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X-ray cavities in TNG-Cluster: a direct comparison to observations

The TNG-Cluster magnetohydrodynamic cosmological simulations produce a diverse population of X-ray cavities in the intracluster medium (ICM) of simulated galaxy clusters. These arise from episodic, high velocity, kinetic energy injections from the central active supermassive black hole (AGN, SMBH)....

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Hauptverfasser: Prunier, Marine (VerfasserIn) , Pillepich, Annalisa (VerfasserIn) , Hlavacek-Larrondo, Julie (VerfasserIn) , Nelson, Dylan (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: May 2025
In: Monthly notices of the Royal Astronomical Society
Year: 2025, Jahrgang: 539, Heft: 2, Pages: 1040-1064
ISSN:1365-2966
DOI:10.1093/mnras/staf525
Online-Zugang:Verlag, kostenfrei, Volltext: https://doi.org/10.1093/mnras/staf525
Volltext
Verfasserangaben:Marine Prunier, Annalisa Pillepich, Julie Hlavacek-Larrondo and Dylan Nelson
Beschreibung
Zusammenfassung:The TNG-Cluster magnetohydrodynamic cosmological simulations produce a diverse population of X-ray cavities in the intracluster medium (ICM) of simulated galaxy clusters. These arise from episodic, high velocity, kinetic energy injections from the central active supermassive black hole (AGN, SMBH). Here, we present the first comprehensive comparative analysis of X-ray cavities in TNG-Cluster with observational data. First, we select a volume-limited sample of 35 real clusters
Beschreibung:Veröffentlicht: 01. April 2025
Gesehen am 30.09.2025
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/staf525

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