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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-1362
DTSTART:20081125T213000Z
DURATION:PT1H0M0S
DTSTAMP:20260415T130202Z
LAST-MODIFIED:20081124T194706Z
LOCATION:6515 Sterling Hall
SUMMARY:Fueling Galaxies at z = 0\, Astronomy Colloquium\, Mary Putnam
 \, Columbia University
DESCRIPTION:Spiral galaxies are thought to have a source of incoming s
 tar formation fuel through the majority of their lifetimes.  This fuel
  source includes satellite galaxies captured by the galaxy and possibl
 y clouds condensing within the galaxies extended hot gaseous halo.   S
 ome galaxies may also be fueling themselves by transferring gas from t
 he outer regions to the inner star forming disk.  The evidence for var
 ious fueling mechanisms and the future fueling prospects for the galax
 ies of the Local Group will be discussed. 
URL:https://www.physics.wisc.edu/events/?id=1362
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