\begin{table}%t4
\caption{Abundances for HD~139409, in the scale where $\log \epsilon$(H)~= 12, and 
normalized with respect to the solar abundances \citep{Grevesse-1998}. 
The standard deviations~$\sigma$ and the number~$N$ of lines used in the analysis are also given.}
\label{Tab:abundances139409}
%\centering
\par
\begin{tabular}{lrrrrr}
\hline\hline
  Element($X$) & $Z$ & $\log \epsilon$($X$) &  $\sigma$ &  $N$ & [$X$/Fe]  \\
\hline
C~{\sc i}   & 6 & 8.46   &  0.10     &  4 &  +0.36  \\
Na~{\sc i}  &  11 & 6.02   &  0.05     &  5 &  +0.11  \\
Mg~{\sc i}  &  12 & 7.31   &  0.12     &  6 &  +0.15  \\
Si~{\sc i}  &  14 & 7.33   &  0.06     & 20 &  +0.20  \\
Ca~{\sc i}  &  20 & 6.20   &  0.07     &  6 &  +0.26  \\
Sc~{\sc ii} &  21 & 2.79   &  0.06     & 10 &  +0.04  \\
Ti~{\sc i}  &  22 & 4.77   &  0.09     & 51 &  +0.17  \\
Ti~{\sc ii} &  22 & 4.72   &  0.11     &  4 &  +0.12  \\
V~{\sc i}   &  23 & 3.76   &  0.11     & 23 &  +0.18  \\
Cr~{\sc i}  &  24 & 5.21   &  0.11     & 11 & $-$0.04 \\
Cr~{\sc ii} &  24 & 5.36   &  0.09     &  3 &  +0.11  \\
Mn~{\sc i}  &  25 & 5.13   &  0.11     &  9 &  +0.16  \\
Fe~{\sc i}  &  26 & 7.08   &  0.08     &136 &   --  \\
Fe~{\sc ii} &  26 & 7.08   &  0.12     & 14 &   --  \\
Ni~{\sc i}  &  28 & 5.86   &  0.07     & 44 &  +0.03  \\
Y~{\sc i}   &  39 & 2.22   &  0.10     &  2 &  +0.40  \\
Y~{\sc ii}  &  39 & 2.41   &  0.07     &  6 &  +0.59  \\
Zr~{\sc i}  &  40 & 2.58   &  0.09     &  3 &  +0.40  \\
Zr~{\sc ii} &  40 & 2.78   &  0.12     &  3 &  +0.60  \\
Ba~{\sc ii} &  56 & 1.89   &  0.12     &  3 &  +0.18  \\
La~{\sc ii} &  57 & 1.05   &  0.12     &  3 &  +0.30  \\
Ce~{\sc ii} &  58 & 1.46   &  0.14     &  5 &  +0.30  \\
Nd~{\sc ii} &  60 & 1.38   &  0.09     &  6 &  +0.30  \\
\hline
\end{tabular}
\end{table}