Issue |
A&A
Volume 694, February 2025
|
|
---|---|---|
Article Number | C7 | |
Number of page(s) | 1 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202453505e | |
Published online | 19 February 2025 |
Super-slowly rotating Ap (ssrAp) stars: Spectroscopic study
(Corrigendum)
1
European Southern Observatory, Alonso de Cordova 3107, Vitacura, Santiago, Chile
2
Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK
3
South African Astronomical Observatory, PO Box 9 Observatory, 7935 Cape Town, South Africa
4
INAF–Osservatorio Astrofisico di Catania, Via S. Sofia 78, 95123 Catania, Italy
5
Centre for Space Research, North-West University, Mahikeng 2745, South Africa
6
Dipartimento di Fisica e Astronomia, Sezione Astrofisica, Università di Catania, Via S. Sofia 78, I-95123 Catania, Italy
⋆ Corresponding author; gmathys@eso.org
This article has no abstract.
Key words: errata, addenda / binaries: spectroscopic / stars: chemically peculiar / stars: magnetic field / 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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