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Oxygen lines in solar granulation: II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance

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Pereira, Tiago; Asplund, Martin; Kiselman, D

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Context: There is a lively debate about the solar oxygen abundance and the role of 3D models in its recent downward revision. These models have been tested using high-resolution solar atlases of flux and disk-centre intensity. Further testing can be done

dc.contributor.authorPereira, Tiago
dc.contributor.authorAsplund, Martin
dc.contributor.authorKiselman, D
dc.date.accessioned2015-12-08T22:46:07Z
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/38006
dc.description.abstractContext: There is a lively debate about the solar oxygen abundance and the role of 3D models in its recent downward revision. These models have been tested using high-resolution solar atlases of flux and disk-centre intensity. Further testing can be done
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: 1-D models; 3D modelling; 3D models; Abundance analysis; Convection - line: formation; Draw-in; High resolution; Inelastic collision; Line data; Line profiles; Oxygen line; Solar disk; Solar models; Solar surfaces; Sun: abundances; Sun: photosphere; Viewi Convection; Line: formation; Sun: abundances; Sun: granulation; Sun: photosphere
dc.titleOxygen lines in solar granulation: II. Centre-to-limb variation, NLTE line formation, blends, and the solar oxygen abundance
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume508
dc.date.issued2009
local.identifier.absfor020109 - Space and Solar Physics
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4326120xPUB156
local.identifier.ariespublicationu4630950xPUB102
local.type.statusPublished Version
local.contributor.affiliationPereira, Tiago, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAsplund, Martin, Max Planck Institute for Astrophysics
local.contributor.affiliationKiselman, D, Royal Swedish Academy of Sciences
local.description.embargo2037-12-31
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage1403
local.bibliographicCitation.lastpage1416
local.identifier.doi10.1051/0004-6361/200912840
dc.date.updated2016-02-24T10:55:14Z
local.identifier.scopusID2-s2.0-72849113796
CollectionsANU Research Publications

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