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

Open Access

Fig. 4

Families I of QS orbits (panel a) and II of HS orbits (panel b) on the (a_d, e_d) plane for our model (µ = 2.1186 × 10⁻¹¹ presented in Fig. 3), together with a comparison with µ = 0.001 and families f and b to highlight the proximity of this model to the unperturbed case.

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