Carbon-enhanced metal-poor stars in the Galaxy

DOI

We have developed a new procedure to search for carbon-enhanced metal-poor (CEMP) stars from the Hamburg/ESO (HES) prism-survey plates. This method employs an extended line index for the CH G band, which we demonstrate to have superior performance when compared to the narrower G-band index formerly employed to estimate G-band strengths for these spectra.

Cone search capability for table J/AJ/139/1051/CEMPstars (Stellar data, atmospheric parameters and carbon abundance estimates for the observed carbon-enhanced metal-poor (CEMP) candidates)

Identifier
DOI http://doi.org/10.26093/cds/vizier.51391051
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/AJ/139/1051
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/139/1051
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/139/1051
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/AJ/139/1051
Provenance
Creator Placco V.M.; Kennedy C.R.; Rossi S.; Beers T.C.; Lee Y.S.; Christlieb N.,Sivarani T.; Reimers D.; Wisotzki L.
Publisher CDS
Publication Year 2012
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