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The lithium isotopic ratio in very metal-poor stars

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dc.contributor.authorLind, Karin
dc.contributor.authorMelendez, Jorge
dc.contributor.authorAsplund, Martin
dc.contributor.authorCollet, Remo
dc.contributor.authorMagic, Zazralt
dc.date.accessioned2015-12-13T22:24:55Z
dc.date.issued2013
dc.date.updated2016-02-24T09:12:51Z
dc.description.abstractContext. Un-evolved, very metal-poor stars are the most important tracers of the cosmic abundance of lithium in the early universe. Combining the standard Big Bang nucleosynthesis model with Galactic production through cosmic ray spallation, these stars a
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/72987
dc.publisherSpringer
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Line: formation; Line: Profiles; Primordial nucleosynthesis; Stars: abundances; Stars: Population II; Techniques: spectroscopic; Calcium; Hydrogen bonds; Isotopes; Lithium; Nucleosynthesis; Sodium; Three dimensional; Three dimensional computer graphics; S Line: formation; Line: profiles; Primordial nucleosynthesis; Stars: abundances; Stars: Population II; Techniques: spectroscopic
dc.titleThe lithium isotopic ratio in very metal-poor stars
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issueA96
local.bibliographicCitation.lastpage15
local.bibliographicCitation.startpage1
local.contributor.affiliationLind, Karin, Max Planck Institut fur Astrophysik
local.contributor.affiliationMelendez, Jorge, University of Sao Paulo
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationCollet, Remo, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMagic, Zazralt, Max-Planck-Institut für Astrophysik
local.contributor.authoruidAsplund, Martin, u4042723
local.contributor.authoruidCollet, Remo, u5236916
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB3512
local.identifier.citationvolume554
local.identifier.doi10.1051/0004-6361/201321406
local.identifier.scopusID2-s2.0-84878897768
local.identifier.thomsonID000320444200095
local.type.statusPublished Version

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