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PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-1590
DTSTART:20090929T203000Z
DTEND:20090929T220000Z
DTSTAMP:20260506T172217Z
LAST-MODIFIED:20090903T130326Z
LOCATION:3425 Sterling Hall
SUMMARY:Spatially-resolved studies of super star cluster feedback in S
 tarburst Galaxies\, Astronomy Colloquium\, Mark Westmoquette\, Univers
 ity College - London
DESCRIPTION:Understanding starburst-driven outflows is important for m
 any reasons  within the context of galaxy evolution. However\, to unde
 rstand outflows on the large scale\, the details of feedback mechanism
 s from individual star clusters must first be understood. In this talk
  I will discuss recent results from a number of high spatial and spect
 ral resolution optical integral field spectroscopic studies of the ion
 ized gas environment surrounding super star clusters (SSCs) within nea
 rby starbursts (e.g. NGC 1569\, M82\, NGC 1140). Through dynamical\, e
 xcitation and density measurements\, these studies are allowing us to 
 build up a picture of (1) how power is fed from these clusters into th
 e surrounding ISM\, and (2) how the ISM properties affect how this pow
 er is directed.
URL:https://www.physics.wisc.edu/events/?id=1590
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