Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81

Studying a centi-parsec supermassive black hole binary (SMBHB) would allow us to explore a new parameter space in active galactic nuclei, and these objects are also potential sources of gravitational waves. We report evidence that an SMBHB with an orbital period of ∼30 yr may be resident in the near...

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Main Authors: Wu Jiang, Zhiqiang Shen, Ivan Martí-Vidal, Zhen Yan, Lei Huang, Roman Gold, Ya-Ping Li, Fuguo Xie, Noriyuki Kawaguchi
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad063d
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author Wu Jiang
Zhiqiang Shen
Ivan Martí-Vidal
Zhen Yan
Lei Huang
Roman Gold
Ya-Ping Li
Fuguo Xie
Noriyuki Kawaguchi
author_facet Wu Jiang
Zhiqiang Shen
Ivan Martí-Vidal
Zhen Yan
Lei Huang
Roman Gold
Ya-Ping Li
Fuguo Xie
Noriyuki Kawaguchi
author_sort Wu Jiang
collection DOAJ
description Studying a centi-parsec supermassive black hole binary (SMBHB) would allow us to explore a new parameter space in active galactic nuclei, and these objects are also potential sources of gravitational waves. We report evidence that an SMBHB with an orbital period of ∼30 yr may be resident in the nearby galactic nucleus M81. This orbital period and the known mass of M81 imply an orbital separation of ∼0.02 pc. The jet emanating from the primary black hole showed a short period of jet wobbling at ∼16.7 yr, superposing a long-term precession at a timescale of several hundred years. Periodic radio and X-ray outbursts were also found two times per orbital period, which could be explained by a double-peaked mass accretion rate variation per binary orbit. If confirmed, M81 would be one of the closest SMBHB candidates, providing a rare opportunity to study the final parsec problem .
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spelling doaj.art-dada47267beb47d1b7af4036c86aa9802023-11-29T16:11:02ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0195911110.3847/1538-4357/ad063dObservational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81Wu Jiang0https://orcid.org/0000-0001-7369-3539Zhiqiang Shen1https://orcid.org/0000-0003-3540-8746Ivan Martí-Vidal2https://orcid.org/0000-0003-3708-9611Zhen Yan3https://orcid.org/0000-0002-5385-9586Lei Huang4https://orcid.org/0000-0002-1923-227XRoman Gold5https://orcid.org/0000-0003-2492-1966Ya-Ping Li6https://orcid.org/0000-0002-7329-9344Fuguo Xie7https://orcid.org/0000-0001-9969-2091Noriyuki Kawaguchi8https://orcid.org/0000-0002-7776-3159Shanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cn; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing 100101, People's Republic of ChinaShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cn; Key Laboratory of Radio Astronomy and Technology, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing 100101, People's Republic of ChinaDepartamento de Astronomía y Astrofísica, Universitat de València , C/Dr. Moliner 50, Agustín Escardino, E-46100 Burjassot, Spain; Observatori Astronòmic, Universitat de València , C/Cat. Agustín Escardino 2, E-16980 Paterna, SpainShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cnShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cnCP3-Origins, University of Southern Denmark , Campusvej 55, DK-5230 Odense M, DenmarkShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cnShanghai Astronomical Observatory, Chinese Academy of Sciences , Shanghai 200030, People's Republic of China ; jiangwu@shao.ac.cn, zshen@shao.ac.cnNational Astronomical Observatory of Japan , 2-21-1 Osawa, Mitaka, Tokyo 181-8588, JapanStudying a centi-parsec supermassive black hole binary (SMBHB) would allow us to explore a new parameter space in active galactic nuclei, and these objects are also potential sources of gravitational waves. We report evidence that an SMBHB with an orbital period of ∼30 yr may be resident in the nearby galactic nucleus M81. This orbital period and the known mass of M81 imply an orbital separation of ∼0.02 pc. The jet emanating from the primary black hole showed a short period of jet wobbling at ∼16.7 yr, superposing a long-term precession at a timescale of several hundred years. Periodic radio and X-ray outbursts were also found two times per orbital period, which could be explained by a double-peaked mass accretion rate variation per binary orbit. If confirmed, M81 would be one of the closest SMBHB candidates, providing a rare opportunity to study the final parsec problem .https://doi.org/10.3847/1538-4357/ad063dVery long baseline interferometrySupermassive black holes
spellingShingle Wu Jiang
Zhiqiang Shen
Ivan Martí-Vidal
Zhen Yan
Lei Huang
Roman Gold
Ya-Ping Li
Fuguo Xie
Noriyuki Kawaguchi
Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
The Astrophysical Journal
Very long baseline interferometry
Supermassive black holes
title Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
title_full Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
title_fullStr Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
title_full_unstemmed Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
title_short Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
title_sort observational evidence of a centi parsec supermassive black hole binary existing in the nearby galaxy m81
topic Very long baseline interferometry
Supermassive black holes
url https://doi.org/10.3847/1538-4357/ad063d
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