| Issue |
A&A
Volume 635, March 2020
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201834461e | |
| Published online | 03 March 2020 | |
Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy (Corrigendum)
1
Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
e-mail: bellinger@phys.au.dk
2
Stellar Ages & Galactic Evolution (SAGE) Group, Max Planck Institute for Solar System Research, Göttingen, Germany
3
Max Planck Institute for Astrophysics, Garching, Germany
4
Department of Astronomy, Yale University, New Haven, CT, USA
This article has no abstract.
Key words: asteroseismology / stars: abundances / stars: low-mass / stars: evolution / stars: oscillations / errata, addenda
© ESO 2020
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