\begin{table}%T7
%\centering
\par
\caption{Final abundance ratios [X/Fe] of the program stars,
compared to those of the
 metal-poor bulge clusters UKS 1 (Origlia et~al. \cite{Origlia05}) and
 Terzan 4 (Origlia et~al. \cite{Origlia04}). In the 2nd column the solar
abundances adopted are reported.
 No. corresponds to the number of lines used.}
\label{t7}
\begin{tabular}{lcrrrrrr}
\hline\hline
Species & $\epsilon$(X)$_{\odot}$ & No. &   HP1-2 &  HP1-3 &  Mean & UKS 1  & Terzan 4 \\
\hline
$\rm [Fe/H]$   & 7.50    & 50 & --1.00 & --0.97 & --0.99 & --0.78 &  --1.60  \\
$\rm [OI/Fe]$  & 8.77  & 1  &  +0.40 &  +0.40 &  +0.40 & +0.27 &  +0.55  \\
$\rm [NaI/Fe]$ & 6.33  & 2  &  +0.00 &  +0.00 &  +0.00 & -- & --   \\
$\rm [MgI/Fe]$ & 7.58  & 4  &  +0.00 &  +0.20 &  +0.10 & +0.32 &   +0.41   \\
$\rm [SiI/Fe]$ & 7.55  & 8  &  +0.30 &  +0.30 &  +0.30 & +0.28 &  +0.55  \\
$\rm [CaI/Fe]$ & 6.36  & 16  & --0.04 &  +0.10 & +0.03 & +0.38 &  +0.53  \\
$\rm [TiI/Fe]$ & 5.02  & 17  & +0.04 & +0.00 &  +0.02 &  +0.32 &  +0.43  \\
$\rm [TiII/Fe]$&  & 3  & +0.10 & +0.15 & +0.13 &   --  \\
$\rm [BaII/Fe]$& 2.13   & 2  & +0.10 & +0.20 &  +0.15 &   --  \\
$\rm [LaII/Fe]$&1.22  & 1  & 0.00 & 0.00   & +0.00 &    --  \\
$\rm [EuII/Fe]$&0.51  & 1  & +0.00 & +0.30 &  +0.15 &  --  \\
\hline 
\end{tabular}
\end{table}