Context. The solar photospheric abundance of oxygen is still a matter of debate. For about ten years some determinations have favoured a low oxygen abundance which is at variance with the value inferred by helioseismology. Among the oxygen abundance indicators, the forbidden line at 630 nm has often been considered the most reliable even though it is blended with a Ni
The forbidden O I lines at λλ5577, 6300, and 6363 appear as faint absorption lines in the solar spec...
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Determinations of the solar oxygen content relying on the neutral forbidden transition at 630 nm dep...
Context. The solar photospheric oxygen abundance is still widely debated. Adopting the solar chemica...
International audienceContext. In the Sun, the two forbidden [O i] lines at 630 and 636 nm were prev...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
The oxygen abundance in the solar photosphere, and consequently the solar metallicity itself, is sti...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
We reexamine closely the solar photospheric line at 6300 A, which is attributed to a forbidden line ...
Aims. The purpose of this work is to better understand the confidence limits of the photospheric sol...
We reexamine closely the solar photospheric line at 6300 A° , which is attributed to a forbidden lin...
International audienceIn recent years the photospheric solar oxygen abundance experienced a signific...
In this work we present support for recent claims that advocate a downward revision of the solar oxy...
International audienceContext: The solar oxygen abundance has undergone a major downward revision in...
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation a...
The forbidden O I lines at λλ5577, 6300, and 6363 appear as faint absorption lines in the solar spec...
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Determinations of the solar oxygen content relying on the neutral forbidden transition at 630 nm dep...
Context. The solar photospheric oxygen abundance is still widely debated. Adopting the solar chemica...
International audienceContext. In the Sun, the two forbidden [O i] lines at 630 and 636 nm were prev...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
The oxygen abundance in the solar photosphere, and consequently the solar metallicity itself, is sti...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
We reexamine closely the solar photospheric line at 6300 A, which is attributed to a forbidden line ...
Aims. The purpose of this work is to better understand the confidence limits of the photospheric sol...
We reexamine closely the solar photospheric line at 6300 A° , which is attributed to a forbidden lin...
International audienceIn recent years the photospheric solar oxygen abundance experienced a signific...
In this work we present support for recent claims that advocate a downward revision of the solar oxy...
International audienceContext: The solar oxygen abundance has undergone a major downward revision in...
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation a...
The forbidden O I lines at λλ5577, 6300, and 6363 appear as faint absorption lines in the solar spec...
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Determinations of the solar oxygen content relying on the neutral forbidden transition at 630 nm dep...