\begin{table}%t6
\par
\caption{\label{tab:mflux}\mjet\ along the HH46-47 jet.}
%\centering
\par
  \begin{tabular}[h]{ccccc}
 \hline     \hline 
 \noalign{\smallskip}
Knot 
& d$v_t$(HVC)\tablefootmark{a}
& \mjet(HVC)\tablefootmark{b} 
& d$v_t$(LVC)\tablefootmark{a}
& \mjet(LVC)\tablefootmark{b}  \\  
  &  \small{\kms}  & \small{10$^{-7}$~\msyr} & \small{\kms} & \small{10$^{-8}$~\msyr} \\ 
\par
\hline 
S &  316 & 0.3--1.9 & 205 & 0.5--3.6 \\
Z2 & 213 & 0.4--0.9 & 136 & 0.2--0.4  \\
Z1 &  166 & 0.4--1.0 &     &  		\\
\hline
\end{tabular}
\tablefoot {\tablefoottext{a}{Tangential velocity derived from the observed radial velocities assuming an orientation angle of the jet with respect to the plane of the sky of 34\degr\ (\citealt{jochen94_hh46}).}
\tablefoottext{b}{\mjet\ measured from the luminosity of the \fe~~1.64~\um\ for the HVC and LVC. The lower value has been derived assuming an iron solar abundance, while the upper value has been inferred assuming the iron gas-phase abundance derived from the \fe/\pii\ ratio.}}
\end{table}