BEGIN:VCALENDAR
VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:1
UID:UW-Physics-Event-4801
DTSTART:20180419T203000Z
DTEND:20180419T220000Z
DTSTAMP:20260419T002324Z
LAST-MODIFIED:20180409T170601Z
LOCATION:4421 Sterling Hall\, Cookies and Coffee 3:30 PM\, Talk begins
  at 4:00 PM
SUMMARY:The Atomic to Molecular (HI-to-H2) Transition in Galaxy Star-F
 orming Regions\, Astronomy Colloquium\, Dr. Amiel Sternberg\, Tel Aviv
  University\, Max Planck Inst. for Extraterrestrial Physics\, Germany\
 , Flatiron Institute\, Simons Foundation USA
DESCRIPTION:The atomic to molecular hydrogen (HI-to-H2) phase transiti
 on is of fundamental importance for star-formation and the emergence o
 f chemical complexity in the interstellar medium of galaxies.  I will 
 present an overview\, and discuss recent theoretical studies\, numeric
 al and analytic\, of the HI-to-H2 transition in irradiated systems\, w
 ith applications to the multi-scale behavior observed in star-forming 
 galaxy disks from low- to high-redshift.
URL:https://www.physics.wisc.edu/events/?id=4801
END:VEVENT
END:VCALENDAR