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SUMMARY:Probing the early history of the Milky Way through ancient carbon-
 rich stars - Anke Ardern-Arentsen / IoA
DTSTART:20250219T134000Z
DTEND:20250219T140500Z
UID:TALK228481@talks.cam.ac.uk
CONTACT:Xander Byrne
DESCRIPTION:The oldest\, most metal-poor stars we find in the Milky Way to
 day were born in pristine environments in the early Universe. These local\
 , ancient stars contain unique clues about the First Stars and the early f
 ormation and evolution of our Galaxy. At low metallicity\, many stars have
  been found to be enhanced in carbon\, coming in two main types: some cont
 ain the fingerprints of the First Stars and others have experienced binary
  interaction with an evolved companion. I recently built a homogeneous sam
 ple of C-rich metal-poor stars using the Gaia XP spectra\, employing a neu
 ral network and a dedicated training sample. I will present this recent pa
 per and discuss how the change in frequency of C-rich stars with Galactic 
 environment relates to globular clusters and clustered star formation in t
 he early Universe. 
LOCATION:The Hoyle Lecture Theatre + Zoom 
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