An Extraordinary Response of Iron Emission to the Central Outburst in a Tidal Disruption Event Candidate
Zhicheng He (USTC), Ning Jiang, Tinggui Wang, Guilin Liu, Mouyuan Sun,, Hengxiao Guo, Lu Shen, Zhenyi Cai, Xinwen Shu, Zhenfeng Sheng, Zhixiong Liang, and Youhua Xu

TL;DR
This study observes a unique hysteresis in iron emission response during a tidal disruption event, linking dust sublimation to iron emission and suggesting new uses for eii\ as a cosmic probe.
Contribution
First detection of hysteresis in eii\ emission response during a TDE, proposing dust sublimation as the mechanism behind iron emission variability.
Findings
eii\ response is stronger during luminosity rise than decline.
Dust sublimation explains the hysteresis effect in eii\ emission.
eii\ emission can serve as a standard candle for cosmology.
Abstract
Understanding the origin of \feii\ emission is important because it is crucial to construct the main sequence of Active Galactic Nuclei (AGNs). Despite several decades of observational and theoretical effort, the location of the optical iron emitting region and the mechanism responsible for the positive correlation between the \feii\ strength and the black hole accretion rate remain open questions as yet. In this letter, we report the optical \feii\ response to the central outburst in PS1-10adi, a candidate tidal disruption event (TDE) taking place in an AGN at that has aroused extensive attention. For the first time, we observe that the \feii\ response in the rising phase of its central luminosity is significantly more prominent than that in the decline phase, showing a hysteresis effect. We interpret this hysteresis effect as a consequence of the gradual sublimation of the…
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