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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-3663
DTSTART:20150319T203000Z
DTEND:20150319T220000Z
DTSTAMP:20260419T142538Z
LAST-MODIFIED:20150216T142454Z
LOCATION:4421 Sterling Hall
SUMMARY:What drives the evolution of the Milky Way’s disk?\, Astrono
 my Colloquium\, Jo Bovy\, Institute for Advanced Study
DESCRIPTION:Observations of the structure and dynamics of different st
 ellar populations in the Milky Way's disk provide a unique perspective
  on disk formation\, evolution\, and dynamics. I will review our curre
 nt knowledge of the chemo-orbital structure of the disk. I will then d
 iscuss new measurements of the kinematics and chemistry of intermediat
 e-age stars over a large part of the Galactic disk from the APOGEE sur
 vey and the new insights these measurements provide about the formatio
 n and evolution of the disk.
URL:https://www.physics.wisc.edu/events/?id=3663
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END:VCALENDAR