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A black hole (BH) can tear apart a star that ventures within its tidal radius, producing a luminous flare as the stellar debris falls back, known as a tidal disruption event (TDE). While TDEs in quiescent galaxies are relatively well…

We present X-ray, UV, optical, and radio observations of the nearby ($\approx78$ Mpc) tidal disruption event (TDE) AT2021ehb/ZTF21aanxhjv during its first 430 days of evolution. AT2021ehb occurs in the nucleus of a galaxy hosting a $\approx…

The tidal disruption event (TDE) AT2018fyk has unusual X-ray, UV, and optical light curves that decay over the first $\sim$600d, rebrighten, and decay again around 1200d. We explain this behavior as a one-off TDE associated with a massive…

High Energy Astrophysical Phenomena · Physics 2024-07-30 S. Wen , P. G. Jonker , A. J. Levan , D. Li , N. C. Stone , A. I. Zabludoff , Z. Cao , T. Wevers , D. R. Pasham , C. Lewin , E. Kara

Tidal disruption events (TDEs) can uncover the quiescent supermassive black holes (SMBHs) at the center of galaxies. After the disruption of a star by a SMBH, the highly elliptical orbit of the debris stream will be gradually circularized…

High Energy Astrophysical Phenomena · Physics 2023-09-08 Jin-Hong Chen , Li-Ming Dou , Rong-Feng Shen

The multiwavelength data of nuclear transient AT2018dyk, initially discovered as a changing-look low-ionization nuclear emission-line region (LINER) galaxy, has been revisited by us and found being in agreement with a tidal disruption event…

High Energy Astrophysical Phenomena · Physics 2023-09-04 Shifeng Huang , Ning Jiang , Zheyu Lin , Jiazheng Zhu , Tinggui Wang

AT 2018hyz (=ASASSN-18zj) is a tidal disruption event (TDE) located in the nucleus of a quiescent E+A galaxy at a redshift of $z = 0.04573$, first detected by the All-Sky Automated Survey for Supernovae (ASAS-SN). We present optical+UV…

Tidal Disruption Events (TDEs) have long been hypothesized as valuable indicators of black holes, offering insight into their demographics and behaviour out to high redshift. TDEs have also enabled the discovery of a few Massive Black Holes…

Tidal disruption events (TDEs) have traditionally been discovered in optical sky surveys through targeted searches of nuclear transients. However, it is expected that some TDEs will occur outside the galaxy nucleus, arising from wandering…

We argue that the `changing look' AGN recently reported by LaMassa et al. could be a luminous flare produced by the tidal disruption of a super-solar mass star passing just a few gravitational radii outside the event horizon of a $\sim 10^8…

High Energy Astrophysical Phenomena · Physics 2015-08-06 A. Merloni , T. Dwelly , M. Salvato , A. Georgakakis , J. Greiner , M. Krumpe , K. Nandra , G. Ponti , A. Rau

We present a search for luminous, long-duration ambiguous nuclear transients (ANTs) similar to the unprecedented discovery of the extreme, ambiguous event AT2021lwx with a $>150$\,d rise time and luminosity $10^{45.7}$\,erg\,s$^{-1}$. We…

Supermassive black hole binaries (SMBHs) are a fascinating byproduct of galaxy mergers in the hierarchical universe. In the last stage of their orbital evolution, gravitational wave radiation drives the binary inspiral and produces the…

High Energy Astrophysical Phenomena · Physics 2022-01-28 Ning Jiang , Huan Yang , Tinggui Wang , Jiazheng Zhu , Zhenwei Lyu , Liming Dou , Yibo Wang , Jianguo Wang , Zhen Pan , Hui Liu , Xinwen Shu , Zhenya Zheng

We report a candidate repeating tidal disruption event (TDE), AT2022sxl, found from large-field optical survey data. Two flares with a separation time of $\sim$7.2\,yr between the two optical peaks are observed. Related mid-infrared (MIR)…

High Energy Astrophysical Phenomena · Physics 2025-08-14 Shunhao Ji , Zhongxiang Wang , Litao Zhu , Stefan Geier , Alok C. Gupta

Massive black holes (BHs) at the centres of massive galaxies are ubiquitous. The population of BHs within dwarf galaxies, on the other hand, is evasive. Dwarf galaxies are thought to harbour BHs with proportionally small masses, including…

Most large galaxies host supermassive black holes in their nuclei and are subject to mergers, which can produce a supermassive black hole binary (SMBHB), and hence periodic signatures due to orbital motion. We report unique periodic radio…

CSS100217 is considered a peculiar tidal disruption event (TDE) candidate occurring in an active galactic nucleus (AGN). Unlike typical TDEs, where the post-flare luminosity is equal to that pre-flare, CSS100217 decayed to $\sim$ 0.4…

High Energy Astrophysical Phenomena · Physics 2025-10-01 Ying Gu , Xiao Li , Xing-Qian Cheng , Dou-Dou Wang , Xue-Guang Zhang , En-Wei Liang

Some electromagnetic outbursts from the nuclei of distant galaxies have been found to repeat on months-to-years timescales, and each of these sources can putatively arise from the accretion flares generated through the repeated tidal…

High Energy Astrophysical Phenomena · Physics 2024-08-30 Ananya Bandopadhyay , Eric R. Coughlin , C. J. Nixon , Dheeraj R. Pasham

We present the results from our multi-wavelength monitoring campaign of the transient AT2022wtn, discovered by the Zwicky Transient Facility in the nucleus of SDSSJ232323.79+104107.7, the less massive galaxy in an active merging pair with a…

Extragalactic nuclear transients that exhibit repeating outbursts can be modeled as the repeated dynamical interaction between bound stars and supermassive black holes (SMBHs). A subset of these transients, with recurrence timescales of…

High Energy Astrophysical Phenomena · Physics 2026-03-06 Ananya Bandopadhyay , Eric R. Coughlin , Julia Fancher , C. J. Nixon , Dheeraj R. Pasham

AT2018cqh is a unique optical tidal disruption event (TDE) discovered in a dwarf galaxy exhibiting delayed X-ray and radio flares. We present the results from high-resolution VLBA and e-MERLIN radio observations of AT2018cqh extending to…

High Energy Astrophysical Phenomena · Physics 2025-09-29 Lei Yang , Xinwen Shu , Guobin Mou , Yongquan Xue , Luming Sun , Fabao Zhang , Zhumao Zhang , Yibo Wang , Tao Wu , Ning Jiang , Hucheng Ding , Tinggui Wang

AT2022rze is a luminous, ambiguous transient located South-East of the geometric center of its host galaxy at redshift z = 0.08. The host appears to be formed by a merging galaxy system. The observed characteristics of AT2022rze are…

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