J/A+A/502/817ivo://CDS.VizieR/J/A+A/502/817doi:10.26093/cds/vizier.35020817CDSAnders P.Lamers H.J.G.L.M.Baumgardt H.2009-10-16T14:02:31Z2009-10-16T13:55:33ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsphotometryEvolutionary synthesis models are the primary means of constructing spectrophotometric models of stellar populations, and deriving physical parameters from observations compared with these models. One of the basic assumptions of evolutionary synthesis models has been the time-independence of the stellar mass function, apart from the successive removal of high-mass stars by stellar evolution. However, dynamical simulations of star clusters in tidal fields have demonstrated that the mass function can be changed by the preferential removal of low-mass stars from clusters. We combine the results of dynamical simulations of star clusters in tidal fields with our evolutionary synthesis code GALEV. We extend the models to consider the total cluster disruption time as additional parameter.2009A&A...502..817Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/502/817CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/106/275 : Theoretical isochrones (Bertelli+ 1994)http://www.phys.uu.nl/~anders/data/SSP_varMF : Models Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/502/817https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/502/817http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/502/817https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/502/817https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/502/817http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/502/817GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/502/817/filelistList of all the model parameters (Z, tdis)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZInitial metallicity Z (1)phys.abund.Zfloat[Fe/H]Initial metallicity [Fe/H]phys.abund.ZfloattdisDissolution timescale (from 100Myr to 200Gyr)yrstat.paramdoubleMassName of the file with mass data in "mass" subdirectorymeta.id;meta.filecharMagName of the file with magnitudes in "mag" subdirectorymeta.id;meta.filechar