\begin{table}%t1
%\centering
\par
\caption{The stellar yields (expressed in solar masses) as derived in this paper, namely those that produce the best 
agreement with observations. Yields for O are identical to metal dependent yields of WW95.\label{Table1}}
\begin{tabular}{cccccc}
\hline\hline
$m(M_{\odot}$)& Mg & Si & Ca& Fe &Zn \\
\hline
11.00 &  .6440E-01& .2170E-01& .1400E-02& .8000E-01& .3510E-04 \\
12.00 &  .5740E-01& .9090E-01& .1500E-01& .5500E-01& .3360E-04 \\
13.00 &  .1148E+00& .5850E-01& .3600E-02& .1460E+00& .4500E-04 \\
15.00 &  .1869E+00& .1100E+00& .1110E-01& .1297E+00& .7280E-04\\
18.00 &  .3864E+00& .1370E+00& .6900E-02& .8300E-01& .1060E-03\\
19.00 &  .1757E+00& .2770E+00& .1380E-01& .1170E+00& .1560E-03\\
20.00 &  .2191E+00& .2880E+00& .1480E-01& .1060E+00& .3160E-03\\
22.00 &  .2912E+00& .3560E+00& .1770E-01& .2225E+00& .3240E-03\\
25.00 &  .7000E-01& .3150E+00& .1690E-01& .1500E+00& .4070E-03\\
30.00 &  .7000E-01& .3160E+00& .1340E-01& .2500E-01& .3818E-03\\
35.00 &  .7000E-01& .1120E+00& .1600E-02& .2770E-01& .4176E-03\\
40.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
50.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
60.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
70.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
80.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
90.00 &  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
100.00&  .7000E-01& .5460E-01& .1600E-02& .2830E-01& .3710E-03\\
\hline
\end{tabular}
\end{table}