All Figures

$\begin{figure} \par {\includegraphics[width=9cm,clip]{8081fig1.eps} } \end{figure}$ Figure 1: Rotation curve data (full circles) of the 3 tidal dwarf galaxies (Bournaud et al. 2007). The lower (red) curves are the Newtonian contribution $V_{\rm bar}$ of the baryons (and its uncertainty, indicated as dotted lines). The upper (black) curves are the MOND prediction and its uncertainty (dotted lines). The top panels have as an implicit assumption (following Bournaud et al.) an inclination angle of 45 degrees. In the middle panels the inclination is a free parameter, and the bottom panels show the fits made with the first estimate for the external field effect (EFE) (Sect. 3).
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In the text

$\begin{figure} \par {\includegraphics[width=5.7cm,clip]{8081fig2.eps} } \end{figure}$ Figure 2: Baryonic Tully-Fisher relation (baryonic mass vs. circular velocity). The small full circles are the disk galaxy data from McGaugh (2005). The 3 TDGs studied here are shown as blue empty circles ( $i=45^{\circ }$ ) and red stars (i as a free parameter).
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In the text

$\begin{figure} \par {\includegraphics[width=6.6cm,clip]{8081fig3.eps} } \end{figure}$ Figure 3: Left: rotation curves with $i=90^{\circ }$ , with the baryonic distribution that best fits them in Newtonian dynamics. Symbols and curves are like in Fig. 1. Right: the corresponding surface density distribution (solid line) and integrated mass (dotted line).
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In the text

$\begin{figure} \par {\includegraphics[width=5.7cm,clip]{8081fig2.eps} } \end{figure}$	Figure 2: Baryonic Tully-Fisher relation (baryonic mass vs. circular velocity). The small full circles are the disk galaxy data from McGaugh (2005). The 3 TDGs studied here are shown as blue empty circles ( $i=45^{\circ }$ ) and red stars (i as a free parameter).
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$\begin{figure} \par {\includegraphics[width=6.6cm,clip]{8081fig3.eps} } \end{figure}$	Figure 3: Left: rotation curves with $i=90^{\circ }$ , with the baryonic distribution that best fits them in Newtonian dynamics. Symbols and curves are like in Fig. 1. Right: the corresponding surface density distribution (solid line) and integrated mass (dotted line).
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