J/A+A/534/A9ivo://CDS.VizieR/J/A+A/534/A9doi:10.26093/cds/vizier.35340009CDSSbordone L.Salaris M.Weiss A.Cassisi S.2011-10-16T15:03:29Z2011-09-22T07:41:14ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frstellar-evolutionary-modelsspectroscopyglobular-star-clustersWe calculated synthetic spectra for typical chemical element mixtures (i.e., a standard alpha-enhanced distribution, and distributions displaying CN and ONa anticorrelations) found in the various subpopulations harboured by individual Galactic globular clusters. From the spectra we determined bolometric corrections to the standard Johnson-Cousins and Stroemgren filters and finally predicted colours. These bolometric corrections and colour-transformations, coupled to our theoretical isochrones with the appropriate chemical composition, provided us with a complete and self-consistent set of theoretical predictions for the effect of abundance variations on the observed cluster colour-magnitude diagrams.2011A&A...534A...9Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/534/A9CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/534/A9https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/534/A9http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/534/A9https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/534/A9https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/534/A9http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/534/A9GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/534/A9/tablea1Abundances for all elements in the considered mixturesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZAtomic numbermeta.id;meta.mainintElElementphys.abundcharfMassReference fractional mass for Y=0.246 (Z=9.9937e-04)meta.ref;phys.massdouble[El]Reference abundance of element (logN(El)-logN(H)+12)) for Y=0.246phys.abundfloatfMass1Fractional mass for CNONa1, Y=0.246 (Z=1.8343e-03)phys.massdouble[El]1Abundance of element (logN(El)-logN(H)+12) for CNONa1, Y=0.246phys.abundfloat[El]1-[El]Difference between this mixture [El] and reference mixture [El] for CNONa1, Y=0.246phys.abundfloatfMass2Fractional mass for CNONa1, Y=0.400 (Z=1.4597e-03)phys.massdouble[El]2Abundance of element (logN(El)-logN(H)+12) for CNONaI, Y=0.400phys.abundfloat[El]2-[El]Difference between this mixture [El] and reference mixture [El] for CNONa1, Y=0.400phys.abundfloatfMass3Fractional mass for CNONa2, Y=0.246 (Z=9.9937e-04)phys.massdouble[El]3Abundance of element (logN(El)-logN(H)+12) for CNONa2, Y=0.246phys.abundfloat[El]3-[El]Difference between this mixture [El] and reference mixture [El] for CNONa2, Y=0.246phys.abundfloat