This is a talk held during the regular colloquium series (usually Tuesdays at 4pm).

The Star Formation in Radio Survey (SFRS): Initial Results from the GBT

Tuesday, January 17, 2012 - 1:00pm
Dr. Eric Murphy (Carnegie Observatories)

High frequency (~10-100 GHz) radio emission from galaxies offers one of the best means to quantify current star formation activity.  At these frequencies, emission is generally optically thin and dominated by free-free radiation, which is directly proportional to the ionizing photon rate of young


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