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Investigating changing-look active galactic nuclei with long-term optical and X-ray observations

Jana, A.; Ricci, C.; Temple, M. J.; Chang, H. K.; Shablovinskaya, E.; Trakhtenbrot, B.; Diaz, Y.; Ilic, D.; Nandi, P.; Koss, M.

Investigating changing-look active galactic nuclei with long-term optical and X-ray observations Thumbnail


Authors

A. Jana

C. Ricci

H. K. Chang

E. Shablovinskaya

B. Trakhtenbrot

Y. Diaz

D. Ilic

P. Nandi

M. Koss



Abstract

Context. Broad emission lines in the UV/optical spectra of changing-look active galactic nuclei (CLAGNs) appear and disappear on timescales of months to decades. Aims. We investigate how changing-look (CL) transitions depend on several active galactic nucleus (AGN) parameters, such as the accretion rate, obscuration properties, and black hole mass. Methods. We studied a sample of 20 nearby optically identified CLAGNs from the BAT AGN Spectroscopic Survey (BASS) using quasi-simultaneous optical and X-ray observations taken in the last ∼40 years. Results. We find that for all CLAGNs, the transition is accompanied by a change in the Eddington ratio. The CL transitions are not associated with changes in the obscuration properties of the AGNs. CLAGNs are found to have a median Eddington ratio lower than that of the AGNs in the BASS sample in which CL transitions were not detected. The median transition Eddington ratio (the Eddington ratio at which an AGN changes its state) is found to be ∼0.01 for type 1 ↔ 1.8, 1.9, and 2 transitions, which is consistent with the hard ↔ soft state transition in black hole X-ray binaries. Most CL events are constrained to have occurred within 3-4 years, which is considerably shorter than the expected viscous timescale in AGN accretion disks. Conclusions. The transitions of the optical CLAGNs studied here are likely associated with state changes in the accretion flow, possibly driven by disk instability.

Citation

Jana, A., Ricci, C., Temple, M. J., Chang, H. K., Shablovinskaya, E., Trakhtenbrot, B., Diaz, Y., Ilic, D., Nandi, P., & Koss, M. (2025). Investigating changing-look active galactic nuclei with long-term optical and X-ray observations. Astronomy & Astrophysics, 693, Article A35. https://doi.org/10.1051/0004-6361/202451058

Journal Article Type Article
Acceptance Date Nov 13, 2024
Online Publication Date Jan 3, 2025
Publication Date Jan 1, 2025
Deposit Date Mar 26, 2025
Publicly Available Date Mar 26, 2025
Journal Astronomy and Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 693
Article Number A35
DOI https://doi.org/10.1051/0004-6361/202451058
Public URL https://durham-repository.worktribe.com/output/3742644

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0),
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.





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