Lithium-rotation connection in the newly discovered young stellar stream Psc-Eri (Meingast 1) (Corrigendum)
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...
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Instituto Nacional de Técnica Aeroespacial (INTA) |
| Repositorio: | DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial |
| OAI Identifier: | oai:digital.inta.es:20.500.12666/261 |
| Acceso en línea: | https://www.aanda.org/articles/aa/full_html/2020/08/aa37137e-19/aa37137e-19.html http://hdl.handle.net/20.500.12666/261 |
| Access Level: | acceso abierto |
| Palabra clave: | Stars: low mass Stars: pre main sequence Stars: abundances Open clusters and associations: individual: Psc-Eri Stars: rotation Errata-addenda |
| Sumario: | 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. |
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