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  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f2r.eps}\end{figure} Figure 2: Same as Fig. 1 for planet's eccentricity equal to 0.1


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f3r.eps}\end{figure} Figure 3: Same as Fig. 1 for the 5:7 resonance


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f4r.eps}\end{figure} Figure 4: Same as Fig. 1 for the 7:9 resonance and different planetary masses. Dashes stand for planet's mass equal to $\mu ={1\over 3150}$ and dots stand for planet's mass equal to $\mu ={1\over 4500}$


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f6r.eps}\end{figure} Figure 6: Same as Fig. 1, with continuous line standing for the generic method


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f7r.eps}\end{figure} Figure 7: Same as Fig. 6, for the 5:7 extended resonance


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f8r.eps}\end{figure} Figure 8: Corotation points for the 7:9 resonance, for the generic method, planet as in Fig. 1, except for planetary masses. Continuous line stands for planet's mass equal to $\mu ={1\over 400}$, dashes stand for planet's mass equal to $\mu ={1\over 3500}$ (extended corotation) and and dots stand for planet's mass equal to $\mu ={1\over 4500}$


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f9r.eps}\end{figure} Figure 9: Corotation points for the 4:7 resonance, for the generic method, planet as in Fig. 1, except for planetary masses. Dots stand for planet's mass equal to $\mu ={1\over 400}$ (extended corotation), continuous line stands for planet's mass equal to $\mu ={1\over 1047.355}$ and dashes stand for planet's mass equal to $\mu ={1\over 2000}$


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f10r.eps}\end{figure} Figure 10: Corotation points for the 3:2 resonance, for the generic method, planet as in Fig. 5. Continuous line and circles stand for points determined considering Stokes drag (generic and numerical methods) while dashes stand for v2 drag


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f11r.eps}\end{figure} Figure 11: Corotation points for the 2:1 resonance, planet as in Fig. 5 and symbols as in Fig. 10


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f12r.eps}\end{figure} Figure 12: Corotation points for the 5:2 resonance, planet as in Fig. 5 and symbols as in Fig. 10


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f13r.eps}\end{figure} Figure 13: Corotation points for the 5:3 resonance, planet as in Fig. 5 and symbols as in Fig. 10


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f14r.eps}\end{figure} Figure 14: Variation of corotation points for the case of Stokes drag, with planet's mass for the 3:2 resonance, generic method with planet, except for masses, as in Fig. 5


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f15r.eps}\end{figure} Figure 15: Variation of corotation points for the case of Stokes drag, with planet's eccentricity, for the 3:2 resonance, generic method with planet, except for eccentricities, as in Fig. 5


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f16r.eps}\end{figure} Figure 16: Corotation points for the 11:10 interior resonance, Stokes drag, generic method, with $\mu_{\rm p} = 1/1000~\mu_{\rm J}$, and planetary orbital elements as in Fig. 1. Continuous line stands for the generic method and points stand for numerical integrations


  \begin{figure}
\par\includegraphics[width=12cm,clip]{MS10194f17r.eps}\end{figure} Figure 17: Same as Fig. 16 for the 9:8 resonance, only generic method


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Up: Resonance trapping of planetesimals points

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