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Primeval oxygen overabundance and type I-1/2 supernovae
Published online by Cambridge University Press: 04 August 2017
Abstract
Models of chemical evolution of the Galaxy have been computed by taking into account the different roles played by TypeI-1/2 (single stars suffering degenerate C-ignition) and Typell supernovae in the chemical enrichment. The overabundance of oxygen observed in the Halo stellar population has been well reproduced.
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- IV. RELATION WITH CHEMICAL EVOLUTION OF GALAXIES AND COSMOLOGY
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- Copyright © Reidel 1984