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<ri:Resource created="2018-12-14T12:25:47Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>A large moving group within the LCC association</title><shortName>J/ApJ/868/32</shortName><identifier>ivo://CDS.VizieR/J/ApJ/868/32</identifier><altIdentifier>doi:10.26093/cds/vizier.18680032</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Goldman B.</name></creator><creator><name>Roser S.</name></creator><creator><name>Schilbach E.</name></creator><creator><name>Moor A.C.</name></creator><creator><name>Henning T.</name></creator><date role="Updated">2020-07-01T08:13:49Z</date><date role="Created">2018-12-14T12:25:47Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>young-stellar-objects</subject><subject>brown-dwarfs</subject><subject>stellar-associations</subject><subject>astrometry</subject><subject>stellar-masses</subject><subject>stellar-ages</subject><subject>effective-temperature</subject><subject>astronomical-object-identification</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Scorpius-Centaurus is the nearest OB association, and its hundreds of members are divided into subgroups, including the Lower Centaurus Crux (LCC). Here we study the dynamics of the LCC area. We report the revelation of a large moving group containing more than 1800 intermediate- and low-mass young stellar objects and brown dwarfs that escaped identification until Gaia DR2 allowed a kinematic and photometric selection to be performed. We investigate the stellar and substellar content of this moving group using the Gaia DR2 astrometric and photometric measurements. The median distance of the members is 114.5pc, and 80% lie between 102 and 135pc from the Sun. Our new members cover a mass range of 0.02-5M_{sun}_ and add up to a total mass of about 700M_{sun}_. The present-day mass function follows a log-normal law with m_c_=0.22M_{sun}_ and {sigma}=0.64. We find more than 200 brown dwarfs in our sample. The star formation rate had its maximum of 8x10^-5^M_{sun}_/yr about 9Myr ago. We grouped the new members into four denser subgroups, which have increasing age from 7 to 10Myr, surrounded by "free-floating" young stars with mixed ages. Our isochronal ages, now based on accurate parallaxes, are compatible with several earlier studies of the region. The whole complex is presently expanding, and the expansion started between 8 and 10Myr ago. Two hundred members show infrared excess compatible with circumstellar disks from full to debris disks. This discovery provides a large sample of nearby young stellar and substellar objects for disk and exoplanet studies.</description><source format="bibcode">2018ApJ...868...32G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/868/32</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/254">III/254 : 2nd Cat. of RVs with Astrometric Data (Kharchenko+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/153/257">J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/595/A22">J/A+A/595/A22 : 9 new open clusters within 500pc from the Sun (Roser+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/461/794">J/MNRAS/461/794 : Scorpius-Centaurus K-Type Stars (Pecaut+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/15">J/ApJS/225/15 : IR excess stars from Tycho-2 and AllWISE (Cotten+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/458/3479">J/MNRAS/458/3479 : SVM selection of WISE YSO Candidates (Marton+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/437/391">J/MNRAS/437/391 : IR excess in Sun-like stars with WISE (Cruz-Saenz+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A53">J/A+A/558/A53 : MW global survey of star clusters. 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(astrometric_pseudo_colour_error)</description><unit>um**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>fvarpi</name><description>[-0.4/0.4] Mean Parallax factor AL (mean_varpi_factor_al)</description><ucd>arith.factor;pos.parallax</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MatchObsA</name><description>[8/108] Matched FOV transits used in the AGIS solution (astrometric_matched_observations)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nper</name><description>[7/20] Number of visibility periods used in Astrometric solution (visibility_periods_used)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>amax</name><description>[0.03/0.9] The longest semi-major axis of the 5-d error ellipsoid (astrometric_sigma5d_max)</description><ucd>phys.angSize.smajAxis</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Vperp</name><description>[-2.4/2.1] Observed tangential velocity perpendicular to the convergent point direction (vperp)</description><unit>km/s</unit><ucd>phys.veloc.transverse</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>type</name><description>[0] The type of the source mainly used for frame rotation (0=ordinary source) (frame_rotator_object_type)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>MatchObs</name><description>[10/110] The total number of FOV transits matched to this source (matched_observations)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Dup</name><description>[0] Source with duplicate sources (false) (duplicated_source)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>o_Gmag</name><description>[81/946] Number of observations contributing to G photometry (phot_g_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_FG</name><description>[0.9/2.1e+06] FG error (phot_g_mean_flux_error)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RFG</name><description>[31/5654] G-band mean flux divided by its error (phot_g_mean_flux_over_error)</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Gmag</name><description>[3.8/18.7] G-band mean magnitude (Vega) (phot_g_mean_mag)</description><ucd>phot.mag;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>o_BPmag</name><description>[2/103] Number of observations contributing to BP photometry (phot_bp_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FBP</name><description>[38/4.3e+08] Mean flux in the integrated BP band (phot_bp_mean_flux)</description><ucd>phot.flux.density;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FBP</name><description>[3.9/1.2e+06] Error on FBP (phot_bp_mean_flux_error)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RFBP</name><description>[4/2465] Integrated BP mean flux divided by its error (phot_bp_mean_flux_over_error)</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>BPmag</name><description>[3.7/21.4] Integrated BP mean magnitude (Vega) (phot_bp_mean_mag)</description><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>o_RPmag</name><description>[2/103] Number of observations contributing to RP photometry (phot_rp_n_obs)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FRP</name><description>[1103/2e+08] Mean flux in the integrated RP band (phot_rp_mean_flux)</description><ucd>phot.flux.density;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_FRP</name><description>[5/577480] Error on FRP (phot_rp_mean_flux_error)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RFRP</name><description>[5/2173] Integrated RP mean flux divided by its error (phot_rp_mean_flux_over_error)</description><ucd>stat.fit.omc</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RPmag</name><description>[4/17.2] Integrated RP mean magnitude (Vega) (phot_rp_mean_mag)</description><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E(BR/RP)</name><description>[1.1/1.8] BP/RP excess factor (phot_bp_rp_excess_factor)</description><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mode</name><description>[0/1] Photometry processing mode (phot_proc_mode)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RV</name><description>[-29/34.1]? Spectroscopic radial velocity in the solar barycentric reference frame (radial_velocity)</description><unit>km/s</unit><ucd>phys.veloc;pos.barycenter</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_RV</name><description>[0.2/19.4]? Radial velocity error (radial_velocity_error)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_RV</name><description>[0/37] Number of transits used to compute radial velocity (rv_nb_transits)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Var</name><description>Photometric variability flag ("VARIABLE" = 36 occurrences) (phot_variable_flag)</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>GLON</name><description>[285.2/319] Galactic longitude (l)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>[-15.3/21.7] Galactic latitude (b)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>ELON</name><description>Ecliptic longitude (ecl_lon)</description><unit>deg</unit><ucd>pos.ecliptic.lon</ucd></column><column><name>ELAT</name><description>Ecliptic latitude (ecl_lat)</description><unit>deg</unit><ucd>pos.ecliptic.lat</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>fPriam</name><description>[100001/102002]? Flags for the Apsis-Priam results (priam_flags)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>TeffA</name><description>[3286/9705]? Stellar effective temperature (estimate from Apsis-Priam) (teff_val)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_TeffA</name><description>[3115/9534]? Uncertainty (lower) on TeffA (16th percentile) (teff_percentile_lower)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_TeffA</name><description>[3343/9947]? Uncertainty (upper) on TeffA (84th percentile) (teff_percentile_upper)</description><unit>K</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AG</name><description>[0.02/3]? Estimate of extinction in the G band from Apsis-Priam (a_g_val)</description><unit>mag</unit><ucd>phys.absorption</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_AG</name><description>[0/2.6]? Uncertainty (lower) on AG estimate from Apsis-Priam (16th percentile) (a_g_percentile_lower)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_AG</name><description>[0.06/3.2]? Uncertainty (upper) on AG estimate from Apsis-Priam (84th percentile) (a_g_percentile_upper)</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E(BP-RP)</name><description>[0.01/1.5]? Estimate of redenning E(BP-RP) from Apsis-Priam (e_bp_min_rp_val)</description><unit>mag</unit><ucd>phot.color.excess</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_E(BP-RP)</name><description>[0/1.3]? Uncertainty (lower) on E(BP-RP) estimate from Apsis-Priam (16th percentile) (e_bp_min_rp_percentile_lower)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_E(BP-RP)</name><description>[0.03/1.7]? Uncertainty (upper) on E(BP-RP) estimate from Apsis-Priam (84th percentile) (e_bp_min_rp_percentile_upper)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>fFLAME</name><description>[200111]? Flags for the Apsis-FLAME results (flame_flags)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Rad</name><description>[0.5/3]? Estimate of radius from Apsis-FLAME (radius_val)</description><unit>solRad</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Rad</name><description>[0.3/3]? Uncertainty (lower) on radius estimate from Apsis-FLAME (16th percentile) (radius_percentile_lower)</description><unit>solRad</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Rad</name><description>[0.5/3.1]? Uncertainty (upper) on radius estimate from Apsis-FLAME (84th percentile) (radius_percentile_upper)</description><unit>solRad</unit><ucd>stat.error;phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lum</name><description>[0.03/26]? Esimate of luminosity from Apsis-FLAME (lum_val)</description><unit>solLum</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>b_Lum</name><description>[0.03/25.8]? Uncertainty (lower) on luminosity estimate from Apsis-FLAME (16th percentile) (lum_percentile_lower)</description><unit>solLum</unit><ucd>stat.error;phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>B_Lum</name><description>[0.03/26.3]? Uncertainty (upper) on luminosity estimate from Apsis-FLAME (84th percentile) (lum_percentile_upper)</description><unit>solLum</unit><ucd>stat.error;phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RVpred</name><description>[5.5/16.7] Predicted radial velocity (vr_pred)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vpar</name><description>[18.3/21.5] Observed tangential velocity toward the convergent point (vpar)</description><unit>km/s</unit><ucd>phys.veloc.transverse</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vpar</name><description>[0.05/1.3] Uncertainty on the observed tangential velocity toward the convergent point (e_vpar)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Vperp</name><description>[0.01/0.5] Uncertainty on the observed tangential velocity perpendicular to the convergent point direction (e_vper)</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vppcor</name><description>[-0.9/0.8] Correlation between the observed tangential velocities toward and perpendicular to the convergent point direction (vparvperpcor)</description><ucd>stat.correlation</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Xgal</name><description>[26/103] X galactic coordinate derived from Gaia DR2 parameters (x_gal)</description><unit>pc</unit><ucd>pos.cartesian.x;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ygal</name><description>[-134.1/-64.6] Y galactic coordinate derived from Gaia DR2 parameters (y_gal)</description><unit>pc</unit><ucd>pos.cartesian.y;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Zgal</name><description>[-30.7/51] Z galactic coordinate derived from Gaia DR2 parameters (z_gal)</description><unit>pc</unit><ucd>pos.cartesian.z;pos.galactic</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>AgeC</name><description>[0.001/0.1]? Age according to the CIFIST isochrones (age_CIFIST)</description><unit>Gyr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>MassC</name><description>[0.02/1.4]? Mass according to the CIFIST isochrones (Mass_CIFIST)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TeffC</name><description>[2632/6766]? Effective temperature according to the CIFIST isochrones (Teff_CIFIST)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logLumC</name><description>[-3/0.6]? log_10 of bolometric luminosity according to the CIFIST isochrones (Lum_CIFIST)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>loggC</name><description>[3.4/5]? log_10 of gravity according to the CIFIST isochrones (logg_CIFIST)</description><unit>log(g.cm**-1.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>AgeP</name><description>[5e+06/1e+08] Age according to the Parsec isochrones (Age_P)</description><unit>yr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MassP</name><description>[0.1/5.4] Initial mass according to the Parsec isochrones (mass_P)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logLumP</name><description>[-2.7/3.1] log_10 of bolometric luminosity according to the Parsec isochrones (logL_P)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logTeffP</name><description>[3.4/4.3] log_10 of effective temperature according to the Parsec isochrones (logTe_P)</description><unit>log(K)</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>loggP</name><description>[3.7/4.8] log_10 of gravity according to the Parsec isochrones (logg_P)</description><unit>log(g.cm**-1.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RecovR</name><description>[0.6/1] Fraction of recovered stars of same G magnitude (recovery_rate)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>[0.001/0.11] Best age (Age)</description><unit>Gyr</unit><ucd>time.age;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Mass</name><description>[0.02/5.4] Best mass (Mass)</description><unit>solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Teff</name><description>[2632/16726] Best effective temperature (Teff)</description><unit>K</unit><ucd>phys.temperature.effective;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>LogLum</name><description>[-3/3.1] log_10 of best bolometric luminosity (LogL)</description><unit>log(solLum)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WISEA</name><description>ID of AllWISE detection (JHHMMSS.ss+DDMMSS.s) (AllWISE_ID)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>logLSED</name><description>[-3.8/590]? log_10 of bolometric luminosity according to the VOSA fit, used for the circumstellar disk analysis (LogL_SED)</description><unit>log(g.cm**-1.s**-2)</unit><ucd>phys.luminosity</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>TeffSED</name><description>[1200/18000]? Effective temperature according to the VOSA fit, used for the circumstellar disk analysis (Teff_SED)</description><unit>K</unit><ucd>phys.temperature.effective;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>DkType</name><description>Circumstellar disk classification (disk_type)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="20*">char</dataType></column><column><name>SName</name><description>Primary SIMBAD name (Simbad_name)</description><ucd>meta.id.cross</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Ref</name><description>? Reference for circumstellar disk (Ref) (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) at Epoch=J2000, proper motions taken into account</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table></schema></tableset></ri:Resource>