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The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View

Rosa, Alessandra De; Vignali, Cristian; Bogdanović, Tamara; Capelo, Pedro R.; Charisi, Maria; Dotti, Massimo; Husemann, Bernd; Lusso, Elisabeta; Mayer, Lucio; Paragi, Zsolt; Runnoe, Jessie; Sesana, Alberto; Steinborn, Lisa; Bianchi, Stefano; Colpi, Monica; Valle, Luciano Del; Frey, Sándor; Gabányi, Krisztina É; Giustini, Margherita; Guainazzi, Matteo; Haiman, Zoltan; Ruiz, Noelia Herrera; Herrero-Illana, Rubén; Iwasawa, Kazushi; Komossa, S.; Lena, Davide; Loiseau, Nora; Perez-Torres, Miguel; Piconcelli, Enrico; Volonteri, Marta

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Authors

Alessandra De Rosa

Cristian Vignali

Tamara Bogdanović

Pedro R. Capelo

Maria Charisi

Massimo Dotti

Bernd Husemann

Lucio Mayer

Zsolt Paragi

Jessie Runnoe

Alberto Sesana

Lisa Steinborn

Stefano Bianchi

Monica Colpi

Luciano Del Valle

Sándor Frey

Krisztina É Gabányi

Margherita Giustini

Matteo Guainazzi

Zoltan Haiman

Noelia Herrera Ruiz

Rubén Herrero-Illana

Kazushi Iwasawa

S. Komossa

Davide Lena

Nora Loiseau

Miguel Perez-Torres

Enrico Piconcelli

Marta Volonteri



Abstract

The quest for binary and dual supermassive black holes (SMBHs) at the dawn of the multi-messenger era is compelling. Detecting dual active galactic nuclei (AGN) – active SMBHs at projected separations larger than several parsecs – and binary AGN – probing the scale where SMBHs are bound in a Keplerian binary – is an observational challenge. The study of AGN pairs (either dual or binary) also represents an overarching theoretical problem in cosmology and astrophysics. The AGN triggering calls for detailed knowledge of the hydrodynamical conditions of gas in the imminent surroundings of the SMBHs and, at the same time, their duality calls for detailed knowledge on how galaxies assemble through major and minor mergers and grow fed by matter along the filaments of the cosmic web. This review describes the techniques used across the electromagnetic spectrum to detect dual and binary AGN candidates and proposes new avenues for their search. The current observational status is compared with the state-of-the-art numerical simulations and models for formation of dual and binary AGN. Binary SMBHs are among the loudest sources of gravitational waves (GWs) in the Universe. The search for a background of GWs at nHz frequencies from inspiralling SMBHs at low redshifts, and the direct detection of signals from their coalescence by the Laser Interferometer Space Antenna in the next decade, make this a theme of major interest for multi-messenger astrophysics. This review discusses the future facilities and observational strategies that are likely to significantly advance this fascinating field.

Citation

Rosa, A. D., Vignali, C., Bogdanović, T., Capelo, P. R., Charisi, M., Dotti, M., …Volonteri, M. (2019). The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View. New Astronomy Reviews, 86, Article 101525. https://doi.org/10.1016/j.newar.2020.101525

Journal Article Type Article
Acceptance Date Jan 28, 2020
Online Publication Date Feb 11, 2020
Publication Date Dec 31, 2019
Deposit Date Feb 12, 2020
Publicly Available Date Feb 11, 2022
Journal New Astronomy Reviews
Print ISSN 1387-6473
Publisher Elsevier
Peer Reviewed Peer Reviewed
Volume 86
Article Number 101525
DOI https://doi.org/10.1016/j.newar.2020.101525

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