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The chemical composition of the Sun

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dc.contributor.authorGrevesse, N
dc.contributor.authorAsplund, Martin
dc.contributor.authorSauval, A J
dc.contributor.authorScott, P
dc.date.accessioned2015-12-13T22:43:49Z
dc.date.issued2010
dc.date.updated2016-02-24T09:37:28Z
dc.description.abstractWe present a redetermination of the solar abundances of all available elements. The new results have very recently been published by Asplund et al. (Annu. Rev. Astron. Astrophys. 47:481, 2009). The basic ingredients of this work, the main results and some of their implications are summarized hereafter.
dc.identifier.issn0004-640X
dc.identifier.urihttp://hdl.handle.net/1885/79373
dc.publisherKluwer Academic Publishers
dc.sourceAstrophysics and Space Science
dc.subjectKeywords: Solar abundances
dc.titleThe chemical composition of the Sun
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage183
local.bibliographicCitation.startpage179
local.contributor.affiliationGrevesse, N, Universite de Liege
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSauval, A J, Observatoire Royal de Belgique
local.contributor.affiliationScott, P, University of Stockholm
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020109 - Space and Solar Physics
local.identifier.ariespublicationf5625xPUB7829
local.identifier.citationvolume328
local.identifier.doi10.1007/s10509-010-0288-z
local.identifier.scopusID2-s2.0-77955090083
local.type.statusPublished Version

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