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Unlocking the Quasiperiodic Eruption Mystery: Star–Disk Collisions in Realistic Active Galactic Nucleus Disks

  • Authors: Zhaohuan Zhu, 照寰 朱, Xiaoshan Huang, 小珊 黄, Yan-Fei Jiang, 燕飞 姜, Shunquan Huang, 顺权 黄

Zhaohuan Zhu et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 6.

Effect of the disk surface density on the flare, for the θ = 135∘ collision. (Left) Excess luminosity ΔL, measured at y/r = −1.2 below the midplane after subtracting the reference run without a star, for a disk with 100 ×  the fiducial surface density (100 Σ, blue solid) and for the standard disk with its ΔL multiplied by 100 (red dashed). The time axis begins at t = 0.15 T0 to exclude the initial relaxation transient. Filled circles mark the light-curve peaks. (Right) Excess spectra Δ(νLν) at those two peaks, with best-fitting single-temperature blackbodies (dotted) at Tbb = 1.3 × 106 K (109 eV) and Tbb = 4.0 × 105 K (34 eV), respectively.

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