Image Details

Choose export citation format:

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 8.

Density and temperature snapshots from run08, where the star impacts the disk at an inclination angle of 45°. The top and bottom rows show density and temperature, respectively. From left to right, each column corresponds to t = 43.6 s, 87.3 s, 174.5 s, and 261.8 s. The gray horizontal lines represent the disk’s midplane, and the green lines represent 4Hd from the midplane.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse