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SUMMARY:Dense gas in galaxy clusters under the influence of an AGN jet - R
 icarda Beckmann
DTSTART:20201111T140000Z
DTEND:20201111T143000Z
UID:TALK150385@talks.cam.ac.uk
CONTACT:Emma Curtis Lake
DESCRIPTION:Extended filamentary nebulae of cold\, dense gas are a strikin
 g feature of nearby brightest cluster galaxies\, and represent an importan
 t component of the gas life cycle in galaxy clusters.  While their formati
 on mechanism and the processes which shape their morphology remain areas o
 f research\, the huge cavities frequently observed in the circumgalactic m
 edium\, which are inflated by the AGN driven jets of the Brightest Cluster
  Galaxy\, play a decisive role in the formation and evolution of these neb
 ulae. These emission nebulae therefore represent one of the most direct ex
 amples of AGN influencing the gas life cycle in and around their host gala
 xies. In this talk\, I will present work that uses simulations to investig
 ate the condensation and evolution of this cold gas under the influence of
  a spin-driven AGN jet in a Perseus-like clusters. 
LOCATION: Webinar  (via Zoom online)
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