\begin{table}%t4
  \caption{Parameter set for the passive disk model, the active model
    (Sect.~\ref{section:  accretion}) and the active model with an envelope 
    (Sect.~\ref{section: dusty envelope}). Results correspond to Fig.~\ref{figure:ry}.}
  %\centering
\par
  \begin{tabular}{lrrr}\hline\hline
    Parameter & Passive disk & Active disk & Active disk ${\rm +}$ envelope \\ 
    & model & model & model \\ \hline
    Stellar mass $M_{\star}$ & $1.69\ M_{\odot}$ & $1.69\ M_{\odot}$ & $1.69\ M_{\odot}$ \\
    Stellar temperature $T_{\star}$ & $5560\ {\rm K}$ & $5560\ {\rm K}$ & $5560\ {\rm K}$ \\
    Stellar luminosity $L_{\star}$ & $10.0\ L_{\odot}$ & $10.0\ L_{\odot}$ & $10.0\ L_{\odot}$ \\
    Disk mass $M_{\rm disk}$ & $1 \times 10^{-2}\ M_{\odot}$ & 
    $4 \times 10^{-3}\ M_{\odot}$ & $4 \times 10^{-3}\ M_{\odot}$ \\
    Outer disk radius $R_{\rm out}$  & $270\ {\rm AU}$ & $270\ {\rm AU}$ & 
    $270\ {\rm AU}$ \\
    Inner disk radius $R_{\rm in}$ & $0.3\ {\rm AU}$ & $0.3\ {\rm AU}$ & $0.3\ {\rm AU}$  \\
    Exponent $p$ (see Eq.~(\ref{eq: sigma})) & $1.3$ & $1.3$ & $1.4$ \\
    Inclination $\vartheta$ & $\lse$$70^{\circ}$ & $\lse$$70^{\circ}$ & $\lse$$65^{\circ}$ \\
    $c_{\rm 1}$ (see Eq.~(\ref{eq: envelope})) & -- & -- & $5.0 \times 10^{-5}$ \\
    $c_{\rm 2}$ (see Eq.~(\ref{eq: envelope})) & -- & -- & $1.0$ \\
    Accretion rate $\dot{M}$ & -- & $9.1 \times 10^{-8}$ $M_{\odot}$ yr$^{-1}$ & $2.5 \times 10^{-8}$ $M_{\odot}$ yr$^{-1}$ \\
    Boundary temperature $T_{\rm bnd}$ & -- & $8000\ {\rm K}$ & $8000\ {\rm K}$ \\
    Truncation radius $R_{\rm bnd}$ & -- & $5\ R_{\star}$ & $5\ R_{\star}$ \\  
    \hline
  \end{tabular}
  \label{table:ry}
\end{table}