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Why GN93 should not be used anymore

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dc.contributor.authorGrevesse, N
dc.contributor.authorAsplund, Martin
dc.contributor.authorSauval, J
dc.contributor.authorScott, Pat
dc.date.accessioned2015-12-13T23:01:01Z
dc.date.issued2013
dc.date.updated2015-12-12T07:37:18Z
dc.description.abstractWe show why the solar chemical composition of [1] (GN93) and the similar values of [2] (AG89) and [3] (GS98), characterized by values of the metallicity of the order of 0.017 to 0.020, largely used in solar and stellar modeling, are now obsolete. They sho
dc.identifier.issn2100-014X
dc.identifier.urihttp://hdl.handle.net/1885/84400
dc.publisherE D P Sciences
dc.sourceEPJ Web of Conferences
dc.titleWhy GN93 should not be used anymore
dc.typeJournal article
local.bibliographicCitation.lastpagep.3)
local.bibliographicCitation.startpage01004 (p.1
local.contributor.affiliationGrevesse, N, Universite de Liege
local.contributor.affiliationAsplund, Martin, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSauval, J, Observatoire Royal de Belgique
local.contributor.affiliationScott, Pat, McGill University
local.contributor.authoruidAsplund, Martin, u4042723
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB12674
local.identifier.citationvolume43
local.identifier.doi10.1051/epjconf/20134301004
local.identifier.scopusID2-s2.0-84875680579
local.identifier.thomsonID000320548900004
local.type.statusPublished Version

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