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Resolving Oblique Star–Disk Collisions in Quasiperiodic Eruptions: Numerical Requirements and the Importance of Geometry

  • Authors: Shunquan Huang, 顺权 黄, Xiaoshan Huang, 小珊 黄, Zhaohuan Zhu, 照寰 朱, Rebecca G. Martin

Shunquan Huang et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

Shock stand-off distance Rsod as a function of the Mach number ﹩{ \mathcal M }﹩. The dots are measured from our simulation, while the solid lines are the best fit for the experimental results from F. S. Billig (1967). The blue and orange crosses represent results from 2D and 3D simulations, respectively. The blue and red lines are the best fit from the experiment for the cylinder wedge and spherical body (F. S. Billig 1967), respectively.

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