\begin{table}%t1
\caption{Line parameters for CO(1--0) and CO(2--1) at the peak and
integrated over the central 10--20$''$. }
\label{he1029-linepara}
%\centerline
{
\begin{tabular}{ccccccc}
\hline
\hline
\noalign{\smallskip}
Line &  Line & Line & Integrated &  Integrated intensity & $z$ & 
$M$(H$_2$+He)$^b$\\
& peak flux$^f$ & width &  peak intensity & in central $\sim$20$''$ 
&   & \\
 & [mJy/beam] & [\kms] & [Jy/beam~\kms] & [Jy\ \kms] &
& [10$^9$\msun]\\
\hline
\multicolumn{7}{c}{PdBI}\\
\hline
CO(1--0) & $65\pm7$ & $121\pm 3$ & $8.4\pm 0.2$ & $21\pm 1$  
& $0.0402\pm 0.0001$ & 1--8 \\
CO(2--1) & $90\pm 20$ & $131\pm 7$ & $12\pm 0.5$ & $25\pm 1$
& $0.0402\pm 0.0001$ & -- \\
\hline
\multicolumn{7}{c}{BIMA}\\
\hline
CO(1--0) & $190\pm 30$ & $150\pm 20$ & $28\pm 3$ & $30\pm 3$  
& $0.0402\pm 0.0002$ & 2--12 \\
\hline
%\hline
\noalign{\smallskip}
 & \multicolumn{2}{c}{Centre of CO emission} & 
\multicolumn{2}{c}{Dynamical Centre of CO emission} &  PA$^c$ & i$^d$  \\
& RA$^e$ & Dec$^e$ &  RA$^e$ & Dec$^e$ & [\degree] & [\degree] \\
\hline
\multicolumn{7}{c}{PdBI}\\
\hline
CO(1--0) & 10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.2$''$  &
10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.4$''$ & $\sim$20
& $\sim$10--30 \\
CO(2--1) & 10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.2$''$  &
 10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.4$''$ & $\sim$3
& -- \\
\hline
\multicolumn{7}{c}{BIMA}\\
\hline
CO(1--0) & 10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.8$''$  &
10$^{\rm h}$31$^{\rm m}$57.3$^{\rm s}$ & $-$18\degree46$'$33.8$''$ & $\sim$0 
& $\sim$10--30 \\
\hline
\end{tabular}}
\medskip
$^a$ Taking a luminosity
distance of 180~Mpc (based on the following cosmology: $H_0=70$~\kms,
$\Omega_m=0.3$ and $\Omega_\lambda=0.7$; 1$''$ corresponds then to
$\sim $0.8~kpc). $^b$ Assuming a $M$(H$_2$) to $L'_{\rm CO}$ conversion
factor of 0.8--4.8~\msun\ (K~\kms\ pc$^2$)$^{-1}$ (Solomon \& Barrett
\cite{solo91}; Downes \& Solomon \cite{down98}) and
$M$(H$_2$+He$)=1.36\times M$(H$_2$). $^c$~Estimated position angle of the
CO emission (from North to East). $^d$ Estimated inclination angle of
the CO disk. $^e$ The position uncertainties are of the order of
$\sim$0.2$''$ for the PdBI data and of $\sim$0.4$''$ for the BIMA
data. $^f$ Flux errors include $\sim$10\% ($\sim$20\%) uncertainties
from the flux calibration at 3~mm (1~mm).
\end{table}