J/A+A/484/815ivo://CDS.VizieR/J/A+A/484/815doi:10.26093/cds/vizier.34840815CDSBertelli G.Girardi L.Marigo P.Nasi E.CDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsIn many astrophysical contexts, the helium content of stars may differ significantly from those usually assumed in evolutionary calculations. In order to improve upon this situation, we have computed tracks and isochrones in the range of initial masses 0.15-20M_{sun}_ for a grid of 39 chemical compositions with the metal content Z between 0.0001 and 0.070 and helium content Y between 0.23 and 0.46. ************************************************************************** * * * Sorry, but the author(s) never supplied the tabular material * * announced in the paper * * * **************************************************************************2008A&A...484..815Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/484/815CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/484/815https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/484/815http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/484/815https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/484/815https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/484/815http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/484/815GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefault