Abundances of F-G main-sequence stars

DOI

Detailed chemical abundances of volatile and refractory elements have been discussed in the context of terrestrial-planet formation during in past years. The HARPS-GTO high-precision planet-search program has provided an extensive database of stellar spectra, which we have inspected in order to select the best-quality spectra available for late type stars. We study the volatile-to-refractory abundance ratios to investigate their possible relation with the low-mass planetary formation.

Cone search capability for table J/A+A/552/A6/abundances (Abundance ratios of all F-, G-type analogs studied in the paper)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35520006
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/552/A6
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/552/A6
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/552/A6
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/552/A6
Provenance
Creator Gonzalez Hernandez J.I.; Delgado-Mena E.; Sousa S.; Israelian G.,Santos N.C.; Adibekyan V.Zh.; Udry S.
Publisher CDS
Publication Year 2013
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; Stellar Astronomy