\begin{table}%t1
\caption{\label{Table01}Range of masses within which the simulations are run.}
%\centering
\par
\begin{tabular}{lccl}
\hline
\hline\noalign{\smallskip}
Total Mass $[M_{\odot}] $ & from       & to  & $\gamma$\\
\hline\noalign{\smallskip}
$M_{{\rm star}}$         & $5.1  \times 10^4 $ & $1.0  \times 10^8$ & $\gamma=1.5$ \\ 
$M_{{\rm dark}}$               & $7.1  \times 10^7$ & $1.9  \times 10^9$ & $\gamma \in [0.5,2]$ \\
$M_{{\rm gas}} $               & $5.5  \times 10^4$ & $6.9  \times 10^6$ & $\gamma=1.5$\\
\hline
\end{tabular}
\tablefoot {The scale lengths refer to $r_{90}$ as discussed in the text. The values listed here are our starting values at the initial time $T=T_0$.}
\end{table}