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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 7.

Density and temperature snapshots for a star impact on the disk with different velocities from run03, 06, and 07. The top and bottom panels show the density and temperature, respectively. The left, middle, and right panels represent velocities of vs = 0.067c, 0.10c, and 0.15c, respectively. Each snapshot shows the moment when the star is at 9.6Rs from the disk’s midplane. The gray horizontal lines represent the disk’s midplane, and the green lines represent 4Hd from the midplane.

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