HERES VI. Galactic chemical evolution of Si and C

DOI

To obtain detailed silicon abundances of metal-poor stars, we aim to explore the correlation between the abundance ratios and the stellar parameters and the chemical enrichment of the interstellar medium (ISM). We determined the silicon abundances of 253 metal-poor stars in the metallicity range -4<[Fe/H]<-1.5, based on non-local thermodynamic equilibrium (NLTE) line formation calculations of neutral silicon and high-resolution spectra obtained with VLT-UT2/UVES.

Cone search capability for table J/A+A/528/A92/table3 (Abundance results of carbon and silicon)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35280092
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/528/A92
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/528/A92
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/528/A92
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/528/A92
Provenance
Creator Zhang L.; Karlsson T.; Christlieb N.; Korn A.J.; Barklem P.S.; Zhao G.
Publisher CDS
Publication Year 2011
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Physics