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Chemical evolution of the Galactic halo and the Origin of Precious Metals
Published online by Cambridge University Press: 23 December 2005
Abstract
Observed large scatters in abundances of neutron-capture elements in metal-poor stars may suggest incomplete mixing of the interstellar medium at the beginning of the Galaxy. Comparing predictions by an inhomogeneous chemical evolution model and new observational results with Subaru HDS, we attempt to constrain the origins of r-process elements.
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- © 2005 International Astronomical Union