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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 2.

Semimajor axis–eccentricity distributions of the bodies at the end of the simulations. Point sizes are scaled by object mass. In both cases, the distributions become dynamically hotter at larger semimajor axes. Our simulation also exhibits a more top-heavy mass distribution than the SyMBA simulation.

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