\begin{table}%t3
%\centering
\small
\caption{\label{tab:cool}Origin of line emission and cooling rates of various species for the HH 46 central spaxel.}\vspace*{-2mm}
\begin{tabular}{l r l}
\hline \hline
Species & Cooling & Origin\\
 & 10$^{-3}$ $L_\odot$ \\ \hline
CO & \phantom{$>$}0.1 & Passively heated envelope \\
CO & \phantom{$>$}3.8 & UV-heated cavity walls \\
CO & \phantom{$>$}2.8 & $C$-type shocks \\
H$_2$O & \phantom{$>$}0.1 & Passively heated envelope \\
H$_2$O & \phantom{$>$}5.0 & UV or $C$-type shocks\\
%H$_2$O & 0.1 & $C$-type shocks \\
\ion{O}{i} & \phantom{$>$}9.5 & $J$-type shock \\
OH     & $>$2.4 & $J$-type shock \\
\ion{C}{ii} & \phantom{$>$}0.1 & Surrounding cloud \\ \hline
Total & $>$23.8 \\ \hline
\end{tabular}%\vspace*{-3mm}
\end{table}