Detection of disk-jet coprecession in a tidal disruption event

  • Yanan Wang
  • , Zikun Lin
  • , Linhui Wu
  • , Wei-Hua Lei
  • , Shuyuan Wei
  • , Shuang-Nan Zhang
  • , Long Ji
  • , Santiago Del Palacio
  • , Ranieri D Baldi
  • , Yang Huang
  • , Ji-Feng Liu
  • , Bing Zhang
  • , Aiyuan Yang
  • , Ru-Rong Chen
  • , Yangwei Zhang
  • , Ai-Ling Wang
  • , Lei Yang
  • , Panos Charalampopoulos
  • , David R A Williams-Baldwin
  • , Zhu-Heng Yao
  • Fu-Guo Xie, Defu Bu, Hua Feng, Xinwu Cao, Hongzhou Wu, Wenxiong Li, Erlin Qiao, Giorgos Leloudas, Joseph P Anderson, Xinwen Shu, Dheeraj R Pasham, Hu Zou, Matt Nicholl, Thomas Wevers, Tomás E Müller-Bravo, Jing Wang, Jian-Yan Wei, Yu-Lei Qiu, Wei-Jian Guo, Claudia P Gutiérrez, Mariusz Gromadzki, Cosimo Inserra, Lydia Makrygianni, Francesca Onori, Tanja Petrushevska, Diego Altamirano, Lluís Galbany, Miguel Peréz-Torres, Ting-Wan Chen

Research output: Contribution to journalArticlepeer-review

Abstract

Theories and simulations predict that intense space-time curvature near black holes bends the trajectories of light and matter, driving disk and jet precession under relativistic torques. However, direct observational evidence of disk-jet coprecession remains elusive. Here, we report the most compelling case to date: a tidal disruption event (TDE) exhibiting unprecedented 19.6-day quasi-periodic variations in both x-rays and radio, with x-ray amplitudes exceeding an order of magnitude. The nearly synchronized x-ray and radio variations suggest a shared mechanism regulating the emission regions. We demonstrate that a disk-jet Lense-Thirring precession model successfully reproduces these variations while requiring a low-spin black hole. This study uncovers previously uncharted short-term radio variability in TDEs, highlights the transformative potential of high-cadence radio monitoring, and offers profound insights into disk-jet physics.
Original languageEnglish
Article numbeready9068
Number of pages15
JournalScience Advances
Volume11
Issue number50
DOIs
Publication statusPublished - 10 Dec 2025

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