Online-Ressource | |
Verfasst von: | François, Patrick [VerfasserIn] |
Caffau, Elisabetta [VerfasserIn] | |
Christlieb, Norbert [VerfasserIn] | |
Klessen, Ralf S. [VerfasserIn] | |
Koch-Hansen, Andreas [VerfasserIn] | |
Ludwig, Hans-Günter [VerfasserIn] | |
Titel: | TOPoS |
Titelzusatz: | V: Abundance ratios in a sample of very metal-poor turn-off stars |
Verf.angabe: | P. François, E. Caffau, P. Bonifacio, M. Spite, F. Spite, R. Cayrel, N. Christlieb, A. J. Gallagher, R. Klessen, A. Koch, H.-G. Ludwig, L. Monaco, B. Plez, M. Steffen, and S. Zaggia |
E-Jahr: | 2018 |
Jahr: | 31 Oct 2018 |
Umfang: | 17 S. |
Fussnoten: | Gesehen am 16.10.2020 |
Titel Quelle: | Enthalten in: De.arxiv.org |
Ort Quelle: | [S.l.] : Arxiv.org, 1991 |
Jahr Quelle: | 2018 |
Band/Heft Quelle: | (2018) Artikel-Nummer 1811.00035, 17 Seiten |
Abstract: | 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. 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. We analysed medium-resolution spectra (R ~ 10 000) obtained with the ESO X-Shooter spectrograph and computed the abundances of several alpha and neutron-capture elements using standard one-dimensional local thermodynamic equilibrium (1D LTE) model atmospheres. 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 [alpha/Fe] ratios with several stars showing sub-solar [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). |
URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt. Volltext: http://arxiv.org/abs/1811.00035 |
Datenträger: | Online-Ressource |
Sprache: | eng |
Sach-SW: | Astrophysics - Solar and Stellar Astrophysics |
K10plus-PPN: | 1586572393 |
Verknüpfungen: | → Sammelwerk |