Can Enhanced Diffusion Improve Helioseismic Agreement for Solar Models with Revised Abundances?

Recent solar photospheric abundance analyses (by Asplund et al. and Lodders) revise the C, N, O, Ne, and Ar abundances downward by 0.15-0.2 dex compared to previous determinations by Grevesse & Sauval. The abundances of Fe and other elements are reduced by smaller amounts, 0.05-0.1 dex. With the...

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Veröffentlicht in:	The Astrophysical journal 2005-07, Vol.627 (2), p.1049-1056
Hauptverfasser:	Guzik, Joyce A, Watson, L. Scott, Cox, Arthur N
Format:	Artikel
Sprache:	eng
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