Titlebook: Understanding the Enrichment of Heavy Elements by the Chemodynamical Evolution Models of Dwarf Galax; Yutaka Hirai Book 2019 Springer Natu

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,Enrichment of ,-Process Elements in?Isolated Dwarf Galaxies,n galaxies with higher star formation efficiencies. The star-to-star scatters of the ratios of .-process elements to iron mainly come from the inhomogeneous spatial metallicity distribution in galaxies. The results demonstrate that it will be possible to estimate the early star formation histories o

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Enrichment of ,-Process Elements in a Cosmological Context, early stages of galaxy formation. This result suggests that .-process rich stars seen in the Milky Way halo come from small size halos with the mass comparable to the Local Group ultra-faint dwarf galaxies.

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2190-5053 ory of the early galaxies, and presents theoretical findings that open new avenues to understanding the formation and evolution of galaxies based on the abundance of heavy elements in metal-poor stars..978-981-13-7884-3Series ISSN 2190-5053 Series E-ISSN 2190-5061

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