \Omega$ -dynamo.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=7.6cm,clip]{Fg163_f2.ps} \end{figure}$	Figure 2: Toroidal ( $B_{\phi }$ ) and the poloidal ( $B_{\rm p}$ ) magnetic field lines. Solid and dashed contours correspond to positive and negative values, respectively. The dot-dashed line marks the position of $R_{\rm c} = 0.6~R$ .
Open with DEXTER