All Figures

$\begin{figure} \par\includegraphics[angle=-90,width=8.6cm,clip]{3905fig1.eps} \end{figure}$ Figure 1: Excitation potential vs. abundance for the final values of $T_{{\rm eff}}$ and $\ensuremath{\log g}$ of HD 74044. Open circles - Fe I, filled circles - Fe II. A least squares linear regression yields: abn = -0.0002 $\chi _{{\rm excit}}$ - 4.18.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3905fig2.eps} \end{figure}$ Figure 2: Comparison of the abundances in HD 74044 (open circles) with those of the CP star HD 74169 (open triangles, Lüftinger, in prep.) and to the mean of the other members of IC 2391 (filled circles). Abundances are in units of $[{N_{{\rm El}}}/{N_{{\rm tot}}}]$ - $[{N_{{\rm El}}}/{N_{{\rm tot}}}]$ $_{\odot }$ (solar abundances according to Grevesse and Sauval 1998). Error bars indicate maximum deviations from the mean.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3905fig3.eps} \end{figure}$ Figure 3: Elemental abundances relative to the sun. Solar values according to Grevesse & Sauval (1998). Data points of elements with consecutive atomic numbers are connected with lines. Errors as in Table 3.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3905fig4.eps} \end{figure}$ Figure 4: Mean abundance pattern of IC 2391 (HD 74044 excluded) derived in this work compared to the abundance pattern found for field stars by Hill & Landstreet (1993) and Hill (1995). Elemental abundances are relative to the sun with solar values according to Grevesse and Sauval (1998). Data points of elements with consecutive atomic numbers are connected with lines. Error bars are variances of the mean abundances.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.6cm,clip]{3905fig1.eps} \end{figure}$	Figure 1: Excitation potential vs. abundance for the final values of $T_{{\rm eff}}$ and $\ensuremath{\log g}$ of HD 74044. Open circles - Fe I, filled circles - Fe II. A least squares linear regression yields: abn = -0.0002 $\chi _{{\rm excit}}$ - 4.18.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{3905fig3.eps} \end{figure}$	Figure 3: Elemental abundances relative to the sun. Solar values according to Grevesse & Sauval (1998). Data points of elements with consecutive atomic numbers are connected with lines. Errors as in Table 3.
Open with DEXTER