Corrigendum: On the nature of the core of $\alpha$ Centauri A: the impact of the metallicity mixture
- 1Centre for Astrophysics, Faculty of Sciences, University of Porto, Portugal
- 2Instituto de Astrofísica e Ciências do Espaço, University of Porto, Portugal
- 3Departamento de Física e Astronomia, Faculty of Sciences, University of Porto, Portugal
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Keywords: HD 128620, Asteroseismology, stellar modeling, Fundamental parameters, Convection, Radiation
Received: 02 Jul 2019;
Accepted: 04 Oct 2019.
Copyright: © 2019 Nsamba, Campante, Monteiro, Cunha and Sousa. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) and the copyright owner(s) are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
* Correspondence: Mx. Benard Nsamba, Centre for Astrophysics, Faculty of Sciences, University of Porto, Porto, Portugal, firstname.lastname@example.org