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SUMMARY:The chemistry of the last major merger - David Aguado\, Universit
 à degli Studi di Firenze
DTSTART:20220302T134500Z
DTEND:20220302T141500Z
UID:TALK170915@talks.cam.ac.uk
CONTACT:Francisco Paz-C
DESCRIPTION:One prediction of ΛCDM is the existence of partially phase-mi
 xed substructures from accreted dwarf galaxies in the Milky Way stellar ha
 lo. Recently\, the discovery of the Gaia Sausage Enceladus (GSE) has revol
 utionised our understanding of the complex assembly of the Milky Way halo.
  We present a review of the chemistry that characterises the last major me
 rger that happened to the Milky Way some 9-10 Gy ago.
LOCATION:The Hoyle Lecture Theatre + Zoom 
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