Abundances in very metal-poor stars

Ryan, Sean G. (2000) Abundances in very metal-poor stars. Institut d'Astrophysique et de Geophysique.

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Metal-poor stars provide information on the characteristics and chemical evolution of the halo population of the Galaxy, the first epoch of star formation and Galaxy formation (not just locally but with relevance to high-redshift objects),and big bang nucleosynthesis. This review looks at recent developments in this subject.

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Date Deposited	14 Nov 2024 10:46
Last Modified	14 Nov 2024 10:46

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