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dc.contributor.authorRyan, Sean G.
dc.date.accessioned2008-03-06T17:29:43Z
dc.date.available2008-03-06T17:29:43Z
dc.date.issued2000
dc.identifier.citationRyan , S 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 , pp. 101- .
dc.identifier.otherPURE: 148576
dc.identifier.otherPURE UUID: e4c8b81b-4225-4cee-97c5-d568c5409e37
dc.identifier.otherdspace: 2299/1771
dc.identifier.otherScopus: 0034394908
dc.identifier.otherORCID: /0000-0001-9069-5122/work/30501375
dc.identifier.urihttp://hdl.handle.net/2299/1771
dc.description.abstractMetal-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.en
dc.language.isoeng
dc.publisherInstitut d'Astrophysique et de Geophysique
dc.relation.ispartofProcs of the 35th Liege International Astrophysics Colloquium
dc.titleAbundances in very metal-poor starsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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