\begin{table}%t1
%\centering
\par
\caption{\label{tab:collision_table}Parameters and results of the first collision sequence studied in this paper. Time $t$ in Myr, masses are in solar units.
The final row gives the age at which our evolution calculations stopped and
the mass of the collision product at the end of the evolution (assumed
black hole mass).  }
\small
\begin{tabular}{rrrrrrr}
\hline\hline
$N$ & $t$ & $M_{1,N\mbox{-}{\rm body}}^{a}$ &
$M_{1,{\rm mix}}^{a}$ & $M_{1,{\rm MMS}}^{a}$ &
$M_2^{a}$ & {$M_{\rm merger}^{a}$} \\
\hline
  1 &  0.22577 &    92.4 &    90.9 &   90.9 &  79.4 &   154.3\\
  2 &  0.22782 &   171.8 &   154.3 &  152.8 &  85.3 &   217.1\\
  3 &  0.23702 &   257.1 &   216.7 &  213.6 &   7.7 &   223.3\\
  4 &  0.31217 &   264.8 &   219.8 &  215.3 &  77.8 &   274.4\\
  5 &  0.40122 &   342.6 &   268.2 &  261.6 &  13.8 &   279.7\\
  6 &  0.43480 &   356.4 &   277.2 &  268.0 &  71.9 &   327.1\\
  7 &  0.43480 &   428.3 &   327.1 &  315.1 &  79.4 &   382.2\\
  8 &  0.74123 &   507.7 &   348.2 &        &  30.1 &   371.8\\
  9 &  0.83549 &   537.7 &   360.2 &        &  66.7 &   406.7\\
 10 &  0.90575 &   604.5 &   397.3 &        &   1.2 &   398.5\\
 11 &  1.29919 &   605.7 &   353.5 &        &  98.2 &   415.2\\
 12 &  1.33450 &   703.9 &   411.0 &        &  24.2 &   430.8\\
 13 &  1.42468 &   728.0 &   417.6 &        &   8.9 &   425.7\\
 14 &  1.50261 &   736.9 &   409.0 &        &   2.2 &   411.2\\
 15 &  1.60190 &   739.1 &   216.7 &        &  60.2 &   256.5\\
 16 &  1.63186 &   799.4 &   221.0 &        &   9.2 &   228.9\\
 17 &  1.68112 &   808.5 &   186.0 &        &  81.1 &   237.1\\
 18 &  1.75684 &   889.6 &   177.3 &        &  40.9 &   205.5\\
 19 &  1.90688 &   930.5 &   193.6 &        &  31.6 &   216.3\\
 20 &  2.07245 &   961.9 &   129.9 &        &   2.6 &   132.2\\
 21 &  2.59778 &   963.1 &    47.6 &        &  55.2 &    88.6\\
 22 &  3.10786 &  1012.7 &    40.9 &        &  75.4$^{b}$ &   110.1\\
    &  3.72835 &  1118.9 &    13.9 \\
\hline
\end{tabular}
\begin{list}{}{}
\item[$^{a}$]
The primary mass according to the $N$-body code
$M_{1,N\mbox{-}{\rm body}}$ and according to our fully mixed models
$M_{1,{\rm mix}}$, the mass of the secondary $M_2$ and the mass of
the fully mixed remnant after the collision $M_{\rm merger}$.
The mass $M_{1,{\rm MMS}}$ according to the MMAMS models we were able to
calculate is given for comparison.
\item[$^{b}$] See text.
\end{list}
\end{table}