Years Delayed X-ray Afterglows of TDEs Originated from Wind-Torus Interactions

TL;DR

This paper proposes that delayed X-ray afterglows in TDEs originate from interactions between ultrafast winds and preexisting AGN tori, with analytical and simulation support, providing new insights into TDE environments.

Contribution

The study introduces a novel model explaining delayed X-ray emissions in TDEs through wind-torus interactions, supported by analytical calculations and simulations.

Findings

X-ray afterglows can occur years after TDEs due to wind-torus collisions.

X-ray luminosity can reach 10^{41-42} erg/s depending on parameters.

Model applied to TDE candidates constrains star masses and torus gas densities.

Abstract

Tidal disruption events (TDEs) occurred in active galactic nuclei (AGNs) are a special class of sources with outstanding scientific significance. TDEs can generate ultrafast winds, which should almost inevitably collide with the preexisting AGN dusty tori. We perform analytical calculations and simulations on the wind-torus interactions and find such a process can generate considerable X-ray afterglow radiation several years or decades later after the TDE outburst. This provides a new origin for the years delayed X-rays in TDEs. The X-ray luminosity can reach 10^{41-42} erg/s, and the light curve characteristics depend on the parameters of winds and tori. We apply the model to two TDE candidates, and provide lower limits on the masses of the disrupted stars, as well as rigorous constraints on the gas densities of tori. Our results suggest that the observations of the time delay, spectral shape, luminosity and the light curve of the X-ray afterglow can be used to constrain the physical parameters of both TDE winds and tori, including the wind velocity, wind density and torus density.