| Issue |
A&A
Volume 675, July 2023
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 2 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/202038753e | |
| Published online | 18 July 2023 | |
Benchmarking the fundamental parameters of Ap stars with optical long-baseline interferometric measurements★ (Corrigendum)
1
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
e-mail: karine.perraut@univ-grenoble-alpes.fr
2
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP,
Rua das Estrelas,
4150-762
Porto, Portugal
3
School of Physics and Astronomy, University of Birmingham,
Birmingham,
B15 2TT, UK
4
Institute of Astronomy, Russian Academy of Sciences,
Pyatnitskaya 48,
119017
Moscow, Russia
5
Max-Planck Institute fur Sonnensystemforschung,
Justus-von-Liebig-Weg 3,
37077
Göttingen, Germany
6
Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange,
France
7
Univ. Lyon, Univ. Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574,
69230
Saint-Genis-Laval, France
8
CHARA Array, Mount Wilson Observatory,
91023
Mount Wilson CA, USA
9
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven,
3001
Leuven, Belgium
Key words: methods: observational / techniques: high angular resolution / techniques: interferometric / stars: fundamental parameters / errata, addenda
This corrigendum corrects Table 1 in which the columns gathering the B and V magnitudes were inverted, and the erroneous value of the effective temperature of HD 201601 that was derived from interferometric observations in Table 4. The corrected Table 1 is given below.
An effective temperature of 7364 ± 235 K was derived for HD 201601, as reported previously in Perraut et al. (2011). Figure 5 and Table 4 have been updated accordingly. These corrections affect neither the results nor the conclusions of the original paper.
Acknowledgements
We thank Victor Maraud for pointing out these imprecisions in our original manuscript.
References
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© The Authors 2023
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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All Tables
Stellar properties for the complete Ap sample, with Teff and L derived from Kochukhov & Bagnulo (2006).
Limb-darkened angular diameters in the R band derived from interferometric measurements, Gaia DR2 parallaxes, radii, effective temperatures, and luminosities derived from interferometric measurements for the complete Ap sample.
All Figures
 |
Fig. 5 Comparison between the radii (left) and the effective temperatures (right) derived from interferometric measurements and those derived from the self-consistent spectroscopic modelling. The dash lines give the 1:1 relations. The numbers close to the symbols refer to Table 4. |
| In the text | |
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