Volume 620, December 2018
|Number of page(s)||1|
|Section||Stellar structure and evolution|
|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
2 Dawn Cosmology Centre, The Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, 2100 Copenhagen, Denmark
e-mail: firstname.lastname@example.org; email@example.com
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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