\begin{table}%t2
%\centering
\par
\caption{The stellar yields (expressed in solar masses) as derived in this paper, namely those that produce the best 
agreement with observations.\label{Table2}}
\begin{tabular}{cccccccc}
\hline\hline
$m(M_{\odot}$)& K& Sc & Ti & Cr &Mn& Co& Ni \\
\hline
11.00 & .4040E-04 & .2564E-05& .3300E-03& .2037E-02& .1290E-03& .1272E-03& .1670E-01\\
12.00 & .1712E-02 & .2714E-05& .3960E-03& .2091E-02& .1400E-03& .2010E-04& .7000E-02\\
13.00 & .6160E-04 & .2553E-05& .3990E-03& .1929E-02& .4490E-03& .2019E-04& .1120E-01\\
15.00 & .2544E-03 & .6751E-05& .7515E-03& .1371E-02& .4710E-03& .3030E-04& .6800E-02\\
18.00 & .1176E-03 & .2415E-05& .8400E-03& .8910E-03& .4040E-03& .4290E-04& .3760E-02\\
19.00 & .6952E-03 & .6038E-05& .8670E-03& .7980E-03& .2060E-03& .7710E-04& .4680E-02\\
20.00 & .7496E-03 & .1086E-04& .8700E-03& .5400E-03& .2130E-03& .8160E-04& .4440E-02\\
22.00 & .1200E-02 & .2530E-04& .8940E-04& .4050E-03& .2300E-03& .8820E-04& .1120E-01\\
25.00 & .4032E-03 & .2622E-05& .7500E-04& .3900E-03& .2580E-03& .7500E-03& .7590E-02\\
30.00 & .2648E-03 & .1610E-05& .1500E-03& .4500E-03& .1040E-03& .8070E-03& .3350E-01\\
35.00 & .1328E-03 & .1345E-05& .4500E-03& .4500E-03& .1330E-03& .7950E-03& .2040E-02\\
40.00 & .8960E-04 & .1621E-05& .4560E-03& .9120E-04& .1340E-03& .8250E-03& .2120E-02\\
50.00 & .8960E-04 & .1621E-05& .4560E-03& .6120E-04& .1340E-03& .8250E-03& .2120E-02\\
60.00 & .8960E-04 & .1621E-05& .4560E-03& .3120E-04& .1340E-03& .8250E-03& .2120E-02\\
70.00 & .8960E-04 & .1621E-05& .4560E-03& .3120E-04& .1340E-03& .8250E-03& .2120E-02\\
80.00 & .8960E-04 & .1621E-05& .4560E-03& .3120E-04& .1340E-03& .8250E-03& .2120E-02\\
90.00 & .8960E-04 & .1621E-05& .4560E-03& .3120E-04& .1340E-03& .8250E-03& .2120E-02\\
100.00& .8960E-04 & .1621E-05& .4560E-03& .3120E-04& .1340E-03& .8250E-03& .2120E-02\\
\hline
\end{tabular}
\end{table}