All Figures

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig1.eps} \end{figure}$ Figure 1: Plots of the mass-velocity relations for all swept-up material (top curve), and for molecular swept-up material only (short-dash) for our $\eta$ = 1 simulation at 1500 yr. Note the break in slope that appears when considering molecular material only (see Downes & Cabrit 2003). Also shown are the mass-velocity relations that would be inferred from the CO(2-1) intensity assuming T=10 K and T=100 K (lowest two curves; see Sect. 3.2). Velocity is projected along the jet z-axis.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig2.eps} \end{figure}$ Figure 2: Plots of the approaching and receding line-of-sight molecular momentum present in the blueshifted lobe of the $\eta =0.1$ simulation, the sum of these components ( $P_{\rm blue} + P_{\rm red}$ ), and the inclination corrected value $(P_{\rm blue} + P_{\rm red})/\sin \alpha$ . Each is normalised to the actual molecular z-momentum in the lobe.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig3.eps} \end{figure}$ Figure 3: As Fig. 2 but for the $\eta =1$ simulation.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig4.eps} \end{figure}$ Figure 4: Plots of the total line-of-sight energy for the $\eta =0.1$ simulation, both before and after correction for inclination by a mean factor of $1/\sin^2 \alpha$ . The energy is normalised by the total kinetic energy in molecular material.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig5.eps} \end{figure}$ Figure 5: As Fig. 4 but for the $\eta =1$ simulation.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig6.eps} \end{figure}$ Figure 6: Frequency distribution of the intensity-weighted local dynamical imescales for both the $\eta =0.1$ simulation (top panel) and the $\eta =1$ simulation (bottom panel). Each plot contains the distribution resulting for both $30^\circ$ and $60^\circ$ to the plane of the sky. The number of counts is the number of pixels with projected area on the sky of $1\times 10^{16}$ cm² ( $\approx$ 10^-5 pc²) and the bin-size is 1500 yr.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig2.eps} \end{figure}$	Figure 2: Plots of the approaching and receding line-of-sight molecular momentum present in the blueshifted lobe of the $\eta =0.1$ simulation, the sum of these components ( $P_{\rm blue} + P_{\rm red}$ ), and the inclination corrected value $(P_{\rm blue} + P_{\rm red})/\sin \alpha$ . Each is normalised to the actual molecular z-momentum in the lobe.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig3.eps} \end{figure}$	Figure 3: As Fig. 2 but for the $\eta =1$ simulation.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig4.eps} \end{figure}$	Figure 4: Plots of the total line-of-sight energy for the $\eta =0.1$ simulation, both before and after correction for inclination by a mean factor of $1/\sin^2 \alpha$ . The energy is normalised by the total kinetic energy in molecular material.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{figures/6921fig5.eps} \end{figure}$	Figure 5: As Fig. 4 but for the $\eta =1$ simulation.
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