Measuring the Metallicity of the High Redshift IGM: Traces of Early Stellar Feedback

Details Measuring the Metallicity of the High Redshift IGM: Traces of Early Stellar Feedback Measuring the Metallicity of the High Redshift IGM: Traces of Early Stellar Feedback

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.3406s&link_type=abstract

American Astronomical Society Meeting 204, #34.06; Bulletin of the American Astronomical Society, Vol. 36, p.704

Astronomy and Astrophysics

Astronomy

Scientific paper

By z 3, a substantial portion of the universe was already populated with heavy elements produced in stars. Observations of these intergalactic metals can be used to characterize early star formation and feedback on cosmic scales. I will summarize the latest progress in cosmic metallicity field measurements, with special attention to what these data reveal about the early stars and galaxies that were the primary agents of chemical enrichment.

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