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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20220120T103000
DTEND;TZID=Atlantic/Canary:20220120T113000
UID:iactalks-1535
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1535
CREATED:2022-01-20T10:30:00+00:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:The chemistry of the last major merger
DESCRIPTION:The chemistry of the last major merger\nDr. David S. Aguado\n\n
 One prediction of ΛCDM is the existence of partially phase-mixed su
 bstructures from accreted dwarf galaxies in the Milky Way stellar halo. Su
 bstructure originating in a single accretion event can be readily identifi
 ed as a tight cluster of stars in phase space with similar chemical proper
 ties. Recently, the discovery of the Gaia Sausage Enceladus (GSE) has revo
 lutionised our understanding of the complex assembly of the Milky Way halo
 . We present a review of the chemistry that characterises the last major m
 erger that happened to the Milky Way some 9-10 Gy ago.
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