\begin{table}%[t]%t1
%\centering
\par
\caption{Main parameters relevant for  the spin evolution of isolated  neutron stars with
hyperons.
The labels "infx'' mark  the configurations for which the curve
$\mb(R_{\rm eq})_{f}$ has a
point of inflexion. For
$f_{\rm 1,infx}<f<f_{\rm 2,infx}$ (corresponding
masses $M_{\rm B}^{\rm (1,infx)}$ and
$M_{\rm B}^{\rm (2,infx)}$) ${\rm BB_{st}}$ exists.
For $M_{\rm B}>M_{\rm B,max}^{\rm stat}$ we have  also ${\rm BB_{ut}}$,
which is the only BB phenomenon  for
$\mb > M_{\rm B}^{\rm (2,infx)}$. For $f>f_{\rm K,flat}$
and  $M_{\rm B}>M_{\rm B}^{\rm (K,flat)}$, a star which is initially in the mass-shedding
(Keplerian) state, spins-up   as it looses angular momentum. The characteristic
S-shape of $J(f)$ is then impossible.}\label{tab:bbhyp}
\begin{tabular}{ccccc}
\hline\hline
Parameter   & N1H1 & N2H1 & N1H2  &N2H2 \\
\hline
 $M_{\rm B,max}^{\rm stat}~[M_{\odot}]$& 1.83 & 2.05 & 1.73 & 1.95\\
\hline
 $f_{\rm 1,infx}$ [Hz]& 860 & 880 & 880 & 910\\
 $M_{\rm B}^{\rm (1,infx)}~[M_{\odot}]$& 1.808 & 1.91 & 1.73 & 1.81\\
\hline
 $f_{\rm K,flat}$ [Hz]     & 1030 & 970 & 1050 & 930\\
 $M_{\rm B}^{\rm (K,flat)}~ [M_{\odot}]$& 1.96 & 2.01 & 1.87  & 1.82\\
\hline
 $f_{\rm 2,infx}$ [Hz]& 1100 & 1320 & 1080 & 1380\\
 $M_{\rm B}^{\rm (2,infx)} ~[M_{\odot}]$& 1.9 & 2.17 & 1.79 & 2.06\\
\hline
\end{tabular}
\end{table}