\begin{table}%t3
\caption{
\label{table:properties-midisurveyII}Parameters of the models that simulate the measured SED
and MIR visibilities best.}
%\centerline
{\begin{tabular}{llrrrrrr}
\hline\hline\noalign{\smallskip}
Object (model-no.) & $M_{\rm disk}$ [$M_{\rm \odot}$] &
$R_{\rm out}$ [AU] & $R_{\rm in}$ [AU] & $\beta$ &
$h_{\rm 100}$ [AU] & $\vartheta$ [$^\circ$] & $\dot{M}$
[$M_{\rm \odot}$/a]\\
\hline  \noalign{\smallskip}
DR~Tau (I) & & & 0.10 & & & & $2.0 \times10^{-8}_{\rm (det.)}$\\ \noalign{\smallskip}
DR~Tau (II) & 0.1 & 90 & 0.10 & 0.75 & 15 & 20 & $8.0 \times 10^{-8}_{\rm (1)}$ \\\noalign{\smallskip}
DR~Tau (III) & & & 0.05 & & & & $8.0 \times 10^{-8}_{\rm (det.)}$\\\noalign{\smallskip}
GW~Ori (I,II) & 1.0 & 360 & 0.35 & 1.10 & 22 & 10 & $2.5 \times 10^{-7}_{\rm (2)}$\\ \noalign{\smallskip}
HD~72106~B & 0.005 & 40 & 0.50 & 1.30 & 8 & 60 & {No Accretion} \\ \noalign{\smallskip}
RU~Lup & 0.1 & 100 & 0.10 & 0.90 & 20 & 28 & $1.0 \times 10^{-8}_{\rm (3)}$ \\\noalign{\smallskip} 
HBC~639 & 0.1 & 120 & 0.10 & 1.00 & 10 & 65 & {No Accretion}  \\ \noalign{\smallskip} 
S~CrA~N (I) & \raisebox{-1.5ex}{0.03}&\raisebox{-1.5ex}{120} & \raisebox{-1.5ex}{0.05} & 1.10 & 9 & \raisebox{-1.5ex}{10}& \raisebox{-1.5ex}{$4.0 \times 10^{-8}_{\rm (det.)}$} \\\noalign{\smallskip}
S~CrA~N (II) & & & & 0.90 & 12 & 45 &  \\\noalign{\smallskip}
S~CrA~S & 0.03 & 100 & 0.10 & 1.05 & 8 & 30 & $4.0 \times 10^{-8}_{\rm (det.)}$  \\
\hline
\end{tabular}}
\medskip
References: $^{(1)}$:~Akeson et~al. (\cite{akeson}); $^{(2)}$:~Calvet et~al.~(\cite{calvetII}); $^{(3)}$:~Herczeg et~al. (\cite{herczeg}).
\end{table}