$\begin{figure} \par\includegraphics[width=8.8cm,clip]{alpha_profile3.eps} \end{figure}$ Figure 1: Profile of the $\alpha$ -viscosity implemented to represent a Dead Zone between 1 and 5 AU with $(\epsilon , \delta _{r}) = (10^{-5}, 50)$ .
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In the text

$\begin{figure} \par\mbox{\epsfig{file=density_1_5AU_accretion.eps,width=5cm}\epsfig{file=RWI_5AU.eps,width=5cm} } \end{figure}$ Figure 2: Left: plot of $\cal L$ a t=0 and once the vortices have formed. Right: plot of the density in the disk at t = 100 years, with the velocity field superimposed. The velocity field shows the vortex at 5 AU. There is also one at 1 AU, not visible here.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{out1_disk_several} \end{figure}$ Figure 3: Zoom of the first 2 inner AU of the simulation at t=0, 100, 200, 300 years, showing the density. One sees three vortices forming, later evolving to two vortices, near the outer edge of the Dead Zone.
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In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{accretion_density_out5_2} \end{figure}$ Figure 4: This figure shows the density profile at t=100 (formation of the vortices) and 400 years: this shows that the spiral waves, seen in Fig. 2 to extend from the vortices, cause accretion across the Dead Zone.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{alpha_profile3.eps} \end{figure}$	Figure 1: Profile of the $\alpha$ -viscosity implemented to represent a Dead Zone between 1 and 5 AU with $(\epsilon , \delta _{r}) = (10^{-5}, 50)$ .
Open with DEXTER

$\begin{figure} \par\mbox{\epsfig{file=density_1_5AU_accretion.eps,width=5cm}\epsfig{file=RWI_5AU.eps,width=5cm} } \end{figure}$	Figure 2: Left: plot of $\cal L$ a t=0 and once the vortices have formed. Right: plot of the density in the disk at t = 100 years, with the velocity field superimposed. The velocity field shows the vortex at 5 AU. There is also one at 1 AU, not visible here.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{out1_disk_several} \end{figure}$	Figure 3: Zoom of the first 2 inner AU of the simulation at t=0, 100, 200, 300 years, showing the density. One sees three vortices forming, later evolving to two vortices, near the outer edge of the Dead Zone.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{accretion_density_out5_2} \end{figure}$	Figure 4: This figure shows the density profile at t=100 (formation of the vortices) and 400 years: this shows that the spiral waves, seen in Fig. 2 to extend from the vortices, cause accretion across the Dead Zone.
Open with DEXTER