| dc.contributor.author | Ryan, Sean G. | |
| dc.contributor.author | Elliott, L. | |
| dc.contributor.editor | Pasquini, Luca | |
| dc.contributor.editor | Randich, Sofia | |
| dc.date.accessioned | 2012-04-30T12:00:11Z | |
| dc.date.available | 2012-04-30T12:00:11Z | |
| dc.date.issued | 2006 | |
| dc.identifier.citation | Ryan , 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 Nature Link , 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.citation | workshop | |
| dc.identifier.other | dspace: 2299/1763 | |
| dc.identifier.other | ORCID: /0000-0001-9069-5122/work/30501338 | |
| dc.identifier.uri | http://hdl.handle.net/2299/8437 | |
| dc.description.abstract | We 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.format.extent | 83791 | |
| dc.language.iso | eng | |
| dc.publisher | Springer Nature Link | |
| dc.relation.ispartof | Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites | |
| dc.title | The Halo Lithium Plateau : Outstanding Issues | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| rioxxterms.versionofrecord | 10.1007/978-3-540-34136-9_66 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
