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Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S

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dc.contributor.authorBensby, T
dc.contributor.authorAsplund, Martin
dc.contributor.authorJohnson, Jennifer A
dc.contributor.authorFeltzing, Sofia
dc.contributor.authorMelendez, Jorge
dc.contributor.authorDong, S
dc.contributor.authorGould, A
dc.contributor.authorHan, C
dc.contributor.authorAden, Daniel
dc.contributor.authorLucatello, Sara
dc.contributor.authorGal-Yam, Avishay
dc.date.accessioned2015-12-13T22:44:54Z
dc.date.issued2010
dc.date.updated2016-02-24T09:38:17Z
dc.description.abstractContext. To study the evolution of Li in the Galaxy it is necessary to observe dwarf or subgiant stars. These are the only long-lived stars whose present-day atmospheric chemical composition reflects their natal Li abundances according to standard models
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/79518
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Chemical compositions; Chemical evolution; Dwarf stars; Elemental abundance; Galactic bulge; Galactic disks; Galaxy: bulge; Galaxy: formation - Galaxy: evolution; Gravitational lensing; High resolution; Line profiles; Metallicities; Micro-lensing; Old age Galaxy: bulge; Galaxy: formation - Galaxy: evolution; gravitational lensing: micro; stars: abundances
dc.titleChemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars: III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S
dc.typeJournal article
local.bibliographicCitation.issue5
local.bibliographicCitation.startpageL57
local.contributor.affiliationBensby, T, European Southern Observatory
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationJohnson, Jennifer A, Ohio State University
local.contributor.affiliationFeltzing, Sofia, Lund Observatory
local.contributor.affiliationMelendez, Jorge, University of Sao Paulo
local.contributor.affiliationDong, S, Institute for Advanced Study
local.contributor.affiliationGould, A, Ohio State University
local.contributor.affiliationHan, C, Chungbuk National University
local.contributor.affiliationAden, Daniel, Lund Observatory
local.contributor.affiliationLucatello, Sara, INAF, Osservatorio Astronomico di Padova
local.contributor.affiliationGal-Yam, Avishay, Weizmann Institute of Science
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB7943
local.identifier.citationvolume521
local.identifier.doi10.1051/0004-6361/201015745
local.identifier.scopusID2-s2.0-77958131717
local.identifier.thomsonID000284150900057
local.type.statusPublished Version

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