J/ApJ/895/126ivo://CDS.VizieR/J/ApJ/895/126doi:10.26093/cds/vizier.18950126CDSHendler N.Pascucci I.Pinilla P.Tazzari M.Carpenter J.Malhotra R.,Testi L.2022-03-10T07:12:38Z2021-10-07T07:54:46ZCDS support team

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

cds-question@unistra.fropen-star-clusterspre-main-sequence-starseffective-temperaturestellar-massesstellar-radiiinfrared-astronomyWe utilize ALMA archival data to estimate the dust disk size of 152 protoplanetary disks in Lupus (1-3Myr), Chamaeleon I (2-3Myr), and Upper-Sco (5-11Myr). We combine our sample with 47 disks from Tau/Aur and Oph whose dust disk radii were estimated, as here, through fitting radial profile models to visibility data. We use these 199 homogeneously derived disk sizes to identify empirical disk-disk and disk-host property relations as well as to search for evolutionary trends. In agreement with previous studies, we find that dust disk sizes and millimeter luminosities are correlated, but show for the first time that the relationship is not universal between regions. We find that disks in the 2-3Myr old ChaI are not smaller than disks in other regions of similar age, and confirm the Barenfeld et al. finding that the 5-10Myr USco disks are smaller than disks belonging to younger regions. Finally, we find that the outer edge of the solar system, as defined by the Kuiper Belt, is consistent with a population of dust disk sizes which have not experienced significant truncation.2020ApJ...895..126Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/895/126CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)J/AJ/124/404 : Upper Scorpius OB association Li survey. II. (Preibisch, 2002)J/AJ/130/1733 : Optical spectroscopy of {rho} Oph stars (Wilking+, 2005)J/ApJ/675/1375 : IRAC/MIPS photometry in Cha I (Luhman+, 2008)J/ApJS/177/551 : Spitzer c2d survey of Lupus dark clouds (Merin+, 2008)J/ApJ/688/377 : Low-mass objects in Upper Scorpius. II. (Slesnick+, 2008)J/ApJ/746/154 : Improved kinematic parallaxes Sco-Cen members (Pecaut+, 2012)J/ApJ/771/129 : Submillimetric Class II sources of Taurus (Andrews+, 2013)J/A+A/561/A2 : 36 accreting YSOs emission lines (Alcala+, 2014)J/ApJ/828/46 : ALMA survey of Lupus protoplanetary disks. I. (Ansdell+, 2016)J/ApJ/827/142 : ALMA observations of GKM stars in Upper Sco (Barenfeld+, 2016)J/ApJ/831/125 : ALMA 887{mu}m obs. ChaI star-forming region (Pascucci+, 2016)J/A+A/602/A33 : X-Shooter spectroscopy of YSOs in Lupus (Frasca+, 2017)J/A+A/601/A97 : Gaia-ESO Survey: Cha I members (Sacco+, 2017)J/ApJ/845/44 : 340GHz SMA obs. 50 nearby protoplanetary disk (Tripathi+,2017)J/ApJ/869/L41 : DSHARP I. Sample, ALMA obs. log and overview (Andrews+, 2018)J/ApJ/869/L42 : DSHARP. II. Annular substructures data (Huang+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/895/126https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/895/126http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/895/126https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/895/126https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/895/126http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/895/126GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/895/126/table10 (Modeling parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/895/126/table10?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/895/126/table10?