Recent Advances in the Study of Extremely Metal-Poor Stars

Details Recent Advances in the Study of Extremely Metal-Poor Stars Recent Advances in the Study of Extremely Metal-Poor Stars

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf...80p&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

The advent of 8-10m class telescopes equipped with very efficient and high resolution spectrographs has strongly boosted the study of chemical patterns in the Galactic halo, allowing us to derive very accurate abundances in the most metal-poor stars. Here, the tremendous progress recently achieved in this field of research is presented and critically reviewed.

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