\begin{table}%t2
\caption{\label{inipar}Initial dynamical and computational parameters for the three model galaxies.}
%\centering
\par
\begin{tabular}{l r c c c}
\hline \hline \noalign{\smallskip}
\multicolumn{2}{c}{\rule{0pt}{10pt} Model} &
\multicolumn{1}{c}{$\rm SCDM$} &
\multicolumn{1}{c}{$\Lambda \rm CDM$} &
\multicolumn{1}{c}{$\Lambda \rm CDM_{mp}$}\\ 
\hline  \noalign{\smallskip}
Initial Total Mass  [$M_{\odot}$]             & $M_{\rm tot}$        & $1.625 \times 10^{12}$ &  $8.830 \times 10^{11}$ & $2.449 \times 10^{11}$ \\
Initial Baryonic Mass Fraction                & $f_{\rm B}$            & $0.1$                  &  $0.176$                & $0.176$              \\
Initial Baryonic Mass [$M_{\odot}$]           & $M_{\rm B}$            & $1.624 \times 10^{11}$ & $1.413 \times 10^{11}$  & $4.164 \times 10^{10}$ \\
Initial Sphere Radius [kpc]                   & $R$              & $33.2$                 & $28$                    & $19$                 \\
Initial Number of Dark Matter Particles       &                  & $13685$                & $13~657$                 & $6966$               \\
Initial Number of Gas Particles               &                  & $13719$                & $13~707$                 & $6995$               \\
Dark Mass per particle [$M_{\odot}$]          & $M_{\rm DM,p}$       & $1.069 \times 10^8$    & $5.435 \times 10^7$     & $2.919 \times 10^7$      \\
Baryonic Mass per particle [$M_{\odot}$]      & $M_{\rm B,p}$        & $1.184 \times 10^7$    & $1.031 \times 10^7$     & $5.954 \times 10^6$      \\
Initial Redshift of the Proto-Halo            & $z_{\rm ini}$        & $50$                   & $60$                    & $58$                 \\
IMF                                           &                  & $\rm Kroupa$               & $\rm Kroupa$                & $\rm Salpeter$           \\
Softening length for Dark Matter [kpc]        & $\epsilon_{\rm DM}$  & $2$                    & $2$                     & $2$                  \\
Softening length for Baryonic Matter [kpc]    & $\epsilon_{\rm b}$   & $1$                    & $1$                     & $1$                  \\
\hline
\end{tabular}
\end{table}