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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 7.

Characteristic disk size 〈rd,imp〉 as a function of the initial angular momentum, for (a) SSPH and (b) DISPH. Sizes are normalized by Uranus’s radius.

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