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Galactic and cosmic chemical evolution with hypernovae
Published online by Cambridge University Press: 23 December 2005
Abstract
We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the G-dwarf problem. We finally show the cosmological simulation and discuss the galaxy formation and chemical enrichment.
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- © 2005 International Astronomical Union