J/A+A/453/769ivo://CDS.VizieR/J/A+A/453/769doi:10.26093/cds/vizier.34530769CDSClaret A.2017-06-30T05:48:30Z2006-07-12T13:29:36ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsIn this paper, we present new specific stellar models for the Large Magellanic Cloud. In order to take the observational uncertainties in the chemical composition into account, we have computed two grids: (X, Z) = (0.730, 0.010) and (0.739, 0.007). The covered mass range was 0.80 up to 125M_{sun}. The effects of rotation can be investigated by using the gravity-darkening exponents that are available for each track. The tidal constant E_2_, depth of the convective outer zone, and the radius of gyration are computed and presented in a suitable format for studying the tidal evolution of a given close binary. The isochrones (and also those corresponding to the previous grids) will be presented in a future paper.2006A&A...453..769Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/453/769CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/424/919 : New grids of stellar models - I. (Claret, 2004)J/A+A/440/647 : New grids of stellar models - II. (Claret, 2005)J/A+A/467/1389 : New grids of stellar models - IV. (Claret, 2007)J/A+AS/109/441 : Stellar models until He burning - I. (Claret, 1995)J/A+AS/114/549 : Stellar models until He burning - II. (Claret+, 1995)J/A+AS/125/439 : Stellar models until He burning - III. (Claret+, 1997)J/A+AS/133/123 : Stellar models until He burning - IV. (Claret+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/453/769https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/453/769http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/453/769https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/453/769https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/453/769http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/453/769GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/453/769/gridSummary of parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMInitial masssolMassphys.massfloatnullablelogMInitial masslog(solMass)phys.massfloatX[0.730-0.739] X initial X composition (H)phys.abund.XfloatZ[0.007-0.01] Z initial compositionsrc.redshift;phys.compositionfloatOv[0/1] Overshooting (G1)stat.paramintFileNameOriginal filename with result (in subdirectory)meta.id;meta.filecharHRPlot the Herzsprung-Russel diagram for this massmeta.ref.urlcharEvolutionDetails of evolution for this set of (X Z M) parametersmeta.ref.urlcharJ/A+A/453/769/z010Grid for (X,Z)=(0.730,0.010)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogMInitial masslog(solMass)phys.massfloatX[0.730-0.739] X initial X composition (H)phys.abund.XfloatZ[0.007-0.01] Z initial compositionsrc.redshift;phys.compositionfloatOv[0/1] Overshooting (G1)stat.paramintAgeAge of the modelsyrtime.agedoublelog(L)Log (Total luminosity)log(solLum)phys.luminositydoublelog(g)Log (Surface gravity)log(cm.s**-2)arith.zpdoublelog(Teff)Log (Effective temperature)log(K)arith.zpdoubleMassActual mass of the modelsolMassphys.mass;meta.modelleddoublelogdM/dtLog (mass loss rate)log(solMass.yr**-1)phys.mass.lossdoublelogDcLog (central density)log(g.cm**-3)arith.zpdoublelogTcLog (central temperature)log(K)arith.zpdoubleQcCore mass (fraction)phys.massdoubleXcH central abundance (mass fraction)phys.abund.XdoubleXsH surface abundance (mass fraction)phys.abund.XdoubleYc4He central abundance (mass fraction)phys.abund;em.wl.centraldoubleYs4He surface abundance (mass fraction)phys.abund.YdoubleC12c12C central abundance (mass fraction)phys.abunddoubleC12s12C surface abundance (mass fraction)phys.abunddoubleC13c13C central abundance (mass fraction)phys.abunddoubleC13s13C surface abundance (mass fraction)phys.abunddoubleN14c14N central abundance (mass fraction)phys.abunddoubleN14s14N surface abundance (mass fraction)phys.abunddoubleO16c16O central abundance (mass fraction)phys.abunddoubleO16s16O surface abundance (mass fraction)phys.abunddoubleO17c17O central abundance (mass fraction)phys.abunddoubleO17s17O surface abundance (mass fraction)phys.abunddoubleO18c18O central abundance (mass fraction)phys.abunddoubleO18s18O surface abundance (mass fraction)phys.abunddoubleNe20c20Ne central abundance (mass fraction)phys.abunddoubleNe20s20Ne surface abundance (mass fraction)phys.abunddoubleNe22c22Ne central abundance (mass fraction)phys.abunddoubleNe22s22Ne surface abundance (mass fraction)phys.abunddoubleMg24c24Mg central abundance (mass fraction)phys.abunddoubleMg24s24Mg surface abundance (mass fraction)phys.abunddoubleMg25c25Mg central abundance (mass fraction)phys.abunddoubleMg25s25Mg surface abundance (mass fraction)phys.abunddoubleMg26c26Mg central abundance (mass fraction)phys.abunddoubleMg26s26Mg surface abundance (mass fraction)phys.abunddoublelogK2Log(Apsidal motion constant (j=2))stat.paramdoublelogK3Log(Apsidal motion constant (j=3))stat.paramdoublelogK4Log(Apsidal motion constant (j=4))stat.paramdoubleXBFFractional depth of convective envelopestat.paramdoublelogE2Log(Tidal torque constant)stat.paramdoubleECOPolytropic envelope characteristicstat.paramdoublealphaPalphaP = -Ep x R/GM2stat.paramdoubleRgyrFractional gyration radiusstat.paramdoublebeta1Gravity-darkening exponentstat.paramdoubleJ/A+A/453/769/z007Grid for (X,Z)=(0.739,0.007)XBFFractional depth of convective envelopestat.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogMInitial masslog(solMass)phys.massfloatX[0.730-0.739] X initial X composition (H)phys.abund.XfloatZ[0.007-0.01] Z initial compositionsrc.redshift;phys.compositionfloatOv[0/1] Overshooting (G1)stat.paramintAgeAge of the modelsyrtime.agedoublelog(L)Log (Total luminosity)log(solLum)phys.luminositydoublelog(g)Log (Surface gravity)log(cm.s**-2)arith.zpdoublelog(Teff)Log (Effective temperature)log(K)arith.zpdoubleMassActual mass of the modelsolMassphys.mass;meta.modelleddoublelogdM/dtLog (mass loss rate)log(solMass.yr**-1)phys.mass.lossdoublelogDcLog (central density)log(g.cm**-3)arith.zpdoublelogTcLog (central temperature)log(K)arith.zpdoubleQcCore mass (fraction)phys.massdoubleXcH central abundance (mass fraction)phys.abund.XdoubleXsH surface abundance (mass fraction)phys.abund.XdoubleYc4He central abundance (mass fraction)phys.abund;em.wl.centraldoubleYs4He surface abundance (mass fraction)phys.abund.YdoubleC12c12C central abundance (mass fraction)phys.abunddoubleC12s12C surface abundance (mass fraction)phys.abunddoubleC13c13C central abundance (mass fraction)phys.abunddoubleC13s13C surface abundance (mass fraction)phys.abunddoubleN14c14N central abundance (mass fraction)phys.abunddoubleN14s14N surface abundance (mass fraction)phys.abunddoubleO16c16O central abundance (mass fraction)phys.abunddoubleO16s16O surface abundance (mass fraction)phys.abunddoubleO17c17O central abundance (mass fraction)phys.abunddoubleO17s17O surface abundance (mass fraction)phys.abunddoubleO18c18O central abundance (mass fraction)phys.abunddoubleO18s18O surface abundance (mass fraction)phys.abunddoubleNe20c20Ne central abundance (mass fraction)phys.abunddoubleNe20s20Ne surface abundance (mass fraction)phys.abunddoubleNe22c22Ne central abundance (mass fraction)phys.abunddoubleNe22s22Ne surface abundance (mass fraction)phys.abunddoubleMg24c24Mg central abundance (mass fraction)phys.abunddoubleMg24s24Mg surface abundance (mass fraction)phys.abunddoubleMg25c25Mg central abundance (mass fraction)phys.abunddoubleMg25s25Mg surface abundance (mass fraction)phys.abunddoubleMg26c26Mg central abundance (mass fraction)phys.abunddoubleMg26s26Mg surface abundance (mass fraction)phys.abunddoublelogK2Log(Apsidal motion constant (j=2))stat.paramdoublelogK3Log(Apsidal motion constant (j=3))stat.paramdoublelogK4Log(Apsidal motion constant (j=4))stat.paramdoublelogE2Log(Tidal torque constant)stat.paramdoubleECOPolytropic envelope characteristicstat.paramdoublealphaPalphaP = -Ep x R/GM2stat.paramdoubleRgyrFractional gyration radiusstat.paramdoublebeta1Gravity-darkening exponentstat.paramdouble