ª $\begin{figure} \par\includegraphics[width=15cm,clip]{fig3b_ms10543.ps} \end{figure}$

Figure 3: Chemical abundances of the program stars (filled rectangles). Abundances from Stürenburg (1993) (triangles) and Paunzen et~al. (1999b) (empty rectangles) are also plotted for comparison. Abundances for the class prototype ( $\lambda$ Boo) and a solar metallicity star (Procyon) are from Paunzen et~al. (1999b) and Steffen (1995), respectively.

$\begin{figure} \par\includegraphics[width=15cm,clip]{fig3b_ms10543.ps} \end{figure}$

Figure 3: (continued).

Up: Physical parameters of Bootis stars

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