Abundances in very metal-poor stars

Ryan, Sean G. (2000) Abundances in very metal-poor stars. In: Procs of the 35th Liege International Astrophysics Colloquium : The Galactic Halo : From Globular Cluster to Field Stars. Institut d'Astrophysique et de Geophysique, 101-.

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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.

Item Type	Book Section
Date Deposited	15 May 2025 16:19
Last Modified	30 May 2025 23:09

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Ryan, Sean G.

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