| Issue |
A&A
Volume 694, February 2025
|
|
|---|---|---|
| Article Number | C6 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/202553907e | |
| Published online | 14 February 2025 | |
Galactic runaway O and Be stars found using Gaia DR3 (Corrigendum)
Departament de Física Quàntica i Astrofísica, Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (IEEC-UB),
Martí i Franquès 1,
08028
Barcelona,
Spain
★ Corresponding author; mcarretero@fqa.ub.edu
Key words: stars: early-type / stars: emission-line, Be / stars: kinematics and dynamics / gamma rays: stars / X-rays: binaries / errata, addenda
The values of U⊙, V⊙, W⊙, dΘ/dR, and their corresponding uncertainties were incorrectly quoted in the original manuscript. The values used in all the computations presented in the original article are U⊙ = 10.6 ± 1.2 km s−1, V⊙ = 10.7 ± 6.0 km s−1, W⊙= 7.6 ± 0.7 km s−1, and dΘ/dR = −1.4 ± 0.3 km s−1 kpc−1. The results and figures are not affected.
© 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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