Issue |
A&A
Volume 695, March 2025
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 1 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202554263e | |
Published online | 18 March 2025 |
Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud (Corrigendum)
1
IAASARS, National Observatory of Athens, 15236 Penteli, Greece
2
National and Kapodistrian University of Athens, 15784 Athens, Greece
3
Institute of Astrophysics FORTH, GR-71110 Heraklion, Greece
⋆ Corresponding author; k.antoniadis@noa.gr
Key words: errata / addenda / stars: evolution / stars: late-type / stars: massive / stars: mass-loss / supergiants
We found a typographical mistake in Tables 3 and 4 of our original paper where we presented the coefficients of our mass-loss rate relation. More specifically, the values of c2 and c3 for log(L/L⊙)≳4.4 were the ones for steady-state winds and the MRN grain size distribution in the range of [0.01, 1] μm instead of [0.1, 1], which is presented in our main results.
1. Results
Tables 1 and 2 are the corrected versions of Tables 3 and 4, respectively, appearing in our paper but replaced with the corrected values for c2 and c3 at log(L/L⊙)≳4.4 for our relation:
Mass-loss rate prescriptions from different works.
2. Conclusion
The figures and conclusions of our work remain the same, since the mistake was just a typo.
Acknowledgments
We thank Amedeo Romagnolo for bringing this mistake to our attention.
References
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© The Authors 2025
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