\begin{table}%T3
\caption{Predicted X-ray properties of the model galaxies.}\label{t3}
%\centerline
{
\begin{tabular}{lllllll}
\hline
\hline
Model & $M_{\rm gas}/ M_{\rm lum}$      & [Fe/H] & [O/Fe]      &$L_{\rm X}$ &$kT_{\rm X}$\\
      &                         &        &            &($10^{41}~\rm erg~ s^{-1}$)&(keV) \\
\hline
L0    & $0.14\times10^{-3}$        &0.85    & --0.56      & $9.3\times10^{-3}$ &1.2 \\
La1   &0.014                    &0.85    & --0.68       & 2             &0.5\\
La10  &0.15                     &0.92    &--1.05       & --             &0.001\\
H0  &  $0.3\times10^{-2}$        &1.23   & --0.87     & 16.7 &1.7 \\
Ha1   &   0.05                   & 1.3&  --1.04&    183 &1\\
Ha10  &  0.17                   & 1.60&  --1.17&    -- &0.001\\
\hline
Ha1-0.3~$Z_{\odot}$   &   0.05                   & 1.4&  --1.02&    175 &0.98\\
Ha1-$Z_{\odot}$   &   0.05                   & 1.3&  --0.98&    254 &0.84\\
\hline
\end{tabular}}
\par
\medskip
Models Ha1-0.3~$Z_{\odot}$ and Ha1-$Z_{\odot}$ are similar to model Ha1, but
the second accretion episode has a metallicity of 0.3~$Z_{\odot}$ and $Z_{\odot}$,
respectively.
\end{table}