Open Access

Fig. 16

image

Same as Fig. 11 for a thin disc stellar particle evolution in the orbits integration (first row and thin lines of third row) and in the simulation (second row and thick lines of third row) in which the stellar particle is an extreme migrator. The black dash-dotted line shows the time evolution of the corotation radius (bottom left panel) and of Ωp (bottom right panel) in the simulations.

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