| Issue |
A&A
Volume 673, May 2023
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 9 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/202244788e | |
| Published online | 28 April 2023 | |
Titanium abundances in late-type stars
I. 1D non-local thermodynamic equilibrium modelling in benchmark dwarfs and giants (Corrigendum)
1
Department of Astronomy, Stockholm University, AlbaNova University Centre,
Roslagstullsbacken,
106 91
Stockholm,
Sweden
e-mail: jack.mallinson@astro.su.se
2
Theoretical Astrophysics, Department of Physics and Astronomy, Uppsala University,
Box 516,
751 20
Uppsala,
Sweden
3
Department of Theoretical Physics and Astronomy, Herzen University,
St. Petersburg,
Riv Moyka
191186,
Russia
Key words: atomic processes / radiative transfer / line: formation / stars: abundances / stars: atmospheres / errata, addenda
The linelist in the appendix was printed with log(gf) values and energies corresponding to the previous line, and two lines belonging to Ti I were mistakenly printed in the Ti II section. These values were not used in calculating abundances and have no impact on the results or conclusions.
Lines considered in the analysis, including saturated lines that were removed during the final abundance calculation.
References
- Scott, P., Asplund, M., Grevesse, N., Bergemann, M., & Sauval, A. J. 2015, A&A, 573, A26 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© 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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Lines considered in the analysis, including saturated lines that were removed during the final abundance calculation.
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