The Physics of High Redshift Galaxies: Star Formation, Chemistry and Gas Flows

Details The Physics of High Redshift Galaxies: Star Formation, Chemistry and Gas Flows The Physics of High Redshift Galaxies: Star Formation, Chemistry and Gas Flows

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sptz.prop..473e&link_type=abstract

Spitzer Proposal ID #473

Physics

Scientific paper

I will use rest-frame UV and optical spectra, models of chemical evolution and star formation, and stellar mass and age determinations from ground-based and Spitzer photometry to constrain the properties of galaxies at z~2-3, the peak era of star formation and black hole accretion in the universe. I will focus on understanding the youngest and lowest mass galaxies, and on refining measurements of chemical abundances and using them to constrain the magnitudes of galactic inflows and outflows.

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