| Issue |
A&A
Volume 694, February 2025
|
|
|---|---|---|
| Article Number | C9 | |
| Number of page(s) | 1 | |
| Section | Stellar atmospheres | |
| DOI | https://doi.org/10.1051/0004-6361/202453645e | |
| Published online | 19 February 2025 | |
Abundances in eight bulge stars from the optical and near-infrared (Corrigendum)
1
Observatoire de Paris, LERMA, Collège de France, CNRS, PSL University, Sorbonne University,
75014,
Paris,
France
2
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Departamento de Astronomia, Universidade de São Paulo,
05508-090,
SP,
Brazil
3
Lund Observatory, Department of Astronomy and Theoretical Physics, Lund University,
Box 43,
221 00
Lund,
Sweden
4
Instituto de Astronomía, Universidad Católica del Norte,
Av. Angamos 0610,
Antofagasta,
Chile
★ Corresponding author; patricia2.silva@alumni.usp.br
Key words: stars: abundances / Galaxy: bulge / globular clusters: individual: NGC 6522 / globular clusters: individual: NGC 6558 / globular clusters: individual: HP 1 / globular clusters: individual: Palomar 6 / errata, addenda
In Table 3, the values for the alpha-to-iron ratios were mistakenly reported as the values for the microturbulence velocity given in the APOGEE survey (fourth column). The correct values, taken from the DR17 APOGEE table of microturbulence velocity, are given in this version of the table presented below.
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© 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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All Tables
ASPCAP (noncalibrated) spectroscopic parameters for the stars from APOGEE, and from UVES.
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