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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 8.

Rock and ice components in the debris disk as a function of Limp for different EOSs in SSPH. The total mass of the rock component is normalized by the present satellite mass Msatellite.

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