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PRODID:-//Heidelberg University//HePhySTO//EN
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DTEND:20260430T101500Z
UID:61ca4b842163b14ca497c567c23a5306@physik.uni-heidelberg.de
DTSTAMP:20260411T175101Z
LOCATION:ARI\, Moenchhofstrasse 12-14\, Seminarraum 1.OG
DESCRIPTION:Barred galaxies tend to exhibit a dense and highly star forming
  \nregion at their center\, called Central Molecular Zone (CMZ). Gas dynami
 cs and star \nformation in CMZs are fundamentally shaped by the complex gas
  motions and extreme \nconditions of the region. Leveraging dedicated radia
 tion-MHD simulations we compare \nISM properties and star formation in such
  a region to a Solar-neighborhood type of \nenvironment\, highlighting and 
 understanding differences. Importantly\, strong shear\, \nshort orbital tim
 escales and frequent cloud collisions\, tend to decouple stars from \ntheir
  surrounding gas early in their evolution\, when feedback is still active. 
 This \nhas important consequences on how stellar feedback couples back to t
 he ISM and changes \nthe classical picture of how HII regions and superbubb
 les evolve.\n\nImported from https://www.physik.uni-heidelberg.de/hephysto/
  (no warranty for accuracy).
URL;VALUE=URI:https://www.physik.uni-heidelberg.de/hephysto/index.php?s=tal
 k&id=12566
SUMMARY:ARI Institute Colloquium: Robin Gopala Tress - Quick dynamical deco
 upling between gas and stars in galaxy centers
DTSTART:20260430T091500Z
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