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Table 6:

$\dot{M}_{\rm jet}$ along the HH46-47 jet.
Knot dvt(HVC)a $\dot{M}_{\rm jet}$(HVC)b dvt(LVC)a $\dot{M}_{\rm jet}$(LVC)b
  km s-1 10-7 $M_{\odot}$ yr-1 km s-1 10-8 $M_{\odot}$ yr-1

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    

Notes. (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$^\circ$ (Eislöffel & Mundt 1994). (b)  $\dot{M}_{\rm jet}$ measured from the luminosity of the [Fe II]  1.64 $\mu $m 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 II]/[P II] ratio.


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