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Clustering Smoothed Particle Hydrodynamics Debris into N-body Fragments: A Collisional Code for Planet Formation

Authors: Samuele Crespi, Mohamad Ali-Dib, Ian Dobbs-Dixon

Samuele Crespi et al 2026 The Astronomical Journal 172 .

Provider: AAS Journals

Caption: Figure 5.

The cumulative mass removed from the simulation over time, separated by sink type. Mass loss as unresolved dust dominates initially, but later plateaus and is overtaken by mass ejected hyperbolically from the solar system.

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