\begin{table}%t3
%\centering

\renewcommand{\footnoterule}{}
\caption {Stellar properties and fit parameters. The stellar parameters
  of CQ~Tau are taken in \citet{CHIANG01}. For HD~135344 and HD~163296,
  the parameters are taken from \citet{MEEUS01} and \citet{VB05}. $H_{p}^{\rm in}/R_{\rm in}$ characterizes the puffed inner
  rim. $q$ is the power-law index of the scale height and~$p$ that of the
  surface density. $H_{\rm p}^{\rm out}/R_{\rm out}$ characterizes the flaring angle of the disk. The last column is the flux at 20.5~$\mu$m
  calculated from the modeled image.\label{resultat_model}}
\small 
{\begin{tabular}{lcccccccccccc}
 \hline\hline
 Object   & Distance & $M_{\star}$ & $T_{\rm eff}$ & $R_{\star}$&   $R_{\rm in}$ & $H_{p}^{\rm in}/R_{\rm in}$     & $R_{\rm out}$ & $H_{p}^{\rm out}/R_{\rm out}$&  $p$  &  $q$ &$i $& $F$ (20.5 $\mu$m)\\
          & (pc) & ($M_{\odot}$)&  (K)        &  ($R_{\odot}$)&   (AU) &    &(AU) &   & &  &(degrees)& (Jy)  \\
 \hline
HD~135344 &  84 &     1.3         & 6750            & 2.1  & 0.24 & 0.065  & 800  &0.21   &    0.8 & 9/7 & 60 & -- \\
(DDN03) &      &  &                &       &      &        &       &       &        &        &   &\\
HD 135344 & 140 &1.3         & 6750            & 2.1  & 0.24 & 0.065  & 200  & 0.12    &  0.8 & 9/7 & 45 &5.7 \\
(in this study)&        &                &       &      &        &       &       &        &       &  & \\
\hline
HD 163296 & 122 &2.5          & 10500         & 1.7  & 0.45  & 0.033  &50   &  0.07   & 0.2 & 9/7    & 65 & --\\
(DDN03) &     &   &                &       &      &        &       &       &              &  & \\
HD 163296 & 100 &2.5          & 10500         & 1.7  & 0.45  & 0.033  &200   &  0.05     & 1. & 1.07    & 60 & 16.6\\
(in this study)&        &                &       &      &        &       &       &   &      &       &   &\\
\hline
CQ~Tau    & 100 & 1.7         & 7130          &  1.3 &  0.23 &  0.0002 &180 &  0.13   & 1.5   &  9/7  & -- & --\\
(Chiang2001) &  &      &                &       &      &        &       &       &    &          &  & \\
CQ~Tau    &  100 &1.7         & 7130          &  1.9 &  0.23 &  0.018  &450 &  0.13       & 0.3   &  9/7  & 33 & 20\\
(in this study)&  &      &                &       &      &        &       &       &    &          & &  \\
\hline
\end{tabular}}
\par
%\smallskip
%$^a$ Disk size compatible with new measurement due to the re-evaluation of the distance.
\end{table}