The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) - IX. Gas-driven origin for the continuum arc in the debris disc of HD121617

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Fig. 13

Particle distributions for the M_gas=5 M_⊕ model after 150 orbits at r₀. Left: radial profiles (cf. Fig. 4); Right: azimuthal profiles (cf. Fig. 5). In both panels the black curve shows the gas surface density (right-hand axis).

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