The chemical composition of the Sun

@article{Grevesse2009TheCC,
  title={The chemical composition of the Sun},
  author={Nicolas Grevesse and Martin Asplund and A. Jacques Sauval and Penny Scott},
  journal={Astrophysics and Space Science},
  year={2009},
  volume={328},
  pages={179-183}
}
We present a redetermination of the solar abundances of all available elements. The new results have very recently been published by Asplund et al. (Annu. Rev. Astron. Astrophys. 47:481, 2009). The basic ingredients of this work, the main results and some of their implications are summarized hereafter. 
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References

SHOWING 1-10 OF 488 REFERENCES
Standard Solar Composition
We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic
The chemical composition of the sun.
The discussion of the chemical composition of the sun includes the basic methods of analysis, a table of solar elemental abundances, and the particularly difficult problems of the abundances of
The solar lithium abundance
A detailed observational study of the solar photospheric lithium feature has been carried out with emphasis on center-limb observations, continuum location, possible effects of telluric lines,
Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in honor of David L. Lambert
We review our current knowledge of the solar chemical composition as determined from photospheric absorption lines. In particular we describe the recent significant revisions of the solar abundances
The Discrepancy between Solar Abundances and Helioseismology
There have been recent downward revisions of the solar photospheric abundances of oxygen and other heavy elements. These revised abundances along with OPAL opacities are not consistent with seismic
What Is the Neon Abundance of the Sun?
We have evolved a series of 13 complete solar models that utilize different assumed heavy-element compositions. Models that are based upon the heavy-element abundances recently determined by Asplund
Atomic data and solar and stellar spectroscopy
Solar photospheric abundances, which are generally used as references for other stars, are now, on the whole, in very good agreement with the meteoritic abundances. This is not due to progress in
Solar and Galactic Composition
This is a personal overview of our joint SOHO/ACE workshop “Solar and Galactic Composition” held in Bern, Switzerland, between the 6th to the 9th of March, 2001. The overview is not complete,
New results on standard solar models
We describe the current status of solar modeling and focus on the problems originating with the introduction of solar abundance determinations with low CNO abundance values. We use models computed
...
...