Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, and detailed treatment of blends have resulted in a significant downward revision of the solar oxygen abundance. Aims. Considering the importance of the Su
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. The...
Context. There is a lively debate about the solar oxygen abundance and the role of 3D models in its ...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
Context. The solar photospheric abundance of oxygen is still a matter of debate. For about ten years...
The forbidden O I lines at λλ5577, 6300, and 6363 appear as faint absorption lines in the solar spec...
We reexamine closely the solar photospheric line at 6300 A, which is attributed to a forbidden line ...
In this work we present support for recent claims that advocate a downward revision of the solar oxy...
We reexamine closely the solar photospheric line at 6300 A° , which is attributed to a forbidden lin...
The oxygen abundance in the solar photosphere, and consequently the solar metallicity itself, is sti...
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation a...
International audienceContext: The solar oxygen abundance has undergone a major downward revision in...
In this work we not only support recent disquieting claims that advocate a downward revision of the ...
International audienceContext. In the Sun, the two forbidden [O i] lines at 630 and 636 nm were prev...
Context.Sulphur is an element which is formed in the α-process and is easily measured in the gaseous...
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. The...
Context. There is a lively debate about the solar oxygen abundance and the role of 3D models in its ...
Context. Recent works with improved model atmospheres, line formation, atomic and molecular data, an...
Context. The solar photospheric abundance of oxygen is still a matter of debate. For about ten years...
The forbidden O I lines at λλ5577, 6300, and 6363 appear as faint absorption lines in the solar spec...
We reexamine closely the solar photospheric line at 6300 A, which is attributed to a forbidden line ...
In this work we present support for recent claims that advocate a downward revision of the solar oxy...
We reexamine closely the solar photospheric line at 6300 A° , which is attributed to a forbidden lin...
The oxygen abundance in the solar photosphere, and consequently the solar metallicity itself, is sti...
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation a...
International audienceContext: The solar oxygen abundance has undergone a major downward revision in...
In this work we not only support recent disquieting claims that advocate a downward revision of the ...
International audienceContext. In the Sun, the two forbidden [O i] lines at 630 and 636 nm were prev...
Context.Sulphur is an element which is formed in the α-process and is easily measured in the gaseous...
Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of th...
Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. The...
Context. There is a lively debate about the solar oxygen abundance and the role of 3D models in its ...
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