A research team led by Professor Tinggui Wang from the Department of Astronomy at the University of Science and Technology of China (USTC) of the Chinese Academy of Sciences presented a detailed analysis of a tidal disruption event (TDE) with unique characteristics, providing new insights into the behavior of TDEs and their multiwavelength emissions. Their findings were published online in The Astrophysical Journal Letterson March 26th.
When a star ventures too close to a supermassive black hole at the center of a galaxy, it gets torn apart by the black hole's immense tidal forces, resulting in a phenomenon known as a tidal disruption event (TDE). The research team found that, the AT2023lli event, observed by various ground and space telescopes including the newly constructed Wide Field Survey Telescope (WFST) jointly operated by USTC and Purple Mountain Observatory, exhibited unique features unlike previous TDEs.
Traditionally, TDE light curves display a smooth "rapid rise, slow decline" trend. However, AT2023lli deviated from this pattern significantly. Optical monitoring revealed a strong "bump" in its early light curve, lasting nearly a month and separated by two months from the main peak. This extended and pronounced "bump" is unprecedented in TDE observations to date. The team proposed that the "bump" could be the result of the self-intersection of the stream debris, while the primary peak is likely generated by the reprocessed emission from the accretion process.
Moreover, the team observed delayed and intermittent X-ray emissions compared to optical/Ultraviolet (UV) radiation, which they attributed to the obscuration of the accretion disk by outflowing material, resulting in the absorption and reprocessing of soft X-rays into optical/UV radiation. The intermittent nature of the X-ray emission is suggested to be due to the presence of an inhomogeneous reprocessing layer around the accretion disk, which could be associated with the obscuring material's patchy distribution.
Schematic illustration of the processes that occurred in AT 2023lli, ordered in a chronological sequence from (a) to (f) (Image by the research team).
This study underscores the importance of high-cadence, multiwavelength sampling in understanding the physics of TDEs. WFST's sensitivity advantage was highlighted in providing high-quality multicolor photometric data during the late evolution of AT2023lli. The unique survey design of WFST's high-cadence deep fields, coupled with the recently launched Einstein Probe, holds promise for significant discoveries in transient source research, including TDEs.
(Written by HUANG Rui, edited by JIANG Zhimo, USTC News Center)
