Abundances in very metal-poor stars

dc.contributor.author	Ryan, Sean G.
dc.date.accessioned	2008-03-06T17:29:43Z
dc.date.available	2008-03-06T17:29:43Z
dc.date.issued	2000
dc.identifier.citation	Ryan , 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.other	dspace: 2299/1771
dc.identifier.other	ORCID: /0000-0001-9069-5122/work/30501375
dc.identifier.uri	http://hdl.handle.net/2299/1771
dc.description.abstract	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.	en
dc.format.extent	321944
dc.language.iso	eng
dc.publisher	Institut d'Astrophysique et de Geophysique
dc.relation.ispartof	Procs of the 35th Liege International Astrophysics Colloquium
dc.title	Abundances in very metal-poor stars	en
dc.contributor.institution	Centre for Astrophysics Research (CAR)
dc.contributor.institution	School of Physics, Engineering & Computer Science
dc.contributor.institution	Department of Physics, Astronomy and Mathematics
rioxxterms.type	Other
herts.preservation.rarelyaccessed	true