Why GN93 should not be used anymore

Why GN93 should not be used anymore

We 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 should be replaced by the new and more precise r...

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Main Authors: Sauval J., Asplund M., Grevesse N., Scott P.
Format: Article
Language:English
Published: EDP Sciences 2013-03-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20134301004
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spelling doaj-68807d375ec74769b890f9d04882d8862021-08-02T17:31:31ZengEDP SciencesEPJ Web of Conferences2100-014X2013-03-01430100410.1051/epjconf/20134301004Why GN93 should not be used anymoreSauval J.Asplund M.Grevesse N.Scott P.We 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 should be replaced by the new and more precise results of [4] (AGSS09), with a much lower metallicity of 0.0134. http://dx.doi.org/10.1051/epjconf/20134301004
collection DOAJ
language English
format Article
sources DOAJ
author Sauval J.
Asplund M.
Grevesse N.
Scott P.
spellingShingle Sauval J.
Asplund M.
Grevesse N.
Scott P.
Why GN93 should not be used anymore
EPJ Web of Conferences
author_facet Sauval J.
Asplund M.
Grevesse N.
Scott P.
author_sort Sauval J.
title Why GN93 should not be used anymore
title_short Why GN93 should not be used anymore
title_full Why GN93 should not be used anymore
title_fullStr Why GN93 should not be used anymore
title_full_unstemmed Why GN93 should not be used anymore
title_sort why gn93 should not be used anymore
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2013-03-01
description We 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 should be replaced by the new and more precise results of [4] (AGSS09), with a much lower metallicity of 0.0134.
url http://dx.doi.org/10.1051/epjconf/20134301004
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AT grevessen whygn93shouldnotbeusedanymore
AT scottp whygn93shouldnotbeusedanymore
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