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J. A. Johnson (DAO/HIA/NRC), M. Bolte (UCO/Lick)
We present abundances in four stars with [Fe/H] < -3.0, derived from high-resolution spectra from HIRES/Keck. Elements from C to Ba are examined. We compare our results with the abundance patterns from other very metal-poor stars and with theoretical predictions for yields for zero-metallicity supernovae.
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.