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The Evolution of the Oxygen Abundance in the Galaxy
Published online by Cambridge University Press: 30 March 2016
Abstract
We discuss the evolution of the [O/Fe] as a function of [Fe/H] in the Galaxy. In particular, we discuss the influence of different stellar yields as well as different SN (II, I) rates on the [O/Fe] ratio. Possible explanations for the steep rise of the [O/Fe] ratio at low metallicities, as indicated by recent observations, are critically discussed.
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- II. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2002