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Galaxy-scale consequences of tidal disruption events: extended emission-line regions, extreme coronal lines, and infrared-to-optical light echoes

Abstract:
Stars in galactic centres are occasionally scattered so close to the central supermassive black hole that they are completely disrupted by tidal forces, initiating a transient accretion event. The aftermath of such a tidal disruption event (TDE) produces a bright-and-blue accretion flow that is known to persist for at least a decade (observationally) and can in principle produce ionizing radiation for hundreds of years. TDEs are known (observationally) to be overrepresented in galaxies that show extended emission-line regions (EELRs), with no pre-TDE classical active galactic nucleus activity, and to produce transient ‘coronal lines’, such as [Fe x] and [Fe xiv]. Using coupled cloudy-TDE disc simulations we show that TDE discs produce a sufficient ionizing radiation flux over their lifetimes to power both EELR of radial extents of light years, and coronal lines. EELRs are produced when the ionizing radiation interacts with low-density () clouds on galactic scales, while coronal lines are produced by high-density () clouds near the galactic centre. High-density gas in galactic centres will also result in the rapid switching on of narrow-line features in post-TDE galaxies, and also various high-ionization lines, which may be observed throughout the infrared with James Webb Space Telescope. Galaxies with a higher intrinsic rate of TDEs will be more likely to show macroscopic EELRs, which can be traced to originate from the previous TDE in that galaxy.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1093/mnras/staf1649

Authors

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Institution:
University of Oxford
Role:
Author
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Role:
Author
ORCID:
0000-0002-3493-7737
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Role:
Author
ORCID:
0000-0001-5578-359X


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Funder identifier:
https://ror.org/012mzw131


Publisher:
Oxford University Press
Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
544
Issue:
2
Pages:
2262-2295
Article number:
staf1649
Publication date:
2025-09-27
Acceptance date:
2025-09-23
DOI:
EISSN:
1365-2966
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
2301973
UUID:
uuid_d05d79f4-6c60-490f-9bd4-ff5c689b5c33
Local pid:
pubs:2301973
Source identifiers:
3487004
Deposit date:
2025-11-19
ARK identifier:
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