\begin{table}%t1
\caption{Properties of isolated static neutron stars of gravitational mass $M=1.35~M_\odot$ for the three EOSs used in our computations. $M/R\equiv GM/Rc^2$ is the compaction parameter,
$R$ is the areal radius, $M_{\rm B}$ is the baryon mass  and~$\rho_{\rm c}$ is the central energy density, \mbox{respectively}.}
\label{EOStable}
%\centering
\par
\begin{tabular}{ccccc}
\hline  \hline
\multicolumn{1}{c}{EOS} & \multicolumn{1}{c}{$M/R$} &
\multicolumn{1}{c}{$R~[{\rm km}]$}&
\multicolumn{1}{c}{$M_{\rm B} [M_{\odot}]$}&
\multicolumn{1}{c}{$\rho_{\rm c}~[10^{14}{\rm g/cm^3}]$} \\
\hline
GNH3 & 0.140 & 14.262 & 1.45351 & 6.26 \\
APR & 0.176 & 11.350 & 1.49110 & 9.80 \\
BPAL12 & 0.191 & 10.447 & 1.48472 & 20.22 \\
\hline
\end{tabular}
\end{table}