9.4k citations · 12.4k across the 19 of their papers we have counts for
19 papers
Helioseismic determination of the solar metal mass fraction
G. Buldgen, A. Noels, V. A. Baturin +5
Context. The metal mass fraction of the Sun Z is a key constraint in solar modelling, but its value is still under debate. The standard solar chemical composition of the late 2000s…
Higher metal abundances do not solve the solar problem
G. Buldgen, P. Eggenberger, A. Noels +4
Context. The Sun acts as a cornerstone of stellar physics. Thanks to spectroscopic, helioseismic and neutrino flux observations, we can use the Sun as a laboratory of fundamental p…
The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines
A. M. Amarsi, N. Grevesse, M. Asplund +1
Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. Their abundances remain hotly debated due to the so-called solar modelling problem…
The chemical make-up of the Sun: A 2020 vision
M. Asplund, A. M. Amarsi, N. Grevesse
The chemical composition of the Sun is a fundamental yardstick in astronomy, relative to which essentially all cosmic objects are referenced. We reassess the solar abundances of al…
The 3D non-LTE solar nitrogen abundance from atomic lines
A. M. Amarsi, N. Grevesse, J. Grumer +3
Nitrogen is an important element in various fields of stellar and Galactic astronomy, and the solar nitrogen abundance is crucial as a yardstick for comparing different objects in…
3D non-LTE line formation of neutral carbon in the Sun
A. M. Amarsi, P. S. Barklem, R. Collet +2
Carbon abundances in late-type stars are important in a variety of astrophysical contexts. However C i lines, one of the main abundance diagnostics, are sensitive to departures fro…