AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11

Fuente: arXiv
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Auteurs principaux: Dage, Kristen C., Darc, Phelipe, Pessi, Thallis, Durgesh, Rupesh, Shenoy, Shravya, Nakazono, Lilianne, Boehm, Celine, Chies-Santos, Ana L., de Souza, Rafael S., Kovacs-Stermeczky, Zsofia V., Bahramian, Arash, Bidaran, Bahar, Ishida, Emille E. O., Krone-Martins, Alberto, Patil, Aarya A., Rosa, Reinaldo R., Wille, Andressa, Plotkin, Richard M., Tahmasebzadeh, Behzad
Format: Preprint
Publié: 2025
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author Dage, Kristen C.
Darc, Phelipe
Pessi, Thallis
Durgesh, Rupesh
Shenoy, Shravya
Nakazono, Lilianne
Boehm, Celine
Chies-Santos, Ana L.
de Souza, Rafael S.
Kovacs-Stermeczky, Zsofia V.
Bahramian, Arash
Bidaran, Bahar
Ishida, Emille E. O.
Krone-Martins, Alberto
Patil, Aarya A.
Rosa, Reinaldo R.
Wille, Andressa
Plotkin, Richard M.
Tahmasebzadeh, Behzad
author_facet Dage, Kristen C.
Darc, Phelipe
Pessi, Thallis
Durgesh, Rupesh
Shenoy, Shravya
Nakazono, Lilianne
Boehm, Celine
Chies-Santos, Ana L.
de Souza, Rafael S.
Kovacs-Stermeczky, Zsofia V.
Bahramian, Arash
Bidaran, Bahar
Ishida, Emille E. O.
Krone-Martins, Alberto
Patil, Aarya A.
Rosa, Reinaldo R.
Wille, Andressa
Plotkin, Richard M.
Tahmasebzadeh, Behzad
contents Tidal Disruption Events (TDEs) have long been hypothesized as valuable indicators of black holes, offering insight into their demographics and behaviour out to high redshift. TDEs have also enabled the discovery of a few Massive Black Holes (MBHs) with inferred masses of $10^4$--$10^6\,M_\odot$, often associated with the nuclei of dwarf galaxies or ultra-compact dwarf galaxies (UCDs). Here we present AT2022zod, an extreme and short-lived optical flare in an elliptical galaxy at z=0.11, residing within 3kpc of the galaxy's centre. Its luminosity and ~30-day duration make it unlikely to have originated from the host galaxy's central supermassive black hole (SMBH), which estimate to have a mass around $10^8\,M_\odot$. Assuming that the emission mechanism is consistent with known observed TDEs, we find that such a rapidly evolving transient could either be produced by a MBH in the intermediate-mass range or, alternatively, result from the tidal disruption of a star on a non-parabolic orbit around the central SMBH. We suggest that the most plausible origin for AT2022zod is the tidal disruption of a star by a MBH embedded in a UCD. As the Vera C. Rubin Observatory's Legacy Survey of Space and Time comes online, we propose that AT2022zod serves as an important event for refining search strategies and characterization techniques for intermediate-mass black holes.
format Preprint
id arxiv_https___arxiv_org_abs_2512_02136
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11
Dage, Kristen C.
Darc, Phelipe
Pessi, Thallis
Durgesh, Rupesh
Shenoy, Shravya
Nakazono, Lilianne
Boehm, Celine
Chies-Santos, Ana L.
de Souza, Rafael S.
Kovacs-Stermeczky, Zsofia V.
Bahramian, Arash
Bidaran, Bahar
Ishida, Emille E. O.
Krone-Martins, Alberto
Patil, Aarya A.
Rosa, Reinaldo R.
Wille, Andressa
Plotkin, Richard M.
Tahmasebzadeh, Behzad
High Energy Astrophysical Phenomena
Astrophysics of Galaxies
Tidal Disruption Events (TDEs) have long been hypothesized as valuable indicators of black holes, offering insight into their demographics and behaviour out to high redshift. TDEs have also enabled the discovery of a few Massive Black Holes (MBHs) with inferred masses of $10^4$--$10^6\,M_\odot$, often associated with the nuclei of dwarf galaxies or ultra-compact dwarf galaxies (UCDs). Here we present AT2022zod, an extreme and short-lived optical flare in an elliptical galaxy at z=0.11, residing within 3kpc of the galaxy's centre. Its luminosity and ~30-day duration make it unlikely to have originated from the host galaxy's central supermassive black hole (SMBH), which estimate to have a mass around $10^8\,M_\odot$. Assuming that the emission mechanism is consistent with known observed TDEs, we find that such a rapidly evolving transient could either be produced by a MBH in the intermediate-mass range or, alternatively, result from the tidal disruption of a star on a non-parabolic orbit around the central SMBH. We suggest that the most plausible origin for AT2022zod is the tidal disruption of a star by a MBH embedded in a UCD. As the Vera C. Rubin Observatory's Legacy Survey of Space and Time comes online, we propose that AT2022zod serves as an important event for refining search strategies and characterization techniques for intermediate-mass black holes.
title AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11
topic High Energy Astrophysical Phenomena
Astrophysics of Galaxies
url https://arxiv.org/abs/2512.02136