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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-3151
DTSTART:20131121T213000Z
DTEND:20131121T230000Z
DTSTAMP:20240329T052724Z
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
\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
\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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