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X-ray quasi-periodic eruptions (QPEs) are discovered recently in active galaxies with unknown driven mechanism. Under the assumption that QPEs are caused by star-disc collisions, we adopt full relativistic method and show that both the…

High Energy Astrophysical Phenomena · Physics 2021-11-25 Jingtao Xian , Fupeng Zhang , Liming Dou , Jiasheng He , Xinwen Shu

We investigate the origins of quasi-periodic eruptions (QPEs) in galactic nuclei using global three-dimensional meshless finite-mass (MFM) simulations. By modeling stellar and black-hole impactors traversing accretion disks under various…

High Energy Astrophysical Phenomena · Physics 2026-03-03 Kun Liu , Shang-Fei Liu , Zhen Pan , Hongping Deng , Rongfeng Shen , Cong Yu

Quasi-periodic eruptions (QPEs), which are a new kind of X-ray bursts with a recurrence time of several hours, have been detected from supermassive black holes (SMBHs) in galactic nuclei. Recently, the two QPEs discovered by the…

High Energy Astrophysical Phenomena · Physics 2022-05-04 Z. Y. Zhao , Y. Y. Wang , Y. C. Zou , F. Y. Wang , Z. G. Dai

Quasiperiodic eruptions (QPEs) are a novel class of transients recently discovered in a few extragalactic nuclei. It has been suggested that a QPE can be produced by a main-sequence star undergoing repeated partial disruptions by the tidal…

High Energy Astrophysical Phenomena · Physics 2024-12-17 Chunyang Cao , F. K. Liu , Xian Chen , Shuo Li

Quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts with recurrence times about a few to ten hours from nearby galactic nuclei. The origin of QPEs is still unclear. In this work, we investigated the extreme mass ratio…

High Energy Astrophysical Phenomena · Physics 2024-05-24 Cong Zhou , Lei Huang , Kangrou Guo , Ya-Ping Li , Zhen Pan

Quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. Though the debates on the origin of QPEs have not completely settled down, more and more…

High Energy Astrophysical Phenomena · Physics 2024-11-28 Cong Zhou , Binyu Zhong , Yuhe Zeng , Lei Huang , Zhen Pan

Recent discoveries from time-domain surveys are defying our expectations for how matter accretes onto supermassive black holes (SMBHs). The increased rate of short-timescale, repetitive events around SMBHs, including the newly-discovered…

Quasi-periodic eruptions (QPEs) are intense repeating soft X-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. More and more analyses show that QPEs are the result of collisions between a stellar mass…

High Energy Astrophysical Phenomena · Physics 2025-04-22 Cong Zhou , Yuhe Zeng , Zhen Pan

Quasi-Periodic Eruptions (QPEs) are luminous, recurring X-ray outbursts from galactic nuclei, with timescales of hours to days. While their origin remains uncertain, leading models invoke accretion disk instabilities or the interaction of a…

Quasi-Periodic Eruptions (QPEs) display correlated long/short and strong/weak patterns that remain unexplained by existing flat-disk collision models. We propose that these features arise from an extreme-mass-ratio inspiral (EMRI) colliding…

High Energy Astrophysical Phenomena · Physics 2026-05-26 Bo-An Chen , Bei You , Giovanni Miniutti , Ning Jiang , Zhen Pan , Tao Yang , Xi-Long Fan , Kai Liao , Xu-Heng Ding , Zong-Hong Zhu , Shuai-Kang Yang , Sai-En Xu , Han He , Xiao Fan

X-ray quasi-periodic eruptions (QPEs) represent a recently discovered example of extreme X-ray variability associated with supermassive black holes. These are high-amplitude bursts recurring every few hours that are detected in the soft…

Quasi-Periodic Eruptions (QPEs) are extreme high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive black holes in galactic nuclei. It is currently unknown what triggers these events,…

Quasi Periodic Eruptions (QPEs) are luminous bursts of soft X-rays recently discovered in galactic nuclei. They repeat on timescales of hours to weeks, superimposed to an otherwise stable quiescent X-ray level, consistent with emission from…

High Energy Astrophysical Phenomena · Physics 2026-03-04 Chiara Maria Allievi , Luca Broggi , Alberto Sesana , Matteo Bonetti

Quasi-Periodic Eruptions (QPEs) are luminous X-ray outbursts recurring on hour timescales, observed from the nuclei of a growing handful of nearby low-mass galaxies. Their physical origin is still debated, and usually modeled as (a)…

Context: Some apparently quiescent supermassive black holes (BHs) at centers of galaxies show quasi-periodic eruptions (QPEs) in the X-ray band, the nature of which is still unknown. A possible origin for the eruptions is an accretion disk,…

High Energy Astrophysical Phenomena · Physics 2024-11-27 Anna Chashkina , Omer Bromberg , Amir Levinson , Ehud Nakar

Quasi-periodic eruptions (QPEs) are a recently discovered class of highly variable X-ray bursts originating in galactic nuclei. These high-amplitude bursts exhibit periodicity ranging from tens of minutes to several days. QPEs are also…

High Energy Astrophysical Phenomena · Physics 2026-05-22 Martin Mondek , Michal Zajaček , Henry Best , Taj Jankovič , Vladimír Karas , Petr Kurfürst

X-ray quasi-periodic eruptions (QPEs) are intense soft X-ray bursts from the nuclei of nearby low-mass galaxies typically lasting about one hour and repeating every few. Their physical origin remains debated, although so-called impacts…

Quasi-periodic eruptions (QPEs) are recurrent X-ray bursts found so far in the nuclei of low-mass galaxies. Their trigger mechanism is still unknown, but recent models involving one or two stellar-mass companions around the central massive…

High Energy Astrophysical Phenomena · Physics 2022-06-15 R. Arcodia , G. Miniutti , G. Ponti , J. Buchner , M. Giustini , A. Merloni , K. Nandra , F. Vincentelli , E. Kara , M. Salvato , D. Pasham

We propose that the recently observed quasi-periodic eruptions (QPEs) in galactic nuclei are produced by unstable mass transfer due to Roche lobe overflow of a low-mass main-sequence star in a mildly eccentric (e ~ 0.5) orbit. We argue that…

High Energy Astrophysical Phenomena · Physics 2023-10-12 Wenbin Lu , Eliot Quataert
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