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Cited article:

Atomic diffusion and mixing in old stars – VIII. Chemical abundance variations in the globular cluster M4 (NGC 6121)

T Nordlander, P Gruyters, O Richard and A J Korn
Monthly Notices of the Royal Astronomical Society 527 (4) 12120 (2023)

Discovery of a thin lithium plateau among metal-poor red giant branch stars

A. Mucciarelli, L. Monaco, P. Bonifacio, M. Salaris, M. Deal, M. Spite, O. A. Richard and R. Lallement
Astronomy & Astrophysics 661 A153 (2022)

Matter accretion in metal-poor stars down to extremely metal-poor stars and the lithium problem

M. Deal, O. Richard and S. Vauclair
Astronomy & Astrophysics 646 A160 (2021)

The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing are at the origin of chemical abundance variations

Ekaterina Semenova, Maria Bergemann, Morgan Deal, et al.
Astronomy & Astrophysics 643 A164 (2020)

The Influence of Atomic Diffusion on Stellar Ages and Chemical Tagging

Aaron Dotter, Charlie Conroy, Phillip Cargile and Martin Asplund
The Astrophysical Journal 840 (2) 99 (2017)

Contribution of Proton Capture Reactions to the Ascertained Abundance of Fluorine in the Evolved Stars of Globular Cluster M4, M22, 47 Tuc and NGC 6397

Upakul Mahanta, Aruna Goswami, H. L. Duorah and K. Duorah
Journal of Astrophysics and Astronomy 38 (4) (2017)

Stellar evolution including diffusion and matter flow induced by mass-loss

O. Richard, M. Vick, G. Alecian, et al.
EAS Publications Series 63 349 (2013)