| Issue |
A&A
Volume 698, May 2025
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/202555611e | |
| Published online | 09 June 2025 | |
Evolution of the near-core rotation frequency of 2497 intermediate-mass stars from their dominant gravito-inertial mode (Corrigendum)
1
Institute of Astronomy, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
2
Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, 6500 GL Nijmegen, The Netherlands
3
Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
4
IRAP, Université de Toulouse, CNRS, UPS, CNES, 14 avenue Édouard Belin, F-31400 Toulouse, France
5
Université Paris-Saclay, Université de Paris, Sorbonne Paris Cité, CEA, CNRS, AIM, 91191 Gif-sur-Yvette, France
6
Institute for Astronomy, University of Hawai’i, Honolulu, HI, 96822, USA
⋆ Corresponding author: conny.aerts@kuleuven.be
Received:
21
May
2025
Accepted:
22
May
2025
This article has no abstract.
Key words: errata, addenda / waves / stars: evolution / stars: interiors / stars: oscillations / stars: rotation
© The Authors 2025
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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