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CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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UID:UW-Physics-Event-2167
DTSTART:20110412T170500Z
DURATION:PT1H0M0S
DTSTAMP:20260419T142836Z
LAST-MODIFIED:20110411T182318Z
LOCATION:4274 Chamberlin
SUMMARY:The Search for the Monsters at the Centers of Galaxies\, Chaos
  & Complex Systems Seminar\, Andy Sheinis\, UW Department of Astronomy
DESCRIPTION:The past decade has given rise to conclusive evidence that
  all galaxies harbor a super-massive black hole in their cores.  A bla
 ck hole is a massive body whose surface gravity is so great that light
  cannot escape its gravitational pull.  A growing understanding of the
  connection between galaxies and their central black holes has emerged
  that relates some of the properties of the black hole\, whose gravity
  influences only the central 1/10\,000 of the galaxy\, to the global p
 roperties of the entire galaxy.  Furthermore the latest galaxy formati
 on and evolution theories require the input of energy from the black h
 ole into the galaxy to achieve the size\, shape and number density of 
 the galaxies we observe today. These facts suggest that the growth mec
 hanisms of the black hole and galaxy must be connected. However\, deta
 ils of the physical processes behind this connection are not yet under
 stood. I will present an overview of the status of the field and then 
 discuss my research to understand the nature of some of the most massi
 ve of these objects that are in the process of consuming massive amoun
 ts of matter from their host galaxies. These objects are Quasi-Stellar
  Objects or QSO's\, which shine brightly in the sky due to the excess 
 gas that escapes their feeding process.<br>\n
URL:https://www.physics.wisc.edu/events/?id=2167
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