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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 14.

Initial density profiles of the target (left column) and the impactor (right column) utilizing the DISPH. The layout and the EOS arrangements are identical to those in Figure 13.

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