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The Prevalence and Properties of Outflowing Galactic Winds at z = 1

The Prevalence and Properties of Outflowing Galactic Winds at z = 1. Katherine A. Kornei (UCLA) Alice E. Shapley (UCLA) Crystal L. Martin (UCSB) Alison L. Coil (UCSD). Berkeley Star Formation Seminar - October 31 , 2011. Galaxies are not closed boxes. outflows?. outflows?. IGM.

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Mgii feature - PowerPoint PPT Presentation

The Prevalence and Properties of Outflowing Galactic Winds at z = 1