J/A+A/361/641ivo://CDS.VizieR/J/A+A/361/641doi:10.26093/cds/vizier.33610641CDSWinters J.M.Le Bertre T.Jeong K.S.Helling C.Sedlmayr E.2000-10-14T22:01:02Z2000-10-14T22:00:41ZCDS support team

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

cds-question@unistra.frvariable-starsstellar-mass-lossastronomical-modelsstellar-atmospheresIn order to investigate the relations between the mass loss from pulsating red giants and quantities which can be obtained from observations, we have explored the behavior of theoretical models which treat the time-dependent hydrodynamics of circumstellar outflows, including a detailed treatment of the dust formation process. This approach, while ignoring effects such as a possible non-sphericity of the stellar atmospheres which are difficult to assess, accounts correctly for factors such as the grain formation and destruction which are crucial to the mass-loss mechanism. We built a grid of ~150 models covering a wide range of physical situations. This grid allows us to characterize the effects of different parameters, such as the stellar luminosity and temperature, the period and the amplitude of the pulsation, and the C/O element abundance ratio, on the behavior of AGB winds and on the rates of mass loss. We find two regimes for the stellar outflows.2000A&A...361..641Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/361/641CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/361/641https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/361/641http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/361/641https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/361/641https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/361/641http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/361/641GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/361/641/table2Parameters and resultant quantities of the modelsDvpPulsation amplitudekm/ssrc.var.amplitudefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintModelModel name (1)meta.id;stat.fitM*Stellar masssolMassphys.massfloatL*Stellar luminosity10000solLumphys.luminosityfloatT*Stellar temperatureKphys.temperatureintC/OCarbon-to-oxygen ratiophys.abundfloatPPulsation perioddtime.periodint<dM/dt>? Average mass loss ratesolMass/yrphys.mass.lossfloatnullablee_<dM/dt>? Relative standard deviation of dM/dtstat.errorfloatnullable<v{inf}>? Average outflow velocitykm/sphys.veloc.expansionfloatnullableDust/Gas? Average dust-to-gas mass ratiophys.mass;arith.ratiofloatnullableK-L'? Average K-L' color indexphot.color;em.IR.K;em.IR.3-4umfloatnullableTypeType of model (2)meta.id;stat.fitchar