\begin{table}%t1
\caption{\label{tab:Parameter}Parameters of the Herbig Ae model series.}
%\centering
 \small \begin{tabular}{ccc}
\hline\hline
 Quantity & Symbol & Value\\
\hline 
stellar mass                      & $M_\star$          & $2.2~M_\odot$\\
effective temperature             & $T_{\rm eff}$      & 8500~K\\
stellar luminosity                & $L_\star$          &$32~L_\odot$\\
%\hline
disk mass  & $M_{\rm disk}$     & $2.2\times 10^{-2}$, $10^{-2}, $ \\
 &                                 & $10^{-3}, 10^{-4}, 10^{-5},$\\
 &                               & $10^{-6}~M_\odot$\\
inner disk radius                 & $\Rin$             & 0.5~AU\tablefootmark{1}\\
outer disk radius                 & $\Rout$            & 700~AU\\
radial column density power index & $\epsilon$         & 1.0\\
%\hline
dust-to-gas mass ratio  & $\rho_d/\rho$      & 0.01\\
minimum dust particle radius      & $\amin$            & $0.05~\mu$m\\
maximum dust particle radius      & $\amax$            & $200~\mu$m\\
dust size distribution power index& $\apow$            & 3.5\\
dust material mass density        & $\rho_{\rm gr}$    & 2.5~g~cm$^{-3}$\\
%\hline 
&&\\[-2.2ex]
strength of incident ISM UV       & $\chi^{\rm ISM}$   & 1\\
cosmic ray ionization rate of H$_2$  
                  & $\zeta_{\rm CR}$   
                  & $5\times 10^{-17}$~s$^{-1}$\\
abundance of PAHs relative to ISM & $f_{\rm PAH}$      & 0.1\\
$\alpha$ viscosity parameter      & $\alpha$           & 0.0\\
\hline
\end{tabular}
 \tablefoot{\tablefoottext{1}{Soft inner edge applied, see Sect.~3.1 of \citet{Woitke2009a}}}.
\vspace*{1cm}
\end{table}