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Quasiperiodic Eruptions from Stellar-mass Black Holes Impacting Accretion Disks in Galactic Nuclei

  • Authors: Kun Liu, 坤 刘, Shang-Fei Liu, 尚飞 刘, Zhen Pan, 震 潘, Hongping Deng, 洪平 邓, Rongfeng Shen, 荣锋 申, Cong Yu, 聪 余

Kun Liu et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 2.

Upper panel: energy budget estimated with Linial’s model for a surface density of 106 g cm−2. The blue solid and red dashed curves correspond to shocked regions of radius RB and 2RB. The gray dotted line indicates the minimum energy budget observed for GSN 069, ≃7 × 1045 erg (G. Miniutti et al. 2023; W. Guo & R.-F. Shen 2026). Lower panel: duration time as a function of inclination. The blue curve shows the prediction of the sBH-disk model, while the red dashed curve corresponds to the star-disk model.

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