$\begin{figure} \par\includegraphics[width=7.8cm,clip]{6718fig1.eps}\end{figure}$ Figure 1: Modulus of the acceleration in a monodimensional bar potential with the parameters of Sect. 2.1.4. Logarithmic scale. Range of x and y between -20 kpc and 20 kpc.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6718fig4.eps} \end{figure}$ Figure 4: Energy gain/loss in the simulation of particles as a function of its Jacobi integral. For comparison, the Jacobi integrals for the Lagrangian points are $H=-1.41\times 10^{11}$ J and $-1.29\times 10^{10}$ J.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{6718fig9.eps}\end{figure}$ Figure 9: Graphical representation of the hyperbolic trajectory of a particles which a approach a star (at the centre O).
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In the text

$\begin{figure} \par\includegraphics[width=7.8cm,clip]{6718fig1.eps}\end{figure}$	Figure 1: Modulus of the acceleration in a monodimensional bar potential with the parameters of Sect. 2.1.4. Logarithmic scale. Range of x and y between -20 kpc and 20 kpc.
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$\begin{figure} \par\includegraphics[width=7.7cm,clip]{6718fig2.eps}\end{figure}$	Figure 2: Histogram of distribution of energy gain/loss per unit mass (kg).
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$\begin{figure} \par\includegraphics[width=8cm,clip]{6718fig3.eps} \end{figure}$	Figure 3: Energy gain/loss in the simulation of particles with different impact parameter (b).
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$\begin{figure} \par\includegraphics[width=8cm,clip]{6718fig4.eps} \end{figure}$	Figure 4: Energy gain/loss in the simulation of particles as a function of its Jacobi integral. For comparison, the Jacobi integrals for the Lagrangian points are $H=-1.41\times 10^{11}$ J and $-1.29\times 10^{10}$ J.
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$\begin{figure} \par\includegraphics[width=7.4cm,clip]{6718fig5.eps}\end{figure}$	Figure 5: Histogram of distribution of energy loss as a function of the initial infall angle.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{6718fig6.eps} \end{figure}$	Figure 6: Histogram of distribution of energy loss as a function of the initial velocity.
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$\begin{figure} \par\includegraphics[width=7.5cm,clip]{6718fig7.eps} \end{figure}$	Figure 7: Histogram of distribution of energy loss as a function of halo mass.
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$\begin{figure} \par\includegraphics[width=7.8cm,clip]{6718fig8.eps}\end{figure}$	Figure 8: Fraction of halo mass accreted by means of the mechanism proposed in this paper.
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$\begin{figure} \par\includegraphics[width=8cm,clip]{6718fig9.eps}\end{figure}$	Figure 9: Graphical representation of the hyperbolic trajectory of a particles which a approach a star (at the centre O).
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