Volume 649, May 2021
|Number of page(s)||1|
|Section||Stellar structure and evolution|
|Published online||24 May 2021|
Probing core overshooting using subgiant asteroseismology: The case of KIC10273246 (Corrigendum)
IRAP, Université de Toulouse, CNRS, CNES, UPS, Toulouse, France
Key words: asteroseismology / convection / stars: evolution / stars: interiors / stars: individual: KIC10273246 / errata, addenda
In Noll et al. (2021), Fig. 8 is not the actual échelle diagram of the best model, and must be replaced with Fig. 1 of the present corrigendum. This has no impact on any result or conclusion of the paper.
Actual échelle diagram of the best model for αov = 0.15, which replaces Fig. 8 of Noll et al. (2021).
|Open with DEXTER|
© A. Noll et al. 2021
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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