CEMP in Gaia DR3

Carbon-enhanced metal-poor (CEMP) stars comprise almost a third of stars with [Fe/H]30kpc. Future higher resolution spectroscopic follow-up of these candidates will provide validations of their classification and enable investigations of the frequency of CEMP-s and CEMP-no stars throughout the Galaxy, to further constrain the nature of their progenitors.

Cone search capability for table J/MNRAS/523/4049/cemp (CEMP candidates (P>=0.5))

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/523/4049
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/523/4049
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/523/4049
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/523/4049
Provenance
Creator Lucey M.; Al Kharusi N.; Hawkins K.; Ting Y.-S.; Ramachandra N.,Price-Whelan A.M.; Beers T.C.; Sun Lee Y.; Yoon J.
Publisher CDS
Publication Year 2023
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; Natural Sciences; Physics; Stellar Astronomy