\begin{table}%t5
\caption {\label{tab:Parameter}Parameter of the model depicted in Figs.~\ref{fig:Tgas} 
         to~\ref{fig:Tcum}.}
%\centerline
 {\begin{tabular}{lcc}
\hline\hline
 Quantity & Symbol & Value\\
\hline 
Stellar mass                      & $M_\star$          & $1~M_\odot$\\
Effective temperature             & $T_{\rm eff}$      & $5770~$K\\
Stellar luminosity                & $L_\star$          &$1~L_\odot$\\
Disk mass                         & $M_{\rm disk}$     & $0.01~M_\odot$\\
Inner disk radius                 & $\Rin$             & 0.5~AU$^{~(1)}$\\
Outer disk radius                 & $\Rout$            & 500~AU\\
Radial column density power index & $\epsilon$         & 1.5\\
Dust-to-gas mass ratio$^{~(2)}$  & $\rho_{\rm d}/\rho$      & 0.01\\
Minimum dust particle radius      & $\amin$            & $0.1~\mu$m\\
Maximum dust particle radius      & $\amax$            & $10~\mu$m\\
Dust size distribution power index& $\apow$            & 2.5\\
Dust material mass density        & $\rho_{\rm gr}$    & 2.5~g~cm$^{-3}$\\
&&\\[-2.2ex]
Strength of incident ISM UV       & $\chi^{\rm ISM}$   & 1\\
Cosmic ray ionisation rate of H$_2$  
                  & $\zeta_{\rm CR}$   
                  & $5\times 10^{-17}$~s$^{-1}$\\
Abundance of PAHs relative to ISM & $f_{\rm PAH}$      & 0.12\\
$\alpha$ viscosity parameter      & $\alpha$           & 0\\
\hline
\end{tabular}}
\par
\smallskip
 (1) Soft inner edge applied, see Sect.~\ref{sec:SoftEdge}.\\
 (2) Dust optical constants from \citet{Draine1984}.
\end{table}