The r-process Alliance: spectroscopic follow-up of low-metallicity star candidates from the best & brightest survey
dc.creator | Placco, Vinicius Moris | |
dc.creator | Santucci, Rafael Miloni | |
dc.creator | Beers, Timothy C. | |
dc.creator | Chanamé, Julio | |
dc.creator | Paz Sepúlveda, María | |
dc.creator | Coronado, Johanna | |
dc.creator | Rossi, Silvia Cristina Fernandes | |
dc.creator | Young, Sun Lee | |
dc.creator | Starkenburg, Else | |
dc.creator | Youakim, Kris | |
dc.date.accessioned | 2023-05-12T15:44:05Z | |
dc.date.available | 2023-05-12T15:44:05Z | |
dc.date.issued | 2019 | |
dc.description.abstract | We present results from an observing campaign to identify low-metallicity stars in the Best & Brightest Survey. From medium-resolution (R ∼ 1200–2000) spectroscopy of 857 candidates, we estimate the stellar atmospheric parameters (Teff, log g, and Fe H [ ]), as well as carbon and α-element abundances. We find that 69% of the observed stars have Fe H [ ] −1.0, 39% have Fe H [ ] −2.0, and 2% have Fe H [ ] −3.0. There are also 133 carbon-enhanced metal-poor (CEMP) stars in this sample, with 97 CEMP Group I and 36 CEMP Group II stars identified in the A(C) versus [Fe/H] diagram. A subset of the confirmed low-metallicity stars were followed-up with high-resolution spectroscopy, as part of the R-process Alliance, with the goal of identifying new highly and moderately r-process-enhanced stars. Comparison between the stellar atmospheric parameters estimated in this work and from high-resolution spectroscopy exhibit good agreement, confirming our expectation that medium-resolution observing campaigns are an effective way of selecting interesting stars for further, more targeted, efforts. | pt_BR |
dc.identifier.citation | PLACCO, Vinicius M. et al. The r-process Alliance: spectroscopic follow-up of low-metallicity star candidates from the best & brightest survey. The Astrophysical Journal, Bristol, v. 870, n. 2, e122, 2019. DOI: 10.3847/1538-4357/aaf3b9. Disponível em: https://iopscience.iop.org/article/10.3847/1538-4357/aaf3b9. Acesso em: 11 maio 2023. | pt_BR |
dc.identifier.doi | 10.3847/1538-4357/aaf3b9 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.uri | http://repositorio.bc.ufg.br/handle/ri/22523 | |
dc.language.iso | eng | pt_BR |
dc.publisher.country | Gra-bretanha | pt_BR |
dc.publisher.department | Instituto de Estudos Socioambientais - IESA (RG) | pt_BR |
dc.rights | Acesso Aberto | pt_BR |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | * |
dc.title | The r-process Alliance: spectroscopic follow-up of low-metallicity star candidates from the best & brightest survey | pt_BR |
dc.type | Artigo | pt_BR |
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