Fig. 2
Example of mass distributions in the circumprimary ring as a function of the asteroids’ semi-major axis under the gravitational influence of a secondary M star at ab = 100 au and eb = 0.1 (■) and eb = 0.5 (•). The vertical line refers to the gas giant’s position. All particles are initially spaced by several Hill’s radii to prevent immediate dynamical instability.
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