| Issue |
A&A
Volume 620, December 2018
|
|
|---|---|---|
| Article Number | C3 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201527235e | |
| Published online | 14 December 2018 | |
The role of binaries in the enrichment of the early Galactic halo
II. Carbon-enhanced metal-poor stars – CEMP-no stars (Corrigendum)
1 George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A&M University, College Station, TX 77843, USA
e-mail: thansen@tamu.de
2 Dawn Cosmology Centre, The Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen, Denmark
e-mail: ja@nbi.ku.dk; birgitta@nbi.ku.dk
3 Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, 8000 Aarhus C, Denmark
4 Department of Physics and JINA Center for the Evolution of the Elements, University of Notre Dame, Notre Dame, IN 46556, USA
5 DTU Space, National Space Institute, Technical University of Denmark, Elektrovej 327, 2800 Lyngby, Denmark
Key words: Galaxy: formation / Galaxy: halo / stars: chemically peculiar / binaries: spectroscopic / ISM: structure / errata, addenda
In Hansen et al. (2016) the RV mean for HE 0020−1741 listed in Table 2 in the printed article is given incorrectly. The correct value is 93.039 km s−1, in agreement with the individual RV values for the star listed in Table A.1.
© ESO 2018
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