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astro-ph.HE2025
Numerical Simulations of the Circularized Accretion Flow in Population III Star Tidal Disruption Events. I. The Accretion Flow and the Wind
Yu-Heng Sheng, De-Fu Bu, Xiao-Hong Yang +2
Tidal Disruption Events (TDEs) have recently been proposed as potential probes for Population III stars. However, the properties of the accretion flow and the wind from the Pop III…
astro-ph.HE2025
Line-force driven wind from a thin disk in tidal disruption event
De-Fu Bu, Xiao-Hong Yang, Liang Chen +2
Winds from the accretion disk in tidal disruption events (TDEs) play a key role in determining the radiation of TDEs. The winds from the super-Eddington accretion phase in TDEs hav…
astro-ph.HE2025
Numerical simulations of the line-force-driven winds from active galactic nuclei: The special relativistic effects
Luobin Tang, Xiaohong Yang, Defu Bu
Ultra-fast outflows (UFOs) with mildly relativistic velocities are frequently observed in active galactic nuclei (AGNs). The line-force-driving mechanism is often taken as a potent…