A Host Galaxy Morphology Link Between Quasi-Periodic Eruptions and Tidal Disruption Events
Olivier Gilbert, John J. Ruan, Michael Eracleous, Daryl Haggard,, Jessie C. Runnoe

TL;DR
This study finds that galaxies hosting Quasi-Periodic Eruptions (QPEs) share morphological features with Tidal Disruption Event (TDE) hosts, supporting a physical connection between QPEs and TDEs through galaxy structure analysis.
Contribution
It provides the first comparative analysis of QPE and TDE host galaxy morphologies, revealing significant similarities that suggest a common physical origin.
Findings
QPE host galaxies have high Sersic indices (~3)
QPE host galaxies have high B/T ratios (~0.5)
QPE and TDE hosts have high surface mass densities (~10^10 Msun kpc^-2)
Abstract
The physical processes that produce X-ray Quasi-Periodic Eruptions (QPEs) recently discovered from the nuclei of several low-redshift galaxies are mysterious. Several pieces of observational evidence strongly suggest a link between QPEs and Tidal Disruption Events (TDE). Previous studies also reveal that the morphologies of TDE host galaxies are highly concentrated, with high Sersic indicies, bulge-to-total light (B/T) ratios, and stellar surface mass densities relative to the broader galaxy population. We use these distinctive properties to test the link between QPEs and TDEs, by comparing these parameters of QPE host galaxies to TDE host galaxies. We employ archival Legacy Survey images of a sample of 9 QPE host galaxies and a sample of 13 TDE host galaxies, and model their surface brightness profiles. We show that QPE host galaxies have high Sersic indices of ~3, high B/T ratios of…
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Taxonomy
Topicsearthquake and tectonic studies
