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SUMMARY:AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphas
 e outflows? - Samuel Ward (Newcastle/ESO)
DTSTART:20231117T113000Z
DTEND:20231117T123000Z
UID:TALK205300@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:In this talk\, I will present our simulations of an AGN wind e
 mbedded within a spatially-resolved\, clumpy ISM to reveal the effect of I
 SM structure on the propagation of AGN-driven outflows. I will also discus
 s the observational implications of this work\, for example\, in the const
 ruction of AGN-galaxy scaling relations\, and how can we observationally c
 onstrain whether an outflow is energy or momentum driven.\n
LOCATION:Ryle seminar room + online
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