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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-3151
DTSTART:20131121T213000Z
DTEND:20131121T230000Z
DTSTAMP:20260419T211736Z
LAST-MODIFIED:20131022T132401Z
LOCATION:4421 Sterling Hall
SUMMARY:Constraining the Physics of Star Formation in Galaxies Using t
 he JVLA and GBT\, Astronomy Colloquium\, Amanda Kepley\, NRAO
DESCRIPTION:Understanding how galaxies evolve requires understanding t
 he properties of the young massive stars that mediate their structure 
 and evolution and understanding the conditions under which these stars
  form.  The latest generation of radio and <br>
\nsubmillimeter telesc
 opes are revolutionizing our ability to probe both the young massive s
 tars and the dense molecular gas out of which they form. In this talk\
 , I will present observations from the JVLA and GBT that demonstrate t
 he capabilities of these telescopes and how they can tell us about the
  properties <br>
\nof the dense gas ionized by the young  massive star
 s in the center of a galaxy much like our own and the properties of th
 e dense molecular gas in a starburst environment.
URL:https://www.physics.wisc.edu/events/?id=3151
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