Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
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Resolving the inner few AU in protostellar disk simulations yields complete tidal disruption of migrating fragments and shorter, sharper accretion outbursts than coarser 30 AU models.
citing papers explorer
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Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
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From Fragments to Flares: Migration, Tidal Disruption, and Observable Bursts in Massive Protostellar Disks
Resolving the inner few AU in protostellar disk simulations yields complete tidal disruption of migrating fragments and shorter, sharper accretion outbursts than coarser 30 AU models.