A new approach to the solar oxygen abundance problem

Abstract

In this work we present new data that sets strong constraints on the solar oxygen abundance. Our approach, based on the analysis of spectro-polarimetric observations, is almost model-independent and therefore extremely robust. The asymmetry of the Stokes V profile of the 6300 A [OI] and NiI blend is used as an indicator of the relative abundances of these two elements. The peculiar shape of the profile requires a value of EO = 730+/-100 ppm (parts per million), or logEO = 8.86+/-0.07 in the logarithmic scale commonly used in Astrophysics. The uncertainty range includes the model dependence as well as uncertainties in the oscillator strengths of the lines. We emphasize that the very low degree of model dependence in our analysis makes it very reliable compared to traditional determinations.

Accepted for publication in The Astrophysical Journal Letters. 12 pages, 3 figures, referee format. This is the replacement of a previous version of the paper. Our revised analysis takes into consideration the formation of molecules, resulting in a substantially larger value for the derived Oxygen abundance

References in corpus (2)

• Helioseismology and Solar Abundances
• Solar Carbon Monoxide, Thermal Profiling, and the Abundances of C, O, and their Isotopes

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