Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies
Janet N.Y. Chang, Connor Bottrell, Lixin Dai, Rudrani Kar Chowdhury, Meng Gu, Renbin Yan, Leonardo Ferreira, Sara L. Ellison, Scott Wilkinson, Thomas de Boer

TL;DR
This study investigates the morphological features of TDE host galaxies, finding that bars and rings, rather than recent mergers, are more common and may drive the conditions leading to tidal disruption events.
Contribution
It introduces a new morphological analysis using deep survey data and machine learning to challenge the merger hypothesis, highlighting bar-driven evolution in TDE hosts.
Findings
TDE hosts are ~16% more centrally concentrated than controls.
No evidence of recent mergers in TDE hosts from morphology or machine learning.
TDE hosts are 1.5 to 2.5 times more likely to have bars or rings.
Abstract
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,…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Gamma-ray bursts and supernovae · Astronomy and Astrophysical Research
