J/A+A/539/A119ivo://CDS.VizieR/J/A+A/539/A119doi:10.26093/cds/vizier.35390119CDSFang M.van Boekel R.King R.R.Henning T.Bouwman J.Doi Y.,Okamato Y.K.Roccatagliata V.Sicilia-Aguilar A.2017-06-30T05:47:55Z2012-03-05T15:29:09ZCDS support team

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

cds-question@unistra.fropen-star-clusterspre-main-sequence-starsx-ray-sourcesinfrared-photometryCircumstellar disks are expected to evolve quickly in massive young clusters harboring many OB-type stars. Two processes have been proposed to drive the disk evolution in such cruel environments: (1) gravitational interaction between circumstellar disks and nearby passing stars (stellar encounters), and (2) photoevaporation by UV photons from massive stars. The relative importance of both mechanisms is not well understood. Studies of massive young star clusters can provide observational constraints on the processes of driving disk evolution. We investigate the properties of young stars and their disks in the NGC 6357 complex, concentrating on the most massive star cluster within the complex: Pismis 24.2012A&A...539A.119Fhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/539/A119CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)J/ApJS/168/100 : X-ray study of star-forming region NGC 6357 (Wang+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/539/A119https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/539/A119http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/539/A119https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/539/A119https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/539/A119http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/539/A119GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/539/A119/Xstars (Photometric magnitudes and derived parameters for stars with X-ray emission in Pismis 24)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/539/A119/Xstars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/539/A119/Xstars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/539/A119/Xstars?GETtext/xml+votable180.050000true260.9747083-34.14736110.0055555555555555566/424622.483060040379131e-20 1.7003137259100215e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/539/A119?format=asciiX-rayInfrareddefaultJ/A+A/539/A119/XstarsPhotometric magnitudes and derived parameters for stars with X-ray emission in Pismis 24recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/643] Sequential numbermeta.recordintprimaryW07[1/778] Wang et al. 2007 (Cat. J/ApJS/168/100) number (<[WTF2007] NNN> in Simbad)meta.id;meta.mainintoffDistance between X-ray source and optical/infrared counterpartarcsecmeta.id.assoc;pos.angDistancefloatRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainRmag? VIMOS R magnitudemagphot.mag;em.opt.Rfloatnullablee_Rmag? rms uncertainty on Rmagmagstat.error;phot.mag;em.opt.RfloatnullableImag? VIMOS I magnitudemagphot.mag;em.opt.Ifloatnullablee_Imag? rms uncertainty on Imagmagstat.error;phot.mag;em.opt.IfloatnullableJmag? 2MASS J magnitudemagphot.mag;em.IR.Jfloatnullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JfloatnullableHmag? 2MASS H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HfloatnullableKsmag? 2MASS Ks magnitudemagphot.mag;em.IR.Kfloatnullablee_Ksmag? rms uncertainty on Ksmagmagstat.error;phot.mag;em.IR.Kfloatnullable[3.6]? IRAC 3.6um magnitudemagphot.mag;em.IR.3-4umfloatnullablee_[3.6]? rms uncertainty on [3.6]magstat.errorfloatnullable[4.5]? IRAC 4.5um magnitudemagphot.mag;em.IR.4-8umfloatnullablee_[4.5]? rms uncertainty on [4.5]magstat.errorfloatnullable[5.8]? IRAC 5.8um magnitudemagphot.flux.density;em.IR.4-8umfloatnullablee_[5.8]? rms uncertainty on [5.8]magstat.errorfloatnullable[8.0]? IRAC 8.0um magnitudemagphot.flux.density;em.IR.8-15umfloatnullablee_[8.0]? rms uncertainty on [8.0]magstat.errorfloatnullableSpTMK spectral typesrc.spTypecharAv? Absorption in V bandmagphot.mag;em.opt.VfloatnullableMass? MasssolMassphys.massfloatnullableAge? AgeMyrtime.agefloatnullable