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II.</title><shortName>J/MNRAS/418/284</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/418/284</identifier><altIdentifier>doi:10.26093/cds/vizier.74180284</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bisterzo S.</name></creator><creator><name>Gallino R.</name></creator><creator><name>Straniero O.</name></creator><creator><name>Cristallo S.</name></creator><creator><name>Kappeler F.</name></creator><date role="Updated">2024-07-16T20:12:08Z</date><date role="Created">2012-06-05T15:39:48Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>giant-stars</subject><subject>chemical-abundances</subject><description>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. 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