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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 5.

Median rotation periods of the post-impact planets as a function of the impact angular momentum Limp, for different EOSs and SPH schemes. Panels show (a) SSPH and (b) DISPH. The dashed line indicates the present rotation period of Uranus (17.24 hr; J. W. Warwick et al. 1986).

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