TOPoS: V. Abundance ratios in a sample of very metal-poor turn-off stars
dc.contributor.author | François P. | |
dc.contributor.author | Caffau E. | |
dc.contributor.author | Bonifacio P. | |
dc.contributor.author | Spite M. | |
dc.contributor.author | Spite F. | |
dc.contributor.author | Cayrel R. | |
dc.contributor.author | Christlieb N. | |
dc.contributor.author | Gallagher A.J. | |
dc.contributor.author | Klessen R. | |
dc.contributor.author | Koch A. | |
dc.contributor.author | Ludwig H. | |
dc.contributor.author | Monaco L. | |
dc.contributor.author | Plez B. | |
dc.contributor.author | Steffen M. | |
dc.contributor.author | Zaggia S. | |
dc.date.accessioned | 2022-06-22T13:28:32Z | |
dc.date.available | 2022-06-22T13:28:32Z | |
dc.date.issued | 2018-12 | |
dc.description | Indexación Scopus | es |
dc.description.abstract | Context. Extremely metal-poor stars are keys to understand the early evolution of our Galaxy. The ESO large programme TOPoS has been tailored to analyse a new set of metal-poor turn-off stars, whereas most of the previously known extremely metal-poor stars are giant stars. Aims. Sixty five turn-off stars (preselected from SDSS spectra) have been observed with the X-shooter spectrograph at the ESO VLT Unit Telescope 2, to derive accurate and detailed abundances of magnesium, silicon, calcium, iron, strontium and barium. Methods. We analysed medium-resolution spectra (R 10 000) obtained with the ESO X-shooter spectrograph and computed the abundances of several α and neutron-capture elements using standard one-dimensional local thermodynamic equilibrium (1D LTE) model atmospheres. Results. Our results confirms the super-solar [Mg/Fe] and [Ca/Fe] ratios in metal-poor turn-off stars as observed in metal-poor giant stars. We found a significant spread of the [α/Fe] ratios with several stars showing subsolar [Ca/Fe] ratios. We could measure the abundance of strontium in 12 stars of the sample, leading to abundance ratios [Sr/Fe] around the Solar value. We detected barium in two stars of the sample. One of the stars (SDSS J114424-004658) shows both very high [Ba/Fe] and [Sr/Fe] abundance ratios (>1 dex). © ESO 2018. | es |
dc.description.uri | https://www.aanda.org/articles/aa/full_html/2018/12/aa34375-18/aa34375-18.html | |
dc.identifier.citation | Astronomy and Astrophysics Volume 6201 December 2018 Article number A187 | es |
dc.identifier.doi | 10.1051/0004-6361/201834375 | |
dc.identifier.issn | 00046361 | |
dc.identifier.uri | https://repositorio.unab.cl/xmlui/handle/ria/22928 | |
dc.language.iso | en | es |
dc.publisher | EDP Sciences | es |
dc.subject | Asymptotic Giant Branch Stars | es |
dc.subject | Iron | es |
dc.subject | Dwarf Galaxies | es |
dc.subject | Local thermodynamic equilibrium | es |
dc.subject | Model atmosphere | es |
dc.subject | Neutron capture | es |
dc.subject | Resolution spectra | es |
dc.title | TOPoS: V. Abundance ratios in a sample of very metal-poor turn-off stars | es |
dc.type | Artículo | es |
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