| Issue |
A&A
Volume 649, May 2021
|
|
|---|---|---|
| Article Number | C6 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/202040055e | |
| 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
e-mail: anoll@irap.omp.eu
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.
 |
Fig. 1.
Actual échelle diagram of the best model for αov = 0.15, which replaces Fig. 8 of Noll et al. (2021). |
| Open with DEXTER | |
References
- Noll, A., Deheuvels, S., & Ballot, J. 2021, A&A, 647, A187 [EDP Sciences] [Google Scholar]
© 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.
All Figures
|
Fig. 1.
Actual échelle diagram of the best model for αov = 0.15, which replaces Fig. 8 of Noll et al. (2021). |
| Open with DEXTER | |
| In the text | |
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