Issue |
A&A
Volume 640, August 2020
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 2 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/201937137e | |
Published online | 07 August 2020 |
Letter to the Editor
Lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1) (Corrigendum)
1
Instituto de Física y Astronomía, Universidad de Valparaíso, Valparaíso, Chile
e-mail: javier.arancibia@postgrado.uv.cl
2
Núcleo Milenio Formación Planetaria – NPF, Universidad de Valparaíso, Av. Gran Bretaña 1111, Valparaíso, Chile
3
IPAG, Univ. Grenoble Alpes, 38000 Grenoble, France
4
Laboratoire d’Astrophysique de Bordeaux, Univ. Bordeaux, CNRS, B18N, Allée Geoffroy Saint-Hilaire, 33615 Pessac, France
5
Max Planck Institute for Astronomy, Heidelberg, Germany
6
Depto. Astrofísica, Centro de Astrobiología (INTA-CSIC), ESAC Campus, Camino Bajo del Castillo s/n, 28692 Villanueva de la Cañada, Spain
Key words: stars: low-mass / stars: pre-main sequence / stars: abundances / open clusters and associations: individual: Psc-Eri / stars: rotation / errata, addenda
In the original paper (Arancibia-Silva et al. 2020), there was a typographic error in Table 1, where column Gbp-Grp was duplicated from column MG and the actual values referring to the quantity were not displayed. However, this has no impact on the analysis, results, or discussion in the paper since the correct values were used in the analysis (see, for example, Fig. 1 of Arancibia-Silva et al. 2020). The complete table with the correct values is presented in this erratum in Table 1.
Stellar sample properties from Curtis et al. (2019) and EW(Li), radial velocity (Vr), and projected rotational velocity (vsini) measurements
References
- Arancibia-Silva, J., Bouvier, J., Bayo, A., et al. 2020, A&A, 635, L13 [CrossRef] [EDP Sciences] [Google Scholar]
- Curtis, J. L., Agüeros, M. A., Mamajek, E. E., Wright, J. T., & Cummings, J. D. 2019, AJ, 158, 77 [NASA ADS] [CrossRef] [Google Scholar]
© ESO 2020
All Tables
Stellar sample properties from Curtis et al. (2019) and EW(Li), radial velocity (Vr), and projected rotational velocity (vsini) measurements
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