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METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20220421T103000
DTEND;TZID=Atlantic/Canary:20220421T113000
UID:iactalks-1543
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1543
CREATED:2022-04-21T10:30:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:The formation of Milky Way-mass galactic disc structure in cosmolog
 ical simulations
DESCRIPTION:The formation of Milky Way-mass galactic disc structure in cosm
 ological simulations\nDr. Robert Grand\n\nRecent years have seen impressiv
 e development in cosmological simulations for spiral disc galaxies like th
 e Milky Way. I present a suite of high-resolution magneto-hydrodynamic sim
 ulations that include many physical processes relevant for galaxy formatio
 n, including star formation, stellar evolution and feedback, active galact
 ic nuclei and magnetic fields. I will discuss how these processes affect t
 he formation of galactic discs, and what these simulations can tell us abo
 ut the formation of the Milky Way, such as the properties of the Galaxy's 
 putative last significant merger and its effect on the formation of the th
 ick disc and stellar halo.&nbsp;
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