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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 .

Caption: Figure 3.

The snapshot of steady-state Mach number at midplane (z = 0) for 3D simulation with ﹩{ \mathcal M }=4﹩.