\begin{table}%t2
  \caption{Model parameters for the test model shown in
  Fig.~\ref{fig:bc-compare}. The composition is given in fractions by mass.
  The photospheric velocity~$v_{\rm ph}$ denotes the velocity where
  $\tau_{\rm Rosseland}=2/3$. $v_{0}$~is the velocity of the actual innermost
  point of the model while~$v_{\rm ph}$ is an~output of the calculation.}\label{table:model}
  %\centering
\small
  \begin{tabular*}{5cm}{l@{\quad}r@{\extracolsep{\fill}}l@{\extracolsep{0pt}\quad}r}
  \hline
  \hline
  C  &  1.1\% &   Ti &  0.1\%\\
  O  & 11.4\% &   Cr &  0.1\%\\
  Mg & 10.2\% &   Fe &  3.1\%\\
  Si & 41.4\% &   Co & 11.4\%\\
  S  & 13.4\% &   Ni &  2.1\%\\
  Ca &  5.7\% &	 & \\ 
  \end{tabular*}
  \begin{tabular*}{5cm}{lr@{ }l}
  $L$          & $1\times10^{43}$   & \ergs \\
  Epoch        & $25~$             & d  \\
  $v_{0}$      & $4.48\times10^{3}$ & \kms \\
  $v_{\rm ph}$ & $6.65\times10^{3}$ & \kms \\
 & & \\[-8pt]
  \hline
  \end{tabular*}
\end{table}