Direct Detection of Black Hole-driven Turbulence in the Centers of Galaxy Clusters

Li, Yuan; Gendron-Marsolais, Marie-Lou; Zhuravleva, Irina; Xu, Siyao; Simionescu, Aurora; Tremblay, Grant R.; Lochhaas, Cassandra; Bryan, Greg L.; Quataert, Eliot; Murray, Norman W.; Boselli, Alessandro; Hlavacek-Larrondo, Julie; Zheng, Yong; Fossati, Matteo; Li, Miao; Emsellem, Eric; Sarzi, Marc; Arzamasskiy, Lev; Vishniac, Ethan T.

doi:10.3847/2041-8213/ab65c7

Direct Detection of Black Hole-driven Turbulence in the Centers of Galaxy Clusters

Li, Yuan; Gendron-Marsolais, Marie-Lou; Zhuravleva, Irina; Xu, Siyao; Simionescu, Aurora; Tremblay, Grant R.; Lochhaas, Cassandra; Bryan, Greg L.; Quataert, Eliot; Murray, Norman W.; Boselli, Alessandro; Hlavacek-Larrondo, Julie; Zheng, Yong; Fossati, Matteo; Li, Miao; Emsellem, Eric; Sarzi, Marc; Arzamasskiy, Lev; Vishniac, Ethan T.

Authors

Yuan Li

Marie-Lou Gendron-Marsolais

Irina Zhuravleva

Siyao Xu

Aurora Simionescu

Grant R. Tremblay

Cassandra Lochhaas

Greg L. Bryan

Eliot Quataert

Norman W. Murray

Alessandro Boselli

Julie Hlavacek-Larrondo

Yong Zheng

Matteo Fossati

Miao Li

Eric Emsellem

Marc Sarzi

Lev Arzamasskiy

Ethan T. Vishniac

Abstract

Supermassive black holes (SMBHs) are thought to provide energy that prevents catastrophic cooling in the centers of massive galaxies and galaxy clusters. However, it remains unclear how this "feedback" process operates. We use high-resolution optical data to study the kinematics of multiphase filamentary structures by measuring the velocity structure function (VSF) of the filaments over a wide range of scales in the centers of three nearby galaxy clusters: Perseus, A2597, and Virgo. We find that the motions of the filaments are turbulent in all three clusters studied. There is a clear correlation between features of the VSFs and the sizes of bubbles inflated by SMBH-driven jets. Our study demonstrates that SMBHs are the main driver of turbulent gas motions in the centers of relaxed galaxy clusters and suggests that this turbulence is an important channel for coupling feedback to the environment. Our measured amplitude of turbulence is in good agreement with Hitomi Doppler line broadening measurement and X-ray surface-brightness fluctuation analysis, suggesting that the motion of the cold filaments is well-coupled to that of the hot gas. The smallest scales that we probe are comparable to the mean free path in the intracluster medium. Our direct detection of turbulence on these scales provides the clearest evidence to date that isotropic viscosity is suppressed in the weakly collisional, magnetized intracluster plasma.

Citation

Li, Y., Gendron-Marsolais, M., Zhuravleva, I., Xu, S., Simionescu, A., Tremblay, G. R., …Vishniac, E. T. (2020). Direct Detection of Black Hole-driven Turbulence in the Centers of Galaxy Clusters. Astrophysical Journal Letters, 889(1), Article L1. https://doi.org/10.3847/2041-8213/ab65c7

Journal Article Type	Article
Acceptance Date	Dec 23, 2019
Online Publication Date	Jan 17, 2020
Publication Date	Jan 20, 2020
Deposit Date	Mar 11, 2020
Publicly Available Date	Mar 11, 2020
Journal	Astrophysical Journal
Print ISSN	2041-8205
Publisher	American Astronomical Society
Peer Reviewed	Peer Reviewed
Volume	889
Issue	1
Article Number	L1
DOI	https://doi.org/10.3847/2041-8213/ab65c7