NGC 3227 Blinks: An Extreme Changing-look Event in a Seyfert Galaxy

Abstract We report a rapid optical changing-look event in the Seyfert galaxy NGC 3227: the optical continuum faded by ∼70%, and broad H β emission nearly disappeared within weeks before recovering within 2 months. Damped random walk simulations calibrated to the source’s normal variability show that such a decline is unlikely for stochastic accretion fluctuations. The optical decline coincides with an X-ray spectral hardening event detected by Swift, indicating additional line-of-sight absorption. During the dim state, reverberation mapping yields a clear 6–8 day lag between the continuum and broad H β , placing the obscurer interior to the broad-line region. Photoionization calculations require a fully ionized Compton-thick column with N H ≈ 1.5 × 10 24 cm −2 to reproduce the optical continuum suppression. Together, these observations demonstrate that compact, high-column-density obscurers interior to the broad-line region can produce extreme optical changing-look behavior on timescales of weeks.

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Journal
The Astrophysical Journal Letters
Published
2026-11-06
DOI
https://doi.org/10.3847/2041-8213/aeb6c3
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
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article

NGC 3227 Blinks: An Extreme Changing-look Event in a Seyfert Galaxy

Feng-Na Fang, Kaiwen Zhang, Daniel Proga A, K. Horne et al.
The Astrophysical Journal Letters
Astrophysical Phenomena and Observations
article

NGC 3227 Blinks: An Extreme Changing-look Event in a Seyfert Galaxy

Feng-Na Fang, Kaiwen Zhang, Daniel Proga A, K. Horne, M. S. Brotherton, Dong-Wei Bao, Bi-Xuan Zhao, Gerard A. Kriss, Jian Wang, Ming Xiao, Chen Hu, Pu Du, Yan-Rong Li
article en

Abstract

Abstract We report a rapid optical changing-look event in the Seyfert galaxy NGC 3227: the optical continuum faded by ∼70%, and broad H β emission nearly disappeared within weeks before recovering within 2 months. Damped random walk simulations calibrated to the source’s normal variability show that such a decline is unlikely for stochastic accretion fluctuations. The optical decline coincides with an X-ray spectral hardening event detected by Swift, indicating additional line-of-sight absorption. During the dim state, reverberation mapping yields a clear 6–8 day lag between the continuum and broad H β , placing the obscurer interior to the broad-line region. Photoionization calculations require a fully ionized Compton-thick column with N H ≈ 1.5 × 10 24 cm −2 to reproduce the optical continuum suppression. Together, these observations demonstrate that compact, high-column-density obscurers interior to the broad-line region can produce extreme optical changing-look behavior on timescales of weeks.

The Astrophysical Journal LettersVol. 1011(2)
University of Wyoming (US), Space Telescope Science Institute (US), University of Nevada, Reno (US), Chinese Academy of Sciences (CN), University of Chinese Academy of Sciences (CN)
National Science Foundation, California Institute of Technology, Northwestern University, University of Washington, University of Warwick, Trinity College Dublin, National Natural Science Foundation of China, Stockholms Universitet, National Science and Technology Major Project, Deutsches Elektronen-Synchrotron, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 30%
Astrophysical Phenomena and Observations
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