Recurring tidal disruption events a decade apart in IRAS F01004-2237

Luming Sun, Ning Jiang, Liming Dou, Xinwen Shu, Jiazheng Zhu, Subo Dong, David Buckley, S. Bradley Cenko, Xiaohui Fan, Mariusz Gromadzki, Zhu Liu, Jianguo Wang, Tinggui Wang, Yibo Wang, Tao Wu, Lei Yang, Fabao Zhang, Wenjie Zhang, Xiaer Zhang

Research output: Contribution to journalArticlepeer-review

Abstract

Context. In theory, recurring tidal disruption events (TDEs) may occur when a close stellar binary encounters a supermassive black hole, if one star is captured and undergoes repeating partial TDEs, or if both stars are tidally disrupted (double TDEs). In addition, independent TDEs may be observed over decades in some special galaxies where the TDE rate is extremely high. Exploring the diversity of recurring TDEs and probing their natures with rich observational data helps us to understand these mechanisms. Aims. We report the discovery of a second optical flare that occurred in September 2021 in IRAS F01004-2237, where a first flare that occurred in 2010 had already been reported. We also present a detailed analysis of multi-band data. We aim to understand the nature of the flare and explore the possible causes of the recurring flares. Methods. We describe our analysis of the position of the flare, the multi-band light curves (LCs), the optical and ultraviolet (UV) spectra, and the X-ray LC and spectra. Results. The position of the flare coincides with the galaxy centre with a precision of 650 pc. The flare peaks in~50 days with an absolute magnitude of~ - 21 and fades in two years, roughly following L α t-5/3. It maintains a nearly constant blackbody temperature of~22 000 K in later stages. Its optical and UV spectra show hydrogen and helium broad emission lines with full width at half maxima of 7000-21 000 km s-1 and a He II/Hα ratio of 0.3-2.3. It shows weak X-ray emission relative to UV emission, with X-ray flares lasting for < 2 - 3 weeks, during which the spectrum is soft with a power-law index of F = 4.4-1.3+1.4. These characters are consistent with a TDE, ruling out the possibilities of a supernova or an active galactic nucleus flare. With a TDE model, we infer a peak UV luminosity of 3.3 ± 0.2 × 1044 erg s-1 and an energy budget of 4.5 ± 0.2 × 1051 erg. Conclusions. A TDE caused the flare that occurred in 2021. The two optical flares separated by 10.3 ± 0.3 years can be interpreted as repeating partial TDEs, double TDEs, or two independent TDEs. Although no definitive conclusion can be drawn, the partial TDEs interpretation predicts a third flare around 2033, and the independent TDEs interpretation predicts a high TDE rate of ≳10-2 yr-1 in F01004-2237, both of which can be tested by future observations.

Original languageEnglish (US)
Article numberA262
JournalAstronomy and astrophysics
Volume692
DOIs
StatePublished - Dec 1 2024

Keywords

  • Accretion
  • Accretion disks
  • Black hole physics
  • Galaxies: nuclei

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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