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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-3440
DTSTART:20141009T203000Z
DTEND:20141009T220000Z
DTSTAMP:20260309T175541Z
LAST-MODIFIED:20140908T132042Z
LOCATION:4421 Sterling Hall
SUMMARY:Puzzles in the Structure of Disk Galaxies\, Astronomy Colloqui
 um\, Stephane Courteau\, Queen's University
DESCRIPTION:Galaxies can be described in terms of their structure\, dy
 namics<br><br>\nand stellar populations.  Some very robust correlatio
 ns between<br><br>\nvarious galaxy structural properties\, such as to
 tal luminosity\,<br><br>\nmaximum circular velocity\, and size show r
 ather small scatter\,<br><br>\nhinting at well-regulated galaxy forma
 tion processes.  A major<br><br>\nchallenge to understanding these sc
 aling relations\, and ultimately<br><br>\ngalaxy formation and evolut
 ion\, is the elusive interplay between<br><br>\nvisible and dark matt
 er.  I will discuss the latest derivations<br><br>\nof galaxy scaling
  relations and their link with modern<br><br>\ncosmological models. 
URL:https://www.physics.wisc.edu/events/?id=3440
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