J/A+A/494/209ivo://CDS.VizieR/J/A+A/494/209doi:10.26093/cds/vizier.34940209CDSLandin N.R.Mendes L.T.S.Vaz L.P.R.2017-07-11T13:08:20Z2009-04-04T21:22:22ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelspre-main-sequence-starsIn close binary systems, the axial rotation and the mutual tidal forces of the component stars deform each other and destroy their spherical symmetry by means of the respective disturbing potentials. We present new models for low-mass, pre-main sequence stars that include the combined distortion effects of tidal and rotational forces on the equilibrium configuration of stars. Using our theoretical results, we aim at investigating the effects of interaction between tides and rotation on the stellar structure and evolution.2009A&A...494..209Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/494/209CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/494/209https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/494/209http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/494/209https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/494/209https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/494/209http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/494/209GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/494/209/table1aEvolutionary tracks for standard modelsrecnoRecord 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.luminositydoublelog(Teff)Effective temperaturelog(K)phys.temperature.effectivedoublelog(g)Surface gravitylog(cm.s**-2)phys.gravitydoublelog(k2)Apsidal motion constant (j=2)stat.paramdoublelog(k3)Apsidal motion constant (j=3)stat.paramdoublelog(k4)Apsidal motion constant (j=4)stat.paramdoublebetaGyration radiiphys.size.radiusdoublePer? Rotational period (for table1c and table1d only)dtime.perioddoublenullableJ/A+A/494/209/table1bEvolutionary tracks for binary modelsrecnoRecord 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.luminositydoublelog(Teff)Effective temperaturelog(K)phys.temperature.effectivedoublelog(g)Surface gravitylog(cm.s**-2)phys.gravitydoublelog(k2)Apsidal motion constant (j=2)stat.paramdoublelog(k3)Apsidal motion constant (j=3)stat.paramdoublelog(k4)Apsidal motion constant (j=4)stat.paramdoublebetaGyration radiiphys.size.radiusdoublePer? Rotational period (for table1c and table1d only)dtime.perioddoublenullableJ/A+A/494/209/table1cEvolutionary tracks for rotating modelsrecnoRecord 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.luminositydoublelog(Teff)Effective temperaturelog(K)phys.temperature.effectivedoublelog(g)Surface gravitylog(cm.s**-2)phys.gravitydoublelog(k2)Apsidal motion constant (j=2)stat.paramdoublelog(k3)Apsidal motion constant (j=3)stat.paramdoublelog(k4)Apsidal motion constant (j=4)stat.paramdoublebetaGyration radiiphys.size.radiusdoublePer? Rotational period (for table1c and table1d only)dtime.perioddoublenullableJ/A+A/494/209/table1dEvolutionary tracks for rotating binary modelsMassMasssolMassphys.massfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlog(Age)Age of modelslog(yr)time.agefloatlog(L)Total luminositylog(solLum)phys.luminositydoublelog(Teff)Effective temperaturelog(K)phys.temperature.effectivedoublelog(g)Surface gravitylog(cm.s**-2)phys.gravitydoublelog(k2)Apsidal motion constant (j=2)stat.paramdoublelog(k3)Apsidal motion constant (j=3)stat.paramdoublelog(k4)Apsidal motion constant (j=4)stat.paramdoublebetaGyration radiiphys.size.radiusdoublePer? Rotational period (for table1c and table1d only)dtime.perioddoublenullable