Articles citing this article

The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).

Cited article:

Population II stars and the Spite plateau - Stellar evolution models with mass loss

M. Vick, G. Michaud, J. Richer, O. Richard

A&A, 552 (2013) A131

Published online: 2013-04-16

DOI: https://doi.org/10.1051/0004-6361/201220726

This article has been cited by the following article(s):

Atomic diffusion and mixing in old stars

P. Gruyters, A. J. Korn, O. Richard, et al.
Astronomy & Astrophysics 555 A31 (2013)
DOI: 10.1051/0004-6361/201220821
See this article

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)
DOI: 10.1007/s12036-017-9481-6
See this article

Atomic Diffusion in Stars

Georges Michaud, Georges Alecian and Jacques Richer
Astronomy and Astrophysics Library, Atomic Diffusion in Stars 189 (2015)
DOI: 10.1007/978-3-319-19854-5_10
See this article

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)
DOI: 10.1051/eas/1363039
See this article

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)
DOI: 10.3847/1538-4357/aa6d10
See this article

Chemical element transport in stellar evolution models

Maurizio Salaris and Santi Cassisi
Royal Society Open Science 4 (8) 170192 (2017)
DOI: 10.1098/rsos.170192
See this article

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)
DOI: 10.1051/0004-6361/202038833
See this article