Investigating the Intracluster Medium Viscosity Using the Tails of GASP Jellyfish Galaxies

Investigating the Intracluster Medium Viscosity Using the Tails of GASP Jellyfish Galaxies

The microphysics of the intracluster medium (ICM) in galaxy clusters is still poorly understood. Observational evidence suggests that the effective viscosity is suppressed by plasma instabilities that reduce the mean free path of particles. Measuring the effective viscosity of the ICM is crucial to...

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Bibliographic Details
Main Authors: Alessandro Ignesti, Gianfranco Brunetti, Marco Gullieuszik, Nina Akerman, Antonino Marasco, Bianca M. Poggianti, Yuan Li, Benedetta Vulcani, Myriam Gitti, Alessia Moretti, Eric Giunchi, Neven Tomičić, Cecilia Bacchini, Rosita Paladino, Mario Radovich, Anna Wolter
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Galaxy clusters
Intracluster medium
Plasma astrophysics
Galaxies
Online Access:https://doi.org/10.3847/1538-4357/ad919b
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https://doi.org/10.3847/1538-4357/ad919b

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