Host galaxies of tidal disruption events (TDEs) show enhanced central stellar concentration and are preferentially found in post-starburst and green valley populations. This connection has led to the proposal that TDE host galaxies likely have gone through recent mergers. We conduct a new morphological study of 14 TDE host galaxies, using the r-band images from Sloan Digital Sky Survey (SDSS), Dark Energy Camera Legacy Survey (DECaLS), and Ultraviolet Near-Infrared Optical Northern Survey (UNIONS), with the images from the latter two surveys having much higher depth and resolution than SDSS. We examine galaxy structures using conventional methods and also apply diagnostics of merger activity from machine learning models. Consistent with previous studies, our results show that TDE host galaxies are ~16% more centrally concentrated when compared to non-TDE-host controls. However, surprisingly, TDE hosts lack any indication of recent merger activity from both morphological analysis and our machine learning merger classifier. Instead, our results reveal that TDE host galaxies are approximately 1.5 to 2.5 times more likely to have bar-like or ring-like structures than their controls. This enhancement is even more prominent for TDEs in the green valley, with the factor reaching almost 3. Based on these results, we propose that bar-driven secular evolution, instead of merger, likely dominates the recent evolution of TDE hosts found in the green valley, which can simultaneously explain their distinctive nuclear properties and enhanced TDE rates.
@article{arxiv.2602.06839,
title = {Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies},
author = {Janet N. Y. Chang and Connor Bottrell and Lixin Dai and Rudrani Kar Chowdhury and Meng Gu and Renbin Yan and Leonardo Ferreira and Sara L. Ellison and Scott Wilkinson and Thomas de Boer},
journal= {arXiv preprint arXiv:2602.06839},
year = {2026}
}