Astronomy & Astrophysics

$\begin{figure} \par\includegraphics[angle=90,width=6.6cm,clip]{0466f1a.ps}\hspac... ...pace*{6mm} \includegraphics[angle=90,width=6.7cm,clip]{0466f1d.ps} \end{figure}$ Figure 1: Light curves of Procyon (LETGS), $\epsilon$ Eri (LETGS), $\lambda$ And (HETGS) and V851 Cen (XMM/MOS 2) with 1- $\sigma$ error bars. The upper axis reports the photometric phase ( $\epsilon$ Eri) and orbital phase ( $\lambda$ And and V851 Cen, with T₀ corresponding to secondary star located behind the primary star).
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{0466f2a.eps}\hspace*{5mm} \i... ...2c.eps}\hspace*{5mm} \includegraphics[width=8cm,clip]{0466f2d.eps} \end{figure}$ Figure 2: Element abundances in the corona of Procyon, $\epsilon$ Eri, $\lambda$ And and V851 Cen (filled circles) with respect to solar photospheric values. Open diamonds represent the stellar photospheric abundances (see text). A dashed line indicates the adopted solar photospheric abundance (Anders & Grevesse 1989).
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In the text

$\begin{figure} \par\includegraphics[width=8.1cm,clip]{0466f3a.eps}\hspace*{3mm} ... ...c.eps}\hspace*{3mm} \includegraphics[width=8.1cm,clip]{0466f3d.eps} \end{figure}$ Figure 3: Coronal to photospheric abundance ratio for Procyon, $\epsilon$ Eri, $\lambda$ And and V851 Cen, with $1\sigma$ error bars. Solar coronal (at $\log T[K]\sim 6.1$ ) to photospheric abundance ratios (Feldman & Laming 2000) are indicated with a dotted line in the Procyon plot.
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{0466f4a.eps}\hspace*{5mm} ... ...eps}\hspace*{5mm} \includegraphics[width=7.8cm,clip]{0466f4d.eps} \end{figure}$ Figure 4: Emission Measure Distribution for Procyon, $\epsilon$ Eri, $\lambda$ And and V851 Cen. Thin lines represent the relative contribution function for each ion (the emissivity function multiplied by the EMD at each point). Small numbers indicate the ionization stages of the species. Also plotted are the observed to predicted line flux ratios for the ion stages in the upper figure. The dotted lines denote a factor of 2.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=6.6cm,clip]{0466f1a.ps}\hspac... ...pace*{6mm} \includegraphics[angle=90,width=6.7cm,clip]{0466f1d.ps} \end{figure}$	Figure 1: Light curves of Procyon (LETGS), $\epsilon$ Eri (LETGS), $\lambda$ And (HETGS) and V851 Cen (XMM/MOS 2) with 1- $\sigma$ error bars. The upper axis reports the photometric phase ( $\epsilon$ Eri) and orbital phase ( $\lambda$ And and V851 Cen, with T₀ corresponding to secondary star located behind the primary star).
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$\begin{figure} \par\includegraphics[width=8cm,clip]{0466f2a.eps}\hspace{5mm} \i... ...2c.eps}\hspace{5mm} \includegraphics[width=8cm,clip]{0466f2d.eps} \end{figure}$	Figure 2: Element abundances in the corona of Procyon, $\epsilon$ Eri, $\lambda$ And and V851 Cen (filled circles) with respect to solar photospheric values. Open diamonds represent the stellar photospheric abundances (see text). A dashed line indicates the adopted solar photospheric abundance (Anders & Grevesse 1989).
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$\begin{figure} \par\includegraphics[width=8.1cm,clip]{0466f3a.eps}\hspace{3mm} ... ...c.eps}\hspace{3mm} \includegraphics[width=8.1cm,clip]{0466f3d.eps} \end{figure}$	Figure 3: Coronal to photospheric abundance ratio for Procyon, $\epsilon$ Eri, $\lambda$ And and V851 Cen, with $1\sigma$ error bars. Solar coronal (at $\log T[K]\sim 6.1$ ) to photospheric abundance ratios (Feldman & Laming 2000) are indicated with a dotted line in the Procyon plot.
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