SN 2023zaw: The Low-energy Explosion of an Ultrastripped Star
The Astrophysical Journal Letters American Astronomical Society 980:2 (2025) l44
Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A
Monthly Notices of the Royal Astronomical Society (2025) staf287
Identification of the Optical Counterpart of the Fast X-Ray Transient EP240414a
The Astrophysical Journal Letters American Astronomical Society 978:2 (2025) l21
Quasi-periodic X-ray eruptions years after a nearby tidal disruption event
Nature Nature Research 634:8035 (2024) 804-808
Abstract:
Quasi-periodic eruptions (QPEs) are luminous bursts of soft X-rays from the nuclei of galaxies, repeating on timescales of hours to weeks1–5. The mechanism behind these rare systems is uncertain, but most theories involve accretion disks around supermassive black holes (SMBHs) undergoing instabilities6–8 or interacting with a stellar object in a close orbit9–11. It has been suggested that this disk could be created when the SMBH disrupts a passing star8, 11, implying that many QPEs should be preceded by observable tidal disruption events (TDEs). Two known QPE sources show long-term decays in quiescent luminosity consistent with TDEs4, 12 and two observed TDEs have exhibited X-ray flares consistent with individual eruptions13, 14. TDEs and QPEs also occur preferentially in similar galaxies15. However, no confirmed repeating QPEs have been associated with a spectroscopically confirmed TDE or an optical TDE observed at peak brightness. Here we report the detection of nine X-ray QPEs with a mean recurrence time of approximately 48 h from AT2019qiz, a nearby and extensively studied optically selected TDE16. We detect and model the X-ray, ultraviolet (UV) and optical emission from the accretion disk and show that an orbiting body colliding with this disk provides a plausible explanation for the QPEs.Analysis of the JWST spectra of the kilonova AT 2023vfi accompanying GRB 230307A
(2024)