J/ApJ/552/289ivo://CDS.VizieR/J/ApJ/552/289doi:10.26093/cds/vizier.15520289CDSAlard C.Blommaert J.A.D.L.Cesarsky C.Epchtein N.Felli M.Fouque P.,Ganesh S.Genzel R.Gilmore G.Glass I.S.Habing H.Omont A.,Perault M.Price S.Robin A.Schultheis M.Simon G.van Loon J.T.,Alcock C.Allsman R.A.Alves D.R.Axelrod T.S.Becker A.C.,Bennett D.P.Cook K.H.Drake A.J.Freeman K.C.Geha M.Griest K.,Lehner M.J.Marshall S.L.Minniti D.Nelson C.Peterson B.A.,Popowski P.Pratt M.R.Quinn P.J.Sutherland W.Tomaney A.B.,Vandehei T.Welch D.L.2018-01-05T08:56:22Z2001-12-31T15:57:40ZCDS support team

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

cds-question@unistra.frvariable-starsphotometrystellar-mass-losseffective-temperatureinfrared-photometryBy cross-correlating the results of two recent large-scale surveys, the general properties of a well-defined sample of semiregular variable stars have been determined. ISOGAL mid-infrared photometry (7 and 15{mu}m and MACHO V and R light curves are assembled for approximately 300 stars in the Baade's windows of low extinction toward the Galactic bulge. These stars are mainly giants of late M spectral type, evolving along the asymptotic giant branch (AGB). They are found to possess a wide and continuous distribution of pulsation periods and to obey an approximate logP-M_bol_ relation or set of such relations.2001ApJ...552..289Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/552/289CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-tohttp://wwwmacho.anu.edu.au/ : The MACHO Project Home Pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/552/289https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/552/289http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/552/289https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/552/289https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/552/289http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/552/289GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/552/289/table1 (Summarized photometry of sources)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/552/289/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/552/289/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/552/289/table1?GETtext/xml+votable180.050000true269.66875-29.0633330.0055555555555555566/28778 28864https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/552/289?format=asciiOpticalInfrareddefaultJ/ApJ/552/289/table1Summarized photometry of sourcesn_ISOGALPNotes on ISOGALP (4)meta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintISOGALPThe full ISOGAL designation (1)meta.idcharBWRunning number during analyses of the Sgr I and NGC6522 fields (G1)meta.idintprimaryMACHOThe MACHO identifier (2)meta.id;meta.maincharprimaryVmagFlux-weighted time-averaged V band magnitudemagphot.mag;em.opt.Vfloatu_Vmag[:] Indicates a by-eye estimate in Vmag (3)meta.code.errorcharRmagFlux-weighted time-averaged R band magnitudemagphot.mag;em.opt.Rfloatu_Rmag[:] Indicates a by-eye estimate in Rmag (3)meta.code.errorcharJmag? The J_0_ band magnitudemagphot.mag;em.IR.JfloatnullableKmag? The K_0_ band magnitudemagphot.mag;em.IR.Kfloatnullable7magMagnitude in the 7 micron bandmagphot.flux.density;em.IR.4-8umfloat15magMagnitude in the 15 micron bandmagphot.flux.density;em.IR.8-15umfloatAmp? The optical pulsation amplitudemagsrc.var.amplitude;em.optfloatnullableLogP? Log of the periodlog(d)time.periodfloatnullableu_LogP[:] Indicates a by-eye estimate in LogPmeta.code.errorchar_RASimbad column added by the CDSdegpos.eq.ra;meta.main_DESimbad column added by the CDSdegpos.eq.dec;meta.mainJ/ApJ/552/289/table2Mira variables in the survey areaComComments (2)meta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintClusterCluster namemeta.id.parentcharTLETLE number (Frogel & Whitford, 1987ApJ...320..199F, TLE NGC 6522 NNN in Simbad)meta.idcharMACHOMACHO designationmeta.id;meta.maincharn_MACHO[M] M: "missing" (1)meta.notechar[7]magAverage [7] magnitude ([7]=12.38-2.5logF_LW2_(mJy))magphot.flux.density;em.IR.4-8umfloat[15]magMagnitude [15] ([[15]=10.79-2.5logF_LW3(mJy))magphot.flux.density;em.IR.8-15umfloatKmagAverage K magnitudemagphot.mag;em.IR.KfloatPer1? MACHO perioddtime.periodintnullablePer2? Lloyd Evans (1976MNRAS.174..169L) perioddtime.periodintnullableu_Per2Uncertainty flag on Per2meta.code.errorcharJ/ApJ/552/289/table3Spectral energy distribution modeling resultsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBWBW number (G1)meta.idintMACHOMACHO designationmeta.id;meta.maincharFW87? Frogel & Whitford (1987ApJ...320..199F) designation (1)meta.idcharMbolBolometric magnitudemagphys.magAbs.bolfloatT(V-K)Effective temperature calculated from dereddened (V-K)0 color and calibration of Bessell et al. (1998, Cat. <J/A+A/333/231>)Kphys.temperature.effective;meta.modelledintTmodBest-fit input model spectrum temperatureKstat.fit.paramintdM/dtL4Mass-loss rate normalised to a luminosity of L=10^4^L_{sun}_phys.mass.lossfloatdM/dtTrue mass-lossmeta.notefloatEF15umExcess of 15{mu}m fluxmJyphot.color.excessfloatVexpExpansion velocity corrected for a factor of (L/10^4^L_{sun}_)^1/4^km/sphys.veloc.expansionfloat