Prevalence of Tidal Interactions among Local Seyfert Galaxies
Cheng-Yu Kuo, Jeremy Lim, Ya-Wen Tang, Paul T. P. Ho

TL;DR
This study reveals that most local Seyfert galaxies show significant tidal disturbances in hydrogen gas, strongly linking such interactions to the initiation of their nuclear activity, despite optical images showing minimal disturbance.
Contribution
First systematic analysis using HI gas to demonstrate high prevalence of tidal interactions in Seyfert galaxies, highlighting their role in triggering nuclear activity.
Findings
94% of Seyfert galaxies disturbed in HI
28% visibly disturbed in optical images
Tidal interactions with nearby galaxies are common
Abstract
No mechanisms have hitherto been conclusively demonstrated to be responsible for initiating optically-luminous nuclear (Seyfert) activity in local disk galaxies. Only a small minority of such galaxies are visibly disturbed in optical starlight, with the observed disturbances being at best marginally stronger than those found in matched samples of inactive galaxies. Here, we report the first systematic study of an optically-selected sample of twenty-three active galaxies in atomic hydrogen (HI) gas, which is the most sensitive and enduring tracer known of tidal interactions. Eighteen of these galaxies are (generally) classified as Seyferts, with over half (and perhaps all) having [OIII] luminosities within two orders of magnitude of Quasi-Stellar Objects. Only ~28% of these Seyfert galaxies are visibly disturbed in optical DSS2 images. By contrast, ~94% of the same galaxies are disturbed…
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