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PRODID:-//eluceo/ical//2.0/EN
VERSION:2.0
CALSCALE:GREGORIAN
BEGIN:VEVENT
UID:bc66ca7b03d69d4dbefd5e90afdad766
DTSTAMP:20261012T154940Z
SUMMARY:Chemical abundances as fossil records of dwarf galaxy evolution
DESCRIPTION:Contact: anastasiia.plotnikova@geol.lu.se\n\nAbstract: Dwarf ga
 laxies are excellent laboratories for studying galaxy evolution. They are 
 typically old and metal-poor systems\, with overall simpler evolutionary h
 istories than the Milky Way. Dwarf galaxies also played a central role in 
 the evolution of the Milky Way\, as there is evidence that several of them
  were accreted by our Galaxy over time. A powerful way to uncover the evol
 utionary history of dwarf galaxies is through their chemical abundance dis
 tributions. Different chemical elements are produced by distinct nucleosyn
 thetic channels and provide insights into the key physical processes that 
 shaped dwarf galaxies\, both those currently orbiting the Milky Way and th
 ose that were accreted onto it. In this talk\, I will present results on t
 he evolutionary histories of dwarf galaxies\, based on chemical abundances
  derived from high-resolution stellar spectra of one of the main building 
 blocks of the Milky Way\, Gaia-Sausage-Enceladus\, as well as on chemical 
 evolution models of several dwarf galaxies.\n\nMore information about the 
 event: https://www.lundobservatory.lu.se/calendar/chemical-abundances-foss
 il-records-dwarf-galaxy-evolution
DTSTART;TZID=GMT:20251126T121500
DTEND;TZID=GMT:20251126T133000
LOCATION:Geocentrum I\, Gotland (first floor\, on the right)
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