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Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact

  • Authors: Keiya Murashima, Takanori Sasaki

Keiya Murashima and Takanori Sasaki 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

Snapshots of a collision with Limp = 3 × 1036 kg m2 s−1 using the Tillotson EOS. Only particles with z  <  0 are shown. Snapshot times are measured in hours from the beginning of the simulation.

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