Disruption of exo-asteroids around white dwarfs and the release of dust particles in debris rings in co-orbital motion

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Fig. 9

DS maps for ∆i = 30° guided by a stable periodic orbit of the F^I family (left) and an unstable periodic orbit of the F^II′ family (middle) and G^II′ family (right). The chosen initial conditions, which remained fixed while some varied for the computation of each grid, are reported above each column (see also Table 3). Presentation as in Fig. 8.

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