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Oxygen Abundances: New Results from [O I] Lines
Published online by Cambridge University Press: 30 March 2016
Abstract
From new high resolution spectra of metal-poor giants we use equivalent widths of [O I], Sc II, and Fe II lines to derive new values of [O/Sc] and [O/Fe]. These results are generally consistent with previous determinations of oxygen abundances from [O I] lines, but the star-to-star scatter is greatly reduced.
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- Copyright © Astronomical Society of Pacific 2002
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