s-process in low-metallicity stars. II.

DOI

High-resolution spectroscopic observations of 100 metal-poor carbon and s-rich stars (CEMP-s) collected from the literature are compared with the theoretical nucleosynthesis models of the asymptotic giant branch (AGB) presented in Paper I, Cat. J/MNRAS/404/1529.

Cone search capability for table J/MNRAS/418/284/stars (C-Enriched Metal Poor (CEMP) stars studied: abundances for CEMP-s and CEMP-s/r stars)

Identifier
DOI http://doi.org/10.26093/cds/vizier.74180284
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/MNRAS/418/284
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/418/284
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/418/284
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/MNRAS/418/284
Provenance
Creator Bisterzo S.; Gallino R.; Straniero O.; Cristallo S.; Kappeler F.
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