J/A+A/537/A105ivo://CDS.VizieR/J/A+A/537/A105doi:10.26093/cds/vizier.35370105CDSGullieuszik M.Groenewegen M.A.T.Cioni M.-R.L.de Grijs R.,van Loon J.T.Girardi L.Ivanov V.D.Oliveira J.M.Emerson J.P.,Guandalini R.2023-12-21T16:01:50Z2012-01-17T07:56:21ZCDS support team

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

cds-question@unistra.frmagellanic-cloudsgiant-starscarbon-starsstellar-mass-lossAsymptotic giant branch (AGB) stars are major contributors to both the chemical enrichment of the interstellar medium and the integrated light of galaxies. Despite its importance, the AGB is one of the least understood phases of stellar evolution. The main difficulties associated with detailed modelling of the AGB are related to the mass-loss process and the 3rd dredge-up efficiency. We provide direct measures of mass-loss rates and luminosities for a complete sample of AGB stars in the Large Magellanic Cloud, disentangling the C- and O-rich stellar populations.2012A&A...537A.105Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/537/A105CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/348/98 : LMC AGB stars IRAS fluxes (Reid+ 1990)J/A+A/506/1277 : Modelisation of Magellanic Cloud C/O stars (Groenewegen+ 2009)J/A+A/530/A90 : Optically bright post-AGB population of LMC (van Aarle+, 2011)J/A+A/531/A157 : VMC. II. LMC planetary nebulae (Miszalski+, 2011)J/AJ/128/1606 : Magellanic Clouds Photometric Survey: the LMC (Zaritsky+ 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/537/A105https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/537/A105http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/537/A105https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/537/A105https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/537/A105http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/537/A105GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/537/A105/results (Parameters of best-fitting models for all AGB candidates (table2))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/537/A105/results?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/537/A105/results?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/537/A105/results?GETtext/xml+votable180.050000true75.5035833-65.386750.0055555555555555565/8281 6/33136 331386.772611666688002e-21 6.118840631666147e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/537/A105?format=asciidefaultJ/A+A/537/A105/resultsParameters of best-fitting models for all AGB candidates (table2)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/374] Sequential numbermeta.recordintprimaryRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.maintau? Optical depth at 0.55 micronphys.absorption.opticalDepthfloatnullablelogMdot? Logarithmic mass-loss ratelog(solMass.yr**-1)arith.ratefloatnullableLum? LuminositysolLumphys.luminosityintnullableClObject Classification (1)src.classcharQ[BSU] Quality Flag, as B=bad fits, S=secure, U=uncertain classificationmeta.code.class;src.class.starGalaxy;meta.fitscharPmeta.ref.urlcharSEDPlot of the SED (optical + IR)meta.ref.urlcharJ/A+A/537/A105/photomPhotometry of sources classified as AGB stars (table6)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/374] Sequential numbermeta.recordintUmag? MCPS U magnitude (J/AJ/128/1606)magphot.mag;em.opt.UfloatnullableBmag? MCPS B magnitude (J/AJ/128/1606)magphot.mag;em.opt.BfloatnullableVmag? MCPS V magnitude (J/AJ/128/1606)magphot.mag;em.opt.VfloatnullableImag? MCPS I magnitude (J/AJ/128/1606)magphot.mag;em.opt.IfloatnullableYmagV? VMC Y magnitudemagphot.mag;em.opt.IfloatnullableJmagV? VMC J magnitudemagphot.mag;em.IR.JfloatnullableKsmagV? VMC Ks magnitudemagphot.mag;em.IR.KfloatnullableJmag22MASS J magnitudemagphot.mag;em.IR.JfloatHmag22MASS H magnitudemagphot.mag;em.IR.HfloatKsmag22MASS Ks magnitudemagphot.mag;em.IR.Kfloat[3.6]1? Spitzer/IRAC 3.6um from SAGE 1st epochmagphot.mag;em.IR.3-4umfloatnullable[3.6]2? Spitzer/IRAC 3.6um from SAGE 2nd epochmagphot.mag;em.IR.3-4umfloatnullable[4.5]1? Spitzer/IRAC 4.5um from SAGE 1st epochmagphot.mag;em.IR.4-8umfloatnullable[4.5]2? Spitzer/IRAC 4.5um from SAGE 2nd epochmagphot.mag;em.IR.4-8umfloatnullable[5.8]1? Spitzer/IRAC 5.8um from SAGE 1st epochmagphot.flux.density;em.IR.4-8umfloatnullable[5.8]2? Spitzer/IRAC 5.8um from SAGE 2nd epochmagphot.flux.density;em.IR.4-8umfloatnullable[8.0]1? Spitzer/IRAC 8.0um from SAGE 1st epochmagphot.flux.density;em.IR.8-15umfloatnullable[8.0]2? Spitzer/IRAC 8.0um from SAGE 2nd epochmagphot.flux.density;em.IR.8-15umfloatnullable[24]1? Spitzer/MIPS 24um from SAGE 1st epochmagphot.flux.density;em.IR.15-30umfloatnullable[24]2? Spitzer/MIPS 24um from SAGE 2nd epochmagphot.flux.density;em.IR.15-30umfloatnullablechi2CReduced {chi}^2^ for best-fitting C-rich modelstat.fit.chi2floatchi2OReduced {chi}^2^ for best-fitting O-rich modelstat.fit.chi2float