Astronomy & Astrophysics

All Figures

$\begin{figure} \par\includegraphics[width=7.4cm,height=5cm,clip]{Fi022_f1.EPSF} \end{figure}$ Figure 1: A map of the surface radial magnetic field of AB Dor. White represents -800 G and black represents 800 G. Since AB Dor is inclined at 60 $^{\circ }$ to the observer, Zeeman-Doppler images provide only limited information in the lower hemisphere. In order to compensate for this, we have generated this combined surface map, with the 1995 map in the upper hemisphere and the 1996 map in the lower hemisphere.
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In the text

$\begin{figure} \par\subfigure[]{\includegraphics[width=5.4cm,clip]{Fi022_f2a.eps... ...\subfigure[]{\includegraphics[width=5.44cm,clip]{Fi022_f2b.epsf} }\end{figure}$ Figure 2: Emission measure images at temperatures of 10⁷ K based on the surface magnetogram shown in Fig. 1. Two rotation periods are shown: 0.54 days (left) and 0.17 days (right).
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In the text

$\begin{figure} \par\includegraphics[width=6.8cm,clip]{Fi022_f3.ps} \end{figure}$ Figure 3: Shown is the emission measure based on the magnetogram shown in Fig. 1. Results are shown for two assumed stellar inclinations, $90^{\circ }$ (solid) and $60^{\circ }$ (dashed).
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In the text

$\begin{figure} \par\includegraphics[width=7cm,clip]{Fi022_f4.ps} \end{figure}$ Figure 4: Shown is the rotational modulation of the X-ray emission measure based on the magnetogram shown in Fig. 1. Results are shown for two assumed stellar inclinations, $90^{\circ }$ (solid) and $60^{\circ }$ (dashed).
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In the text

$\begin{figure} \par\subfigure[]{\includegraphics[width=5.4cm,clip]{Fi022_f2a.eps... ...\subfigure[]{\includegraphics[width=5.44cm,clip]{Fi022_f2b.epsf} }\end{figure}$	Figure 2: Emission measure images at temperatures of 10⁷ K based on the surface magnetogram shown in Fig. 1. Two rotation periods are shown: 0.54 days (left) and 0.17 days (right).
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$\begin{figure} \par\includegraphics[width=6.8cm,clip]{Fi022_f3.ps} \end{figure}$	Figure 3: Shown is the emission measure based on the magnetogram shown in Fig. 1. Results are shown for two assumed stellar inclinations, $90^{\circ }$ (solid) and $60^{\circ }$ (dashed).
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$\begin{figure} \par\includegraphics[width=7cm,clip]{Fi022_f4.ps} \end{figure}$	Figure 4: Shown is the rotational modulation of the X-ray emission measure based on the magnetogram shown in Fig. 1. Results are shown for two assumed stellar inclinations, $90^{\circ }$ (solid) and $60^{\circ }$ (dashed).
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