\begin{table}%t1
%\centering
\par
\caption {Main parameters of the EOSs with mixed-phase
segment. Below the mixed-phase transition point $n_1$  a
polytropic EOS with $\Gamma_{\rm A}$ is used. Mixed phase
extends within
 $n_1 < n_{\rm b} < n_2$, and is described by a
polytrope with adiabatic index $\Gamma_{\rm m}$.
Above the density $n_2$  we assume pure quark matter with  MIT bag model
EOS $p={1\over 3}(\rho-\rho_0)c^2$. In all
cases the dimensionless polytropic pressure coefficient $K$
was equal~0.025
 (see Appendix~A for details).
$M_{\rm b,max}^{\rm stat}$ and $M^{\rm stat}_{\rm max}$ denote
the maximum allowable baryon and gravitational mass of the
 non-rotating star. The EOSs are labeled as follows: MSt
 produces a stable back bending, MUn -- an  unstable one, and MM
 produces a  marginally stable case
 (for more details see the text).\label{tab:mixeos}}
\begin{tabular}{cccccc}
\hline\hline
EOS & $\Gamma_{\rm A}$ & $n_1$
& $\Gamma_{\rm m}$ & $n_2$
& $M_{\rm b,~max}^{\rm stat}~(M^{\rm stat}_{\rm max})$\\
%%%%%%%%%%%%%
 &    & $[{\rm fm^{-3}}]$
&   & $[{\rm fm^{-3}}]$
& $[M_\odot]$\\
\par
\hline
MSt & 2 & 0.35 & 1.5 & 0.8 & 1.508 (1.393) \\
MUn & 2.5 & 0.2 & 1.3 & 0.65 & 1.586 (1.453) \\
MM & 2.25 & 0.25 & 1.25 & 0.57 & 1.685 (1.534)\\
\hline
\end{tabular}
\end{table}