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CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
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SEQUENCE:0
UID:UW-Physics-Event-4269
DTSTART:20160922T203000Z
DTEND:20160922T220000Z
DTSTAMP:20260419T060510Z
LAST-MODIFIED:20160830T170627Z
LOCATION:4421 Sterling Hall\, Coffee and Cookies at 3:30 PM \, Talk at
  3:45 PM
SUMMARY:Low Mass Galaxies and their Gas at the Peak Epoch of Star Form
 ation\, Astronomy Colloquium\, Dawn Erb\, UW Milwaukee
DESCRIPTION:Because faint\, low mass galaxies are numerous at high red
 shifts\, their impact on the Universe is expected to be significant. T
 hey may host a substantial fraction of the Universe's star formation\,
  provide many of the energetic photons needed to reionize the intergal
 actic medium\, and affect their surroundings via powerful\, starburst-
 driven galactic outflows. Because of their faintness\, however\, the p
 roperties of these galaxies are difficult to determine. I will discuss
  a variety of observations aimed at characterizing the physical condit
 ions in low mass galaxies during the peak epoch of star formation\, wh
 en the Universe was ~20% of its current age\, with particular emphasis
  on the study of galactic outflows in faint galaxies.
URL:https://www.physics.wisc.edu/events/?id=4269
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