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Tracking the spectral properties of ESO 511-G030 across different epochs

Middei, R.; Petrucci, P.-O.; Bianchi, S.; Ursini, F.; Matzeu, G. A.; Vagnetti, F.; Tortosa, A.; Marinucci, A.; Matt, G.; Piconcelli, E.; De Rosa, A.; De Marco, B.; Reeves, J.; Perri, M.; Guainazzi, M.; Cappi, M.; Done, C.

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Authors

R. Middei

P.-O. Petrucci

S. Bianchi

F. Ursini

G. A. Matzeu

F. Vagnetti

A. Tortosa

A. Marinucci

G. Matt

E. Piconcelli

A. De Rosa

B. De Marco

J. Reeves

M. Perri

M. Guainazzi

M. Cappi



Abstract

The Type 1 active galactic nucleus (AGN) ESO 511-G030, a formerly bright and soft excess dominated source, was observed in 2019 in the context of a multi-wavelength monitoring campaign. In the new exposures, the source was found to be in a flux state approximately ten times lower than archival exposures and without any trace of the soft excess. Interestingly, the X-ray weakening observed in the 2019 data corresponds to a comparable fading of the UV flux, suggesting a strong link between these two components. The UV-X-ray spectral energy distribution (SED) of ESO 511-G030 shows remarkable variability. We tested both phenomenological and physically motivated models on the data, finding that the overall emission spectrum of ESO 511-G030 in this extremely low flux state is due to the superposition of a power-law-like continuum (Γ ∼ 1.7) and two reflection components emerging from hot and cold matter. Both the primary X-ray continuum and relativistic reflection are produced in the inner regions close to the supermassive black hole. The prominent variability of ESO 511-G030 and the lack of a soft excess can be explained by the dramatic change in the observed accretion rate, which dropped from an L/LEdd of 2% in 2007 to one of 0.2% in 2019. The X-ray photon index also became harder during the low flux observations from 2019, perhaps as a result of a photon starved X-ray corona.

Citation

Middei, R., Petrucci, P., Bianchi, S., Ursini, F., Matzeu, G. A., Vagnetti, F., …Done, C. (2023). Tracking the spectral properties of ESO 511-G030 across different epochs. Astronomy & Astrophysics, 672, 1-17. https://doi.org/10.1051/0004-6361/202244022

Journal Article Type Article
Acceptance Date Feb 4, 2023
Online Publication Date Apr 5, 2023
Publication Date 2023-04
Deposit Date Nov 8, 2023
Publicly Available Date Nov 8, 2023
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 672
Article Number A101
Pages 1-17
DOI https://doi.org/10.1051/0004-6361/202244022
Keywords Space and Planetary Science; Astronomy and Astrophysics
Public URL https://durham-repository.worktribe.com/output/1901679

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http://creativecommons.org/licenses/by/4.0/

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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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Published Journal Article





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