\begin{table}%t1
   \caption{Fundamental parameters of FUor models: accretion rate, inner
      radius of the disc, flaring~$H/r$, type of dust opacity~$\kappa_\lambda$, and
      extinction~$A_{\rm V}$.}\label{tab:param-fit}
   %\centering
\par
   \begin{tabular}{lccccc}
      \hline\hline
                & $\Mstar\Mdot$   & $\Rmin$    & $H/r$        & $\kappa_\lambda$ & $A_{\rm V}$\\
                & ($\Msun^2/\yr$) & ($\Rsun$)  & (at 10~\AU) & (Ref.)           &      \\
      \hline
      FU~Ori    & $\sci{3.2}{-5}$   & 4        &  0.20        & i                & 1.3\\
      V1057~Cyg & $\sci{2.0}{-5}$   & 2        &  0.35        & i                & 4.5\\
      V1515~Cyg & $\sci{1.3}{-5}$   & 5        &  0.35        & h                & 2.8\\
      Z~CMa B   & $\sci{1.4}{-5}$   & 2        &  0.20\rlap{$^\star$}     & i                & 1.8\\
      \hline
      \multicolumn{6}{l}{i: Inhomogeneous aggregates \citep{Henning96}.}\\
      \multicolumn{6}{l}{h: Homogeneous aggregates \citep{Henning96}.}\\
      \multicolumn{6}{l}{$^\star$: Not constrained.}\\
   \end{tabular}
\end{table}