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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 10.

Snapshots of a collision with an Limp = 3 × 1036 kg m2 s−1 using SESAME and ANEOS EOS with SSPH. Particles with z  <  0 are shown. The snapshot times are given in hours from the beginning of the simulation.

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