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SUMMARY:Galactic Archaeology with Globular Clusters - Stephanie Monty (IoA
 )
DTSTART:20240112T113000Z
DTEND:20240112T123000Z
UID:TALK207511@talks.cam.ac.uk
CONTACT:Sandro Tacchella
DESCRIPTION:Globular clusters (GCs) are among the most ancient objects in 
 the local Universe\, acting as tracers of galaxy formation across both spa
 ce and time. With the recent JWST discovery of nitrogen-rich star formatio
 n in a redshift 11 galaxy\, and the discovery that over 50% of the in-situ
  stars in the Milky Way (MW) likely formed in clusters\, understanding the
  role of GCs in the context of galaxy evolution is becoming ever more impo
 rtant. The MW hosts a large (~150) and diverse population of GCs. Among th
 ese clusters\, a fraction are thought to have formed in-situ\, alongside t
 he MW\, while others were likely accreted alongside disrupted dwarf galaxi
 es. A small number of MW GCs may themselves be the sole remaining remnants
  of disrupted dwarf galaxies as stripped nuclear star clusters. In this ta
 lk I will discuss ongoing work to identify the origins of accreted GCs\, h
 ighlighting the strength of combining high resolution chemical abundances 
 with dedicated dynamical simulations. I will present results for populatio
 ns of accreted GCs as well as individuals\, presenting initial results as 
 to the origins of the MW’s two most enigmatic GCs\, NGC 2419 and M 22.
LOCATION:Ryle seminar room + online
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