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dc.contributor.authorRyan, Sean G.
dc.contributor.authorElliott, L.
dc.contributor.editorPasquini, Luca
dc.contributor.editorRandich, Sofia
dc.date.accessioned2012-04-30T12:00:11Z
dc.date.available2012-04-30T12:00:11Z
dc.date.issued2006
dc.identifier.citationRyan , S G & Elliott , L 2006 , The Halo Lithium Plateau : Outstanding Issues . in L Pasquini & S Randich (eds) , Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites : Procs of ESO Workshop . Springer , pp. 185-190 , ESO Workshop , Castiglione della Pescaia , Italy , 13/09/04 . https://doi.org/10.1007/978-3-540-34136-9_66
dc.identifier.citationworkshop
dc.identifier.otherPURE: 824711
dc.identifier.otherPURE UUID: 77dc5b60-64a5-4d14-b80b-3224345199a9
dc.identifier.otherdspace: 2299/1763
dc.identifier.otherScopus: 33749447164
dc.identifier.otherORCID: /0000-0001-9069-5122/work/30501338
dc.identifier.urihttp://hdl.handle.net/2299/8437
dc.description.abstractWe examine outstanding issues in the analysis and interpretation of the halo Li plateau. We show that the majority of very Li-poor halo Li-plateau stars (5 out of 8) have high projected rotation velocities vsini between 4.7 and 10.4 km s-1. Such stars have very different evolutionary histories to Li-normal plateau stars, and hence cannot be included in studies of Li depletion by normal halo dwarfs. Uncertainties in the effective temperature scale for metal-poor stars continue to challenge the analysis of Li.en
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofChemical Abundances and Mixing in Stars in the Milky Way and its Satellites
dc.rightsOpen
dc.titleThe Halo Lithium Plateau : Outstanding Issuesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Accepted Version
dcterms.dateAccepted2006
rioxxterms.versionAM
rioxxterms.versionofrecordhttps://doi.org/10.1007/978-3-540-34136-9_66
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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