Elemental abundances of models in Serenelli et al. (2009)
GS98[1]
(Z/X)PH=0.0229

AGS05[2]
(Z/X)PH=0.0165

AGSS09[3]
(Z/X)PH=0.0178

AGSS09ph[3]
(Z/X)PH=0.0181

C
8.52
0.06
8.39
0.05
8.43
0.05
8.43
0.05
N
7.92
0.06
7.78
0.06
7.83
0.06
7.83
0.06
O
8.83
0.06
8.66
0.05
8.69
0.05
8.69
0.05
Ne
8.08
0.06
7.84
0.06
7.93
0.06
7.93
0.06
Na
6.32
0.03
6.27
0.03
6.27
0.03
6.24
0.03
Mg
7.58
0.03
7.53
0.03
7.53
0.03
7.60
0.03
Al
6.49
0.03
6.43
0.03
6.43
0.03
6.45
0.03
Si
7.56
0.02
7.51
0.02
7.51
0.02
7.51
0.02
S
7.20
0.04
7.16
0.04
7.15
0.04
7.12
0.04
Ar
6.40
0.06
6.18
0.08
6.40
0.08
6.40
0.08
Ca
6.35
0.03
6.29
0.03
6.29
0.03
6.34
0.03
Cr
5.69
0.03
5.63
0.03
5.64
0.03
5.64
0.03
Mn
5.53
0.03
5.47
0.03
5.48
0.03
5.43
0.03
Fe
7.50
0.03
7.45
0.03
7.45
0.03
7.50
0.03
Ni
6.25
0.03
6.19
0.03
6.20
0.03
6.22
0.03

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.


References
  1. N. Grevesse & J. Sauval 1998, Space Sci. Rev., 85, 161
  2. M. Asplund, N. Grevesse & J. Sauval 2005, Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, 336, 25
  3. M. Asplund, N. Grevesse, J. Sauval & P. Scott, ARAA, 47. 567