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Quasi-periodic eruptions (QPEs) are X-ray transients characterized by nearly regular recurring flares from galactic nuclei. Recent observations have confirmed that some QPEs occur in galactic centers that experienced a tidal disruption…

High Energy Astrophysical Phenomena · Physics 2025-12-09 Tomoya Suzuguchi , Tatsuya Matsumoto

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 Erupters (QPEs) are a remarkable class of objects exhibiting very large amplitude quasi-periodic X-ray flares. Although numerous dynamical models have been proposed to explain them, relatively little attention has been given…

High Energy Astrophysical Phenomena · Physics 2022-12-21 Julian H. Krolik , Itai Linial

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

Quasi-periodic eruptions (QPEs) are rapid, recurring X-ray bursts from supermassive black holes, believed to result from interactions between accretion disks and surrounding matter. The galaxy SDSS1335+0728, previously stable for two…

X-ray Quasi-Periodic Eruptions (QPEs) are a recently discovered phenomenon associated with supermassive black holes at the centers of galaxies. They are high amplitude soft X-ray flares that recur on timescales of hours, but what causes…

High Energy Astrophysical Phenomena · Physics 2021-11-17 Joheen Chakraborty , Erin Kara , Megan Masterson , Margherita Giustini , Giovanni Miniutti , Richard Saxton

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

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

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

Quasi-periodic eruptions (QPEs) are recurring soft X-ray transients emerging from the vicinity of supermassive black holes (SMBHs) in nearby, low-mass galaxy nuclei; about ten QPE hosts have been identified thus far. Here we report the…

I consider the current sample of galaxy nuclei producing quasiperiodic eruptions (QPEs). If the quasiperiod results from the orbital motion of a star around the central black hole, the dearth of associated black hole masses $\gtrsim…

High Energy Astrophysical Phenomena · Physics 2023-08-16 Andrew King

Quasi-Periodic Eruptions (QPEs) are recurrent X-ray eruptions discovered so far in the nuclei of low-mass galaxies. However, despite considerable observational progress, the origin of QPEs remains unclear. A variety of models have been…

High Energy Astrophysical Phenomena · Physics 2026-02-25 Wen-Long Xu , Hui-Hui Wang , Yi-Gu Chen , Yu-Zhe Li , Wei-Hua Lei

Recent observations of accreting black holes reveal the presence of quasi-periodic oscillations (QPO) in the optical power density spectra. The corresponding oscillation periods match those found in the X-rays, implying a common origin.…

High Energy Astrophysical Phenomena · Physics 2013-11-25 Alexandra Veledina , Juri Poutanen , Adam Ingram

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

Black hole and neutron star X-ray binary systems routinely show quasi-periodic oscillations (QPOs) in their X-ray flux. Despite being strong, easily measurable signals, their physical origin has long remained elusive. However, recent…

High Energy Astrophysical Phenomena · Physics 2021-06-30 Adam Ingram , Sara Motta

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

``Quasi-periodic eruptions'' (QPE) are recurrent nuclear transients with periods of several hours to almost a day, which thus far have been detected exclusively in the X-ray band. We have shown that many of the key properties of QPE flares…

High Energy Astrophysical Phenomena · Physics 2023-11-29 Itai Linial , Brian D. Metzger

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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