\begin{table}%t3
\caption {\label{tab3}Abundances $\log$(N(elem)/N$_{tot}$) for HR~6000 and 46~Aql 
from ATLAS12 models. }
%\centerline
 {\begin{tabular}{lccrccccccccccccccc}
\hline\hline\noalign{\smallskip}
\multicolumn{1}{c}{Elem}&
\multicolumn{1}{c}{HR~6000}&
\multicolumn{1}{c}{46~Aql}&
\multicolumn{1}{c}{Sun$^a$}
\\
& [13~450~K, 4.3]&[12~560~K, 3.8]&\\
\hline\noalign{\smallskip}
\ion{He}{i} & $-$2.10 & $-$2.00 & $-$1.05\\
\ion{Be}{ii} & $-$9.78 & $-$9.91 & $-$10.64\\
\ion{C}{ii}  & $-$5.50 & $-$4.75 & $-$3.52\\ 
\ion{N}{i}  & $\le$$-$5.82&$\le$$-$5.50 & $-$4.12\\
\ion{O}{i}  & $-$3.68~$\pm$~0.4 & $-$3.51~$\pm$~0.10 & $-$3.21 \\
\ion{Ne}{i}& $\le$$-$4.86 & $-$4.51 & $-$3.96\\
\ion{Na}{i} &$\le$$-$5.71 & $-$5.69 & $-$5.71\\
\ion{Mg}{ii} & $-$5.66 & $-$5.45 & $-$4.46\\
\ion{Al}{i} & $\le$$-$7.30 & $-$6.65 & $-$5.57\\
\ion{Al}{ii} & $\le$$-$7.30 &$\le$$-$7.40 & $-$5.57\\
\ion{Si}{ii} & $-$7.35 & $-$5.61~$\pm$~0.06 & $-$4.49\\
\ion{P}{ii} & $-$4.44~$\pm$~0.27 & $-$5.02~$\pm$~0.30 & $-$6.59\\
\ion{P}{iii}& $-$5.11~$\pm$~0.26 & $-$5.87          &$-$6.59\\
\ion{S}{ii} &$-$6.26  & $-$5.74 & $-$4.71\\
\ion{Cl}{i} &$\le$$-$7.74 & $\le$$-$7.04 & $-$6.54\\
\ion{Ca}{ii} & $-$5.68 & $-$5.98 & $-$5.68\\
\ion{Sc}{ii} &$\le$$-$9.50 & $\le$$-$9.50 & $-$8.87\\
\ion{Ti}{ii} & $-$6.47~$\pm$~0.13 &$-$6.46~$\pm$~0.06  & $-$7.02\\
\ion{V}{ii}  &$\le$$-$9.14 & $-$8.94 & $-$8.04\\
\ion{Cr}{ii} & $-$6.10~$\pm$~0.09 & $-$7.48 & $-$6.37\\
\ion{Mn}{ii} & $-$5.18~$\pm$~0.32 & $-$5.82~$\pm$~0.22 & $-$6.65\\
\ion{Fe}{i} & $-$3.65~$\pm$~0.07 & $-$3.91~$\pm$~0.06 & $-$4.54\\
\ion{Fe}{ii} & $-$3.65~$\pm$~0.09 & $-$3.91~$\pm$~0.08 & $-$4.54\\
\ion{Co}{ii} &$\le$$-$8.42 &$\le$$-$8.02 & $-$7.12\\
\ion{Ni}{ii} &$-$6.24 & $-$6.47 & $-$5.79\\
\ion{Cu}{ii} &$\le$$-$7.83 & $-$6.24~$\pm$~0.02 & $-$7.83\\
\ion{Zn}{i}  & $-$        &$-$5.85  & $-$7.44\\
\ion{Zn}{ii} & $-$        &$-$5.76  & $-$7.44\\
\ion{As}{ii} & $-$        & $>$$-$9.67 & $-$9.67\\
\ion{Sr}{ii} &$\le$$-$10.07     & $-$10.67 & $-$9.07\\
\ion{Y}{ii}  &$-$8.60      & $-$8.09~$\pm$~0.08  & $-$9.80\\
\ion{Xe}{ii} &$-$5.23      & $-$5.81  & $-$9.87\\
\ion{Hg}{ii} & $-$8.20       & $-$7.10  & $-$10.91\\
\hline
\end{tabular}}
\par
\smallskip
$^a$ Solar abundances are from Grevesse \& Sauval (\cite{Grevesse98}).
\end{table}