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Resolving Oblique Star–Disk Collisions in Quasiperiodic Eruptions: Numerical Requirements and the Importance of Geometry
Shunquan Huang et al 2026 The Astrophysical Journal 1005 .
Caption: Figure 10.
Similar to Figure 9 but as a function of t with an impact angle iv = 45° (run03 and 08).
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© 2026. The Author(s). Published by the American Astronomical Society.
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