\begin{table}%t8
\caption{\label{4:tab:outflow1}Outflow parameters from the CO 3--2 mapping.}
%\centerline
 {\small \begin{tabular}{l l l l l l l l l l}
\hline \hline\noalign{\smallskip}
Source &  $i$ &  Mass$^a$ & $\Delta V_{\rm max}$$^b$ & $R_{\rm out}$$^b$ & $t_{\rm d}$$^{b,c}$ & $\dot{M}$$^{a,d}$ & $F_{\rm CO}^a$$^{,e}$ & $L_{\rm kin}$$^{a,f}$  \\
& &($M_\odot$) & (km~s$^{-1}$) & (AU) & (yr)&  ($M_\odot$ &($M_\odot$~yr$^{-1}$ & ($L_\odot$)  \\  
& & & & &      &  yr$^{-1}$)&~km~s$^{-1}$) & \\
\hline  
\multicolumn{6}{c}{Red lobe} \\
%\hline
Ced 110 IRS 4 & 15  & 1.4e-2& 4.0  & 2.4e3 & 2.8e3 & 4.2e-6 & 4.6e-5 & 7e-5\\ 
CrA IRAS 32   & 45  & 6.6e-2& 6.3 & 9.3e3 & 7.1e3 & 9.3e-6 & 1.3e-4 & 5.5e-4\\
HH 100        & 60  & 3.6e-1& 14.7 & $>$ 6.1e3 & $>$2.0e3 & $<$1.5e-4& $<$4.9e-3 & $<$7.2e-2\\
RCrA IRS 7    & 45  & 1.1e0& 23.0 & $>$1e4& $>$2.1e3 & $<$4.3e-4 & $<$2.2e-2 & $<$5.0e-1 \\
HH46          & 35  & 4.3e-1& 9.5 & $>$2.5e4& $>$1.2e4& $<$3.2e-5 & $<$4.4e-4 & $<$3.1e-3\\  
IRAS 15398-3359& 75 &  2.9e-2& 8.2& 2.9e3 & 4.6e3 & 6.4e-7 & 6.4e-6 & 1.6e-5 \\
\hline
\multicolumn{6}{c}{Blue lobe} \\
%\hline
Ced 110 IRS 4 & 15 & 5.8e--3& --4.2  & -- & -- & -- & -- & -- \\ 
CrA IRAS 32   & 45 & 1.7e--2& --5.4  & 4.6e3 & 4.0e3& 4.3e--6 & 5e--5 & 1.8e--4\\
HH 100        & 60 & 4.7e--2& --9.7 & 4.6e3 & 2.2e3& 2.1e--5 & 4.4e--4 & 2.9e--4 \\
RCrA IRS 7    & 45 & 1.2e0 & --15.8& $>$5e3& $>$1.5e3& $<$7.9e--4 & $<$2.7e-2 & $<$2.9e--1\\
HH46          & 35 & 1.4e--1& --7.4 & 1.4e4 & 9.0e3& 1.5e--5 & 1.7e--4 & 9.3e--4\\  
IRAS 15398-3359& 75& 9.2e--2& 0.7 & 3.9e3 & 4.1e4& 2.2e--6 & 3.3e--5 & 1.2e--4\\
\hline
\end{tabular}}
\medskip
$^a$ Corrected for inclination using the average correction factors of \citet{Cabrit90}; $^b$~not corrected for inclination; $^c$~dynamical time scale: $t_{\rm{d}}=R/V_{\rm{max}}$; $^d$~mass outflow rate: $\dot{M}=M/t_{\rm{d}}$; $^e$~outflow force : $F_{\rm CO}=MV_{\rm{max}}^2/R$;
$^f$~kinetic luminosity : $L_{\rm kin}= 0.5~MV^3_{\max}/R$.
\end{table}