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

Keiya Murashima and Takanori Sasaki 2026 The Astrophysical Journal 1005 .

Caption: Figure 15.

Snapshots of the second collision with DISPH and L_imp = 7.0 × 10³⁶ kg m² s⁻¹ for SESAME/ANEOS (top), Tillotson EOS (middle), and HM80 EOS (bottom).