TY - JOUR
T1 - Recurring tidal disruption events a decade apart in IRAS F01004-2237
AU - Sun, Luming
AU - Jiang, Ning
AU - Dou, Liming
AU - Shu, Xinwen
AU - Zhu, Jiazheng
AU - Dong, Subo
AU - Buckley, David
AU - Bradley Cenko, S.
AU - Fan, Xiaohui
AU - Gromadzki, Mariusz
AU - Liu, Zhu
AU - Wang, Jianguo
AU - Wang, Tinggui
AU - Wang, Yibo
AU - Wu, Tao
AU - Yang, Lei
AU - Zhang, Fabao
AU - Zhang, Wenjie
AU - Zhang, Xiaer
N1 - Publisher Copyright:
© 2024 EDP Sciences. All rights reserved.
PY - 2024/12/1
Y1 - 2024/12/1
N2 - 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.
AB - 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.
KW - Accretion
KW - Accretion disks
KW - Black hole physics
KW - Galaxies: nuclei
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U2 - 10.1051/0004-6361/202452380
DO - 10.1051/0004-6361/202452380
M3 - Article
AN - SCOPUS:85212978811
SN - 0004-6361
VL - 692
JO - Astronomy and astrophysics
JF - Astronomy and astrophysics
M1 - A262
ER -