\begin{table}%T1
\par
\caption{Overview of our models (see text for details).}
    \label{tab:models}
%%\centerline
\par
{%\small
\begin{tabular}{l c c r l r r r r  r r r r}
\hline
\hline
Name
& \mach %\footnote{Mach number}
& $k$ %\footnote{driving wave number}
& \multicolumn{1}{c}{$n_{\rm p}$$^a$}
& $M_{\rm min}$$^b$
& $M_{\rm accr}$$^c$
& $n_*$$^d$
& $n_*$$^e$ & $\sigma_{\rm mean}$$^f$
& \multicolumn{4}{c}{$\dot{M}_{\rm mean}$ [$10^5 ~{M_{\sun} ~\rm yr^{-1}}$]}\\
& & & & \multicolumn{1}{c}{\scriptsize [$M_{\sun}$]} & \multicolumn{1}{c}{\scriptsize [\%]} &  & {\scriptsize fitted} & & {\scriptsize bin1} & {\scriptsize bin2} & {\scriptsize bin3} & {\scriptsize bin4}\\
\hline
G1    & --& --&  50~000 & 0.44  & 93.1 & 56 & 31 & 0.49 & 1.18 & 1.30 & 1.70 & 2.93 \\
G2    & --& --& 500~000 & 0.044 & 84.9 & 56 & 52 & 0.43 & 0.94 & 1.40 & 2.09 & 3.51\\
%\hline
M01k2 & 0.1 & 1..2 & 205~379 & 0.058 & 74.9 & 95 & 91 & 0.43 & 0.77 & 1.76 & 3.04 & --    \\ %Mc1I
M01k4 & 0.1 & 3..4 & 205~379 & 0.058 & 27.2 &  3 &  3 & 0.81 & 2.83 & --   & --   & 57.98 \\ %Mc2I
M01k8 & 0.1 & 7..8 & 205~379 & 0.058 & 85.9 &  3 &  3 & 0.47 & --   & 1.37 & 13.25& 59.16 \\ %Mc3I
M05k2 & 0.5 & 1..2 & 205~379 & 0.058 & 37.2 & 23 & 22 & 0.49 & 1.63 & 5.05 & 4.88 & 12.95 \\ %Mb1I
M05k4 & 0.5 & 3..4 & 205~379 & 0.058 & 77.9 & 48 & 48 & 0.39 & 1.31 & 2.49 & 2.56 & 6.30  \\ %Mb2I
M05k8 & 0.5 & 7..8 & 205~379 & 0.058 & 59.5 & 48 & 48 & 0.40 & 1.34 & 2.22 & 3.79 & 7.77  \\ %Mb3I
M2k2  &  2  & 1..2 & 205~379 & 0.058 & 75.1 & 68 & 62 & 0.41 & 0.86 & 1.38 & 2.54 & 4.32  \\ %Mz1I
M2k4  &  2  & 3..4 & 205~379 & 0.058 & 47.9 & 62 & 62 & 0.44 & 1.35 & 1.92 & 2.43 & 3.84  \\ %Mz2I
M2k8  &  2  & 7..8 & 205~379 & 0.058 & 66.2 & 42 & 40 & 0.42 & 0.87 & 1.29 & 1.72 & 3.38  \\ %Mz3I
M3k2  & 3.2 & 1..2 & 205~379 & 0.058 & 79.7 & 65 & 65 & 0.46 & 1.31 & 1.86 & 2.98 & 3.78  \\ %X01
M3k4  & 3.2 & 3..4 & 205~379 & 0.058 & 82.1 & 37 & 35 & 0.55 & 1.01 & 1.13 & 1.15 & 1.86  \\ %X02
M3k8  & 3.2 & 7..8 & 205~379 & 0.058 & 60.2 & 17 & 17 & 0.41 & 0.51 & 1.09 & 1.74 & 5.84  \\ %X03
M6k2a &  6  & 1..2 & 205~379 & 0.058 & 85.4 &100 & 97 & 0.49 & 0.79 & 1.69 & 1.96 & 3.39  \\ %M01I
M6k4a &  6  & 3..4 & 205~379 & 0.058 & 62.4 & 98 & 93 & 0.44 & 0.38 & 0.83 & 0.89 & 1.10  \\ %M02I
M6k2b &  6  & 1..2 & 195~112 & 0.062 & 34.5 & 50 & 50 & 0.42 & 1.02 & 1.81 & 2.50 & --    \\ %Z01
M6k4b &  6  & 3..4 &  50~653 & 0.24  & 29.7 & 50 & 47 & 0.43 & 0.72 & 1.66 & 1.87 & --    \\ %Z02
M6k8b &  6  & 7..8 &  50~653 & 0.24  & 35.7 & 25 & 25 & 0.44 & 0.35 & 0.61 & 1.38 & 2.47  \\ %Z03
M6k2c &  6  & 1..2 & 205~379 & 0.058 & 75.8 &110 & 97 & 0.43 & 0.83 & 1.32 & 1.50 & 1.23  \\ %Z01I
M6k4c &  6  & 3..4 & 205~379 & 0.058 & 61.9 & 53 & 46 & 0.54 & 1.31 & 1.46 & 2.05 & 1.97  \\ %Z02I
M6k8c &  6  & 7..8 & 205~379 & 0.058 &  6.4 & 12 & 10 & 0.43 & 0.50 & 0.62 & 0.58 & --    \\ %Z03I
M10k2 & 10  & 1..2 & 205~379 & 0.058 & 56.5 &150 &146 & 0.44 & 1.08 & 2.62 & 2.09 & --    \\ %My1I
M10k8 & 10  & 7..8 & 205~379 & 0.058 & 32.4 & 54 & 44 & 0.53 & 0.26 & 0.64 & --   & --    \\ \hline
\end{tabular}}
\par
\medskip
$^a$ Number of particles in the
simulation; \\
$^b$ SPH resolution limit; \\
$^c$ fraction of the total mass that has been accreted by the end of the simulation; \\
$^d$ total number of formed protostars; \\
$^e$ number of protostars that can be fitted by Eq.~(\ref{eq:fit}); \\
$^f$ mean deviation of the fits, calculated from Eq.~(\ref{eq:sigma}).
\end{table}