\begin{table}%t3 \caption{Simulations: final results.\label{cosmsimtable_fin}} %\centerline {\begin{tabular}{c c c c c c c c } %\tableline\tableline %\noalign{\smallskip} \hline\hline $N$ & $M_{\rm DM}$ & $R_{\rm DM}$ & $S_{\rm m}$ & $Q_{\rm t}$ & $a_{\rm max}$ & bulge & bars in bars\\ %\noalign{\smallskip} %\tableline %\noalign{\smallskip} %\tableline \hline c1 & 0.79 & 0.8 & 0.42 & 0.38 & 7 & y & n\\ c2 & 0.77 & 2.39 & 0.33 & 0.44 & 8 & y & n\\ c3 & 0.73 & 7.41 & 0.8 & 0.07 & 3.8 & n & y\\ c4 & 0.78 & 2.40 & 0.48 & 0.37 & 5 & weak & n\\ c5 & 0.73 & 7.41 & 0.70 & 0.08 & 6.5 & n & y\\ c6 & 0.79 & 2.43 & 0.35 & 0.42 & 6.8 & weak & n\\ c7 & 0.77 & 7.73 & 0.58 & 0.16 & 5.0 & n & y\\ i1 & 0.73 & 2.21 & 0.25 & 0.4 & 9.5 & y & n \\ i2 & 0.51 & 5.1 & 0.68 & 0.1 & 8 & n & y \\ i3 & 0.7 & 2.12 & 0.3 & 0.39 & 10 & y & n \\ i4 & 1. & 3.03 & 0.33 & 0.42 & 6 & y & n \\ 15 & 0.95 & 9.5 & 0 & 0 & 0 & n & no bar \\ %\noalign{\smallskip} \hline %\tableline \end{tabular}} \par \smallskip \par Column~1: simulation number and simulation type; Col.~2: DM mass inside the disk radius in $5.9\times 10^{10}~ M_{\odot}$; Col.~3: halo-to disk mass ratio inside the disk radius; Col.~4: maximum bar strength at $z=0$: strong bar \citet{Ma01} require $S_{\rm m}\le 0.6$; Col~5: bar strength evaluated according to \citet{Comb81}, stronger bar corresponds to higher values of $Q_{\rm t}$; Col.~6: major axis (physical kpc) corresponding to the maximum bar strength; Col.~7: morphology of the inner region of the disk; Col.~8: peculiar features inside the disk. \end{table}