All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f1} \end{figure}$ Figure 1: The Mn distribution on the surface of $\epsilon$ UMa, obtained with INVERS11 from the Fe II and Mn II 4518 Å to 4522 Å blend.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f2} \end{figure}$ Figure 2: Ti distribution on the surface of $\epsilon$ UMa produced with INVERS11, obtained with the blend of Ti II and Cr II in the region from 4563 Å to 4565 Å.
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In the text

$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f3a}\includegraphics[width=4.35cm,clip]{1708.f3b} \end{figure}$ Figure 3: Mn II ( left, blended with Fe II between 4518 Å and 4522 Å) and Ti II ( right, blended with Cr II in the region from 4563 Å to 4565 Å) profiles.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f4} \end{figure}$ Figure 4: Sr surface distribution of $\epsilon$ UMa, obtained with the INVERS11 code from the blend of Sr II with Cr II at 4215 Å.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f5} \end{figure}$ Figure 5: Mg map, obtained with INVERS11 from the Mg I, 4167 Å line.
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In the text

$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f6a}\includegraphics[width=4.35cm,clip]{1708.f6b} \end{figure}$ Figure 6: Sr II ( left, blended with Cr II at 4215 Å) and Mg I, 4167 Å ( right) profiles.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f7} \end{figure}$ Figure 7: Cr map of $\epsilon$ UMa obtained from the Cr II 4558 Å line calculated with the INVERS11 code.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f8} \end{figure}$ Figure 8: The Fe map of $\epsilon$ UMa, obtained with INVERS11 from the three Fe I/ II lines at 4490 Å, 4520 Å and 4576 Å.
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In the text

$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f9a}\includegraphics[width=4.35cm,clip]{1708.f9b} \end{figure}$ Figure 9: The Cr II, 4558 Å ( left) and Fe I/ II, 4490 Å ( right) profiles of $\epsilon$ UMa. Crosses represent observed and solid lines the calculated profiles.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f10} \end{figure}$ Figure 10: Ca I distribution on the surface of $\epsilon$ UMa determined with INVERS11, obtained with the blend of Cr I and Fe I/ II in the region around 4526 Å.
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In the text

$\begin{figure} \par\includegraphics[width=5cm,clip]{1708.f11} \end{figure}$ Figure 11: Ca I profiles of $\epsilon$ UMa blended with Cr I and Fe I/ II in the region around 4526 Å.
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In the text

$\begin{figure} \par\includegraphics[width=7.2cm,clip]{1708.f12} \end{figure}$ Figure 12: Position of $\epsilon$ UMa, CU Vir, $\Phi$ Dra, ET And and $\theta$ Aur along the ZAMS (evolutionary tracks are based on A.A. Pamyatnykh 2000)
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f13} \end{figure}$ Figure A.1: Cr (top) and Fe (bottom) distribution obtained with the blend of Cr I, Fe I/ II, and Ca I in the region around 4526 Å. Results on the left side represent the Cr and Fe structure with Ca considered inhomogeneously distributed, on the right side a mean, constant, Ca abundance was used for mapping.

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f1} \end{figure}$	Figure 1: The Mn distribution on the surface of $\epsilon$ UMa, obtained with INVERS11 from the Fe II and Mn II 4518 Å to 4522 Å blend.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f2} \end{figure}$	Figure 2: Ti distribution on the surface of $\epsilon$ UMa produced with INVERS11, obtained with the blend of Ti II and Cr II in the region from 4563 Å to 4565 Å.
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$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f3a}\includegraphics[width=4.35cm,clip]{1708.f3b} \end{figure}$	Figure 3: Mn II ( left, blended with Fe II between 4518 Å and 4522 Å) and Ti II ( right, blended with Cr II in the region from 4563 Å to 4565 Å) profiles.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f4} \end{figure}$	Figure 4: Sr surface distribution of $\epsilon$ UMa, obtained with the INVERS11 code from the blend of Sr II with Cr II at 4215 Å.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f5} \end{figure}$	Figure 5: Mg map, obtained with INVERS11 from the Mg I, 4167 Å line.
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$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f6a}\includegraphics[width=4.35cm,clip]{1708.f6b} \end{figure}$	Figure 6: Sr II ( left, blended with Cr II at 4215 Å) and Mg I, 4167 Å ( right) profiles.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f7} \end{figure}$	Figure 7: Cr map of $\epsilon$ UMa obtained from the Cr II 4558 Å line calculated with the INVERS11 code.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f8} \end{figure}$	Figure 8: The Fe map of $\epsilon$ UMa, obtained with INVERS11 from the three Fe I/ II lines at 4490 Å, 4520 Å and 4576 Å.
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$\begin{figure} \par\includegraphics[width=4.35cm,clip]{1708.f9a}\includegraphics[width=4.35cm,clip]{1708.f9b} \end{figure}$	Figure 9: The Cr II, 4558 Å ( left) and Fe I/ II, 4490 Å ( right) profiles of $\epsilon$ UMa. Crosses represent observed and solid lines the calculated profiles.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{1708.f10} \end{figure}$	Figure 10: Ca I distribution on the surface of $\epsilon$ UMa determined with INVERS11, obtained with the blend of Cr I and Fe I/ II in the region around 4526 Å.
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$\begin{figure} \par\includegraphics[width=5cm,clip]{1708.f11} \end{figure}$	Figure 11: Ca I profiles of $\epsilon$ UMa blended with Cr I and Fe I/ II in the region around 4526 Å.
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$\begin{figure} \par\includegraphics[width=7.2cm,clip]{1708.f12} \end{figure}$	Figure 12: Position of $\epsilon$ UMa, CU Vir, $\Phi$ Dra, ET And and $\theta$ Aur along the ZAMS (evolutionary tracks are based on A.A. Pamyatnykh 2000)
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