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SUMMARY:The structure of the interstellar medium as probe of the baryonic 
 physics of galaxy evolution - Jindra Gensior (University of Zurich)
DTSTART:20231103T113000Z
DTEND:20231103T123000Z
UID:TALK206752@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:Understanding what shapes the cold gas component of galaxies i
 s crucial to our understanding of galaxy evolution. Not only because cold 
 gas provides the fuel for star formation\, but also because its structural
  and kinematic properties are affected by the resultant stellar feedback. 
 I will present detailed analysis of isolated galaxy and cosmological simul
 ations and discuss how the interstellar medium (and star formation) are af
 fected by the gravitational potential of galaxies\, as well as how the int
 erstellar medium structure can be a probe for different star formation and
  feedback models. 
LOCATION:Ryle seminar room + online
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