\begin{table}%t1
\caption{\label{tab:Parameter}Herbig Ae type disk model parameter.}
%\centerline
 {\small \begin{tabular}{lcc}\\ 
\hline\hline
 Quantity & Symbol & Value\\
\hline  
stellar mass                      & $M_\star$          & $2.2~M_\odot$\\
effective temperature             & $T_{\rm eff}$      & 8600~K\\
stellar luminosity                & $L_\star$          & $32~L_\odot$\\
\hline
disk mass                         & $M_{\rm disk}$     & $0.01~M_\odot$\\
inner disk radius                 & $\Rin$             & 0.5~AU$^{~(1)}$\\
outer disk radius                 & $\Rout$            & 150~AU\\
radial column density power index & $\epsilon$         & 1.0\\
\hline
dust-to-gas mass ratio            & $\rho_d/\rho$      & 0.01\\
minimum dust particle radius      & $\amin$            & $0.1~\mu$m\\
maximum dust particle radius      & $\amax$            & $200~\mu$m\\
dust size distribution power index& $\apow$            & 3.5\\
dust material mass density$^{~(2)}$& $\rho_{\rm gr}$  & 2.5~g~cm$^{-3}$\\
\hline  %&&\\[-2.2ex]
strength of incident ISM UV       & $\chi^{\rm ISM}$   & 1\\
abundance of PAHs relative to ISM & $f_{\rm PAH}$      & 0.1\\
\hline
\end{tabular}}
\medskip
$^{(1)}$ Soft inner edge applied, see Woitke \etal (2009); $^{(2)}$:~dust optical constants from \citet{Draine1984}.
\end{table}