J/A+A/510/A46ivo://CDS.VizieR/J/A+A/510/A46doi:10.26093/cds/vizier.35100046CDSLandin N.R.Mendes L.T.S.Vaz L.P.R.2017-07-10T06:22:16Z2010-03-01T14:49:58ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelspre-main-sequence-starsMagnetic fields are at the heart of the observed stellar activity in late-type stars, and they are presumably generated by a dynamo mechanism at the interface layer (tachocline) between the radiative core and the base of the convective envelope. Since dynamo models are based on the interaction between differential rotation and convective motions, the introduction of rotation in the ATON 2.3 stellar evolutionary code allows for explorations regarding a physically consistent treatment of magnetic effects in stellar structure and evolution, even though there are formidable mathematical and numerical challenges involved.2010A&A...510A..46Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/510/A46CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/494/209 : Pre-main sequence evolutionary tracks (Landin+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/510/A46https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/510/A46http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/510/A46https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/510/A46https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/510/A46http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/510/A46GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/510/A46/table1Evolutionary tracksrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMassMasssolMassphys.massfloatlog(Age)Age of modelslog(yr)time.agefloatlog(L)Total luminositylog(solLum)phys.luminosityfloatlog(Teff)Effective temperaturelog(K)phys.temperature.effectivefloatlog(g)Surface gravitylog(cm.s**-2)phys.gravityfloatlog(k2)Local convective turnover timelog(s)stat.paramfloatlog(k3)Global convective turnover timelog(d)stat.paramdoublelog(k4)Rossby numberstat.paramfloat