\begin{table}
\caption{\label{result_tableCO}$^ {13}$CO Gaussian fits$^{a}$.  $T_{\rm b}$ uses a source size for the PDR (narrow component) of 120\arcsec~$\rightarrow \eta_{\rm bf}$~= 2, and  a source size for the broad outflow component of 85\arcsec~$\rightarrow \eta_{\rm bf}$~=~3.} 
\small%\centerline
 {
 {
\begin{tabular}{  l r r r r r r r}
\hline
\hline
Pos.  	&	$\upsilon_{{\rm LSR}}$& err  & $T^{~*}_{{\rm A}}$ & $T_{\rm b}$ & err&  	$\Delta \upsilon$ & err  \\
	 &	  [km~s$^{-1}$]&[km~s$^{-1}$] &[mK]&[mK]&[mK]&[km~s$^{-1}$]	&[km~s$^{-1}$] \\
\hline
1&--7.7&0.04&2665&5920	&68&2.8&0.08\\ 
2&--7.3&0.02&5877&	13~060	&	56&3.3&0.04\\
3&--7.3&0.01&6610&	14~690	&199&3.2&0.07\\
3&--6.8&0.33&612&  2040		&207&8.2&1.54\\
4&--7.3&0.03&3620&		8040	&66&3.5&0.07\\
5&--8.2&0.25&1124&		2500	&282&2.1&0.62\\
\hline
\end{tabular}}}
\medskip
$^{a}$ Gaussian fits (including errors) to the spectra in 5~positions. For most positions two Gaussians are needed to fit the spectra. Parameters: $\upsilon_{\rm LSR}$~= the LSR~velocity at the peak temperature, $T^{~*}_{{\rm A}}$~= the amplitude of the Gaussian fit, $\Delta \upsilon$~= FWHM line width.
\end{table}