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SUMMARY:A disturbing FABLE of mergers\, feedback\, turbulence\, and mass b
 iases in simulated galaxy clusters - Jake Bennet
DTSTART:20220427T121500Z
DTEND:20220427T124500Z
UID:TALK173426@talks.cam.ac.uk
CONTACT:Hannah Uebler
DESCRIPTION:The use of galaxy clusters as cosmological probes often relies
  on understanding the properties and evolution of ICM. However\, the ICM i
 s a complex plasma\, regularly stirred by mergers and feedback\, with non-
 negligible bulk and turbulent motions and a non-thermal pressure component
 \, making it difficult to construct a coherent and comprehensive picture. 
 To this end\, we use the FABLE simulations to investigate how the hydrosta
 tic mass bias is affected by cluster dynamical state\, mergers\, AGN feedb
 ack and turbulence over cosmic time. We also look at how this links to the
  evolution of chemo-thermodynamic cluster profiles\, compared to observati
 ons and other simulations.
LOCATION:The Hoyle Lecture Theatre + Zoom 
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