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/895/126/table10?GETtext/xml+votable180.050000true163.4156719-77.20942890.0055555555555555565/9239 11091 11094 6/36946 37122 37128-37129 42597-42599 42605 42611 42614-42615 42704-42705 42714 42727 42736-42737 42943 42979 42984 42990 43001 44118 44317 44343 44352 44355-44356 44358 44360-44361 44363 44369 44371 44386 44389 44400-44401https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/895/126?format=asciiInfrareddefaultJ/ApJ/895/126/table10Modeling parametersalpha[1.98/83.89] Transition indexstat.fit.paramfloati[3.67/77.72] Inclinationdegsrc.orbital.inclinationfloat2MASS2MASS identifiermeta.id;meta.maincharprimaryl_R68Limit flag on R68meta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintR68[0.06/0.82] Radius containing 68% of the fluxarcsecphys.size.radiusfloatE_R68[0.0/0.84]? Upper uncertainty in R68arcsecstat.error;stat.maxfloatnullablee_R68[0.0/0.57]? Lower uncertainty in R68arcsecstat.errorfloatnullablel_R60Limit flag on R60meta.code.errorcharR60[0.07/1.37] Radius containing 60% of the fluxarcsecphys.size.radiusfloatE_R60[0.0/1.29]? Upper uncertainty in R60arcsecstat.error;stat.maxfloatnullablee_R60[0.0/0.7]? Lower uncertainty in R60arcsecstat.errorfloatnullableRt[0.05/1.11] Transition radiusarcsecphys.size.radiusfloatE_Rt[0.0/0.91] Upper uncertainty in Rtarcsecstat.error;stat.maxfloate_Rt[0.0/0.66] Lower uncertainty in Rtarcsecstat.errorfloatf0[5.23/11.47] Amplitude coefficientJy/srstat.fit.paramfloatE_f0[0.01/3.63] Upper uncertainty in f0Jy/srstat.error;stat.maxfloate_f0[0.01/5.12] Lower uncertainty in f0Jy/srstat.errorfloatE_alpha[2.74/68.11] Upper uncertainty in alphastat.error;stat.maxfloate_alpha[0.4/53.55] Lower uncertainty in alphastat.error;pos.eq.rafloatbeta[1.25/14.38] Outer cutoff indexstat.fit.paramfloatE_beta[0.2/9.58] Upper uncertainty in betastat.error;stat.maxfloate_beta[0.16/7.37] Lower uncertainty in betastat.errorfloatgamma[-6.16/0.5] Inner cutoff indexstat.fit.paramfloatE_gamma[0.01/4.88] Upper uncertainty in gammastat.error;stat.maxfloate_gamma[0.01/4.96] Lower uncertainty in gammastat.errorfloatE_i[0.6/46.25] Upper uncertainty in degdegstat.error;stat.maxfloate_i[0.53/44.6] Lower uncertainty in degdegstat.errorfloatPosAng[-16.22/209.14] Position angledegpos.posAngfloatE_PosAng[0.52/103.18] Upper uncertainty in PosAngdegstat.error;stat.maxfloate_PosAng[0.57/87.7] Lower uncertainty in PosAngdegstat.errorfloatdDE[-1.73/1.82] Declination offsetarcsecpos;arith.difffloatE_dDE[0.0/1.9] Upper uncertainty in dDEarcsecstat.error;stat.maxfloate_dDE[0.0/1.88] Lower uncertainty in dDEarcsecstat.errorfloatdRA[-1.58/1.82] Right Ascension offsetarcsecpos;arith.difffloatE_dRA[0.0/2.0] Upper uncertainty in dRAarcsecstat.error;stat.maxfloate_dRA[0.0/2.03] Lower uncertainty in dRAarcsecstat.errorfloatlnwcorr[-4.47/-0.47] Natural log fitted weight correction factorinstr.paramfloatE_lnwcorr[0.0/0.02] Upper uncertainty in lnwcorrstat.error;stat.maxfloate_lnwcorr[0.0/0.01] Lower uncertainty in lnwcorrstat.errorfloatPropIndicates that stellar and disk properties arre available (table7)meta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPosition from SIMBAD (right ascension part)degpos.eq.ra;meta.main_DEPosition from SIMBAD (declination part)degpos.eq.dec;meta.mainJ/ApJ/895/126/table7Stellar and disk propertiesE_Teff[0.0/241.7]? Upper uncertainty in TeffKstat.error;stat.maxfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint2MASS2MASS identifiermeta.id;meta.maincharRegionRegion identifiermeta.id;obs.fieldcharDist[94.4/208.26] Distancepcpos.distancefloatE_Dist[0.65/31.0] Upper uncertainty in Distpcstat.error;stat.maxfloate_Dist[0.64/20.0] Lower uncertainty in Distpcstat.errorfloatlogL*[-2.52/0.71] log stellar luminositysolLumphys.luminosityfloatE_logL*[0.0/2.98] Upper uncertainty in logL*solLumstat.error;stat.maxfloate_logL*[0.0/2.98] Lower uncertainty in logL*solLumstat.errorfloatTeff[2935/5623.41] Effective temperatureKphys.temperature.effectivefloate_Teff[0.0/230.83]? Lower uncertainty in TeffKstat.error;phys.temperature.effectivefloatnullablelogM*[-1.13/0.67] log stellar masssolMassphys.massfloatE_logM*[0.02/0.97] Upper uncertainty in logM*solMassstat.error;stat.maxfloate_logM*[0.02/0.88] Lower uncertainty in logM*solMassstat.errorfloatLmm[0.58/784.48] The mm luminosity (1)mJyphys.luminosityfloatE_Lmm[0.14/86.39] Upper uncertainty in LmmmJystat.error;stat.maxfloate_Lmm[0.14/77.52] Lower uncertainty in LmmmJystat.errorfloat