Recurring, quasi-periodic bursts of high-energy radiation from the vicinity of a supermassive black hole.Quasi-periodic eruptions (QPEs) are recurring bursts of high-energy radiation, typically in X-rays, that originate from the immediate vicinity of a supermassive black hole at the center of a galaxy. These eruptions repeat on timescales of hours to days, with a quasi-periodic pattern—meaning the intervals are roughly regular but not perfectly so. They are thought to be caused by material, such as a star or a cloud of gas, that is being partially disrupted and accreted by the black hole, producing intense flashes of radiation each time the material interacts with the accretion disk or the black hole's corona.
QPEs were first discovered in 2019 using data from the XMM-Newton and Chandra X-ray observatories, with the first confirmed source identified in the galaxy GSN 069. The phenomenon was recognized as a distinct class of transient events in the early 2020s.
The leading explanation involves a star or a compact object on a highly elliptical orbit around the black hole. Each time it passes close to the black hole, it strips off some material, which spirals inward and emits a burst of X-rays. The quasi-periodicity arises because the orbital period is not perfectly stable due to gravitational interactions or changes in the accretion flow. Alternatively, the eruptions could be caused by instabilities in the accretion disk itself, where the disk periodically becomes hot and bright before cooling down.
They provide a natural laboratory for studying the extreme physics of black hole accretion and the dynamics of stars near supermassive black holes, helping to refine models of tidal disruption events and accretion disk behavior.
The first QPE source, GSN 069, exhibits eruptions every 9 hours, and the energy released in each burst is comparable to the total energy emitted by the Sun in a year.



















