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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-3865
DTSTART:20151203T213000Z
DTEND:20151203T230000Z
DTSTAMP:20260419T110434Z
LAST-MODIFIED:20161104T130639Z
LOCATION:4421 Sterling Hall\, Talk starts at 3:45 PM
SUMMARY:Star Formation in HI Dominated Environments \, Astronomy Collo
 quium\, Jennifer Donovan Meyer\, NRAO
DESCRIPTION:I will discuss recent work on star forming\, HI-dominated 
 environments from nearby\, low-mass dwarf galaxies to extended ultravi
 olet (XUV) disks. In both cases\, stars are forming at low levels -- r
 equiring interstellar media capable of doing so -- but the gas columns
  and molecular fractions in these regions can differ substantially fro
 m those in the main disks of normal\, star forming galaxies. I'll pres
 ent some ongoing studies of the gas available for stars to form in the
 se very different environments and discuss their broader context by co
 mparing to more typically studied star forming gas. Finally\, I will a
 ddress the evolutionary context of these environments\, as they are gr
 eat examples of the ways in which atomic gas affects the ongoing evolu
 tion of galaxies of all sizes. 
URL:https://www.physics.wisc.edu/events/?id=3865
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