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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 5.

Density snapshots for the star–disk collision with different resolutions and SMR levels. Each column represents a different configuration: the first four columns correspond to a resolution of 1024 × 1600 with SMR levels 0, 1, 2, and 3, respectively, while the fifth column shows results at a uniform resolution of 4096 × 6400. Note that the effective highest resolution of the third column (1024 × 1600 with SMR level 2) around the star is equivalent to the resolution of the fifth column. Rows represent the simulation time at frames −43.6 s, 43.6 s, 174.5 s, and 327.2 s, from top to bottom. The gray horizontal lines represent the disk’s midplane, and the green lines represent 4Hd from the midplane.

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