Work

Relativistic Outflows Power a Quasi-periodic Eruption: Constraints on Energetics, Mass Loss, and Emission Mechanisms

Year: 2026
Type: article
Abstract: Quasi-periodic eruptions (QPEs) are recurring bursts of X-ray radiation originating from supermassive black holes (SMBHs). They are an unprecedented type of structured, high-amplitude SMBH variability, but the physical origins of their regularity, timescales, energetics, and emission are uncertain. We present new XMM-Newton observations of the QPEs in ZTF 19acnskyy/“Ansky,” constituting the deepest observations of individual bursts in any source thus far. The X-ray spectra reveal time-evolving P Cygni profiles comprising blueshifted absorption and redshifted emission from L-shell transitions of Fe xix – xxiv , with column densities N H ∼ 10 22−23 cm −2 and bulk velocities of ∣ v w / c ∣ ∼ 0.2, indicating relativistic mass ejections during each eruption. We construct a time-dependent analytical model of a wind turning on to self-consistently compute its evolving luminosity and ionization properties, and find that the light curve and spectral lines can be simultaneously produced by a wide-angle outflow with M ̇ ∼ 1 0 − 9 – 1 0 − 8 M ⊙ s − 1 kinetically powering the X-rays with an efficiency of L X / E ̇ K ∼ 0.1 . For a covering fraction f Ω ∼ 0.5, each eruption ejects ∼10 −3 M ⊙ and ≳10 49 erg of kinetic energy, setting an upper bound on the QPE lifetime of ≲1000 bursts if the underlying mass reservoir is ∼1 M ⊙ , and implying that the bursts may result in detectable multiwavelength signatures of reverberation and feedback. These measurements provide new quantitative constraints on QPE energetics, emission mechanisms, and the mass/energy they recycle into their circumnuclear environments, as well as an observational probe for direct comparison with physical models and hydrodynamical simulations of QPEs.
Language: English
Open Access status: gold
Estimated APC paid: $2,400
OpenAlex ID: W7204972605
FWCI: 0.821
Cites: 82
Cited by: 1
Related to: 10