Elemental abundances of models in Serenelli et al. (2009) | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Abundances and uncertainties are given in units of ε(X)= log10 (NX/NH) + 12 * Only elements needed for opacity calculations are included in the table. Full list of abundances are given in the original references [1,2,3]. ** AGSS09ph is formed only with photospheric abundances. Other composition adopt meteoritic values for refractories, assuming Si abundance ratio is the same both in the photospheric and meteoritic scales. |
Non composition parameters are as in BPS08 and can be found here.