| 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
This article has no abstract.
Key words: errata / addenda / stars: evolution / stars: late-type / stars: massive / stars: mass-loss / supergiants
© 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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