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<ri:Resource created="2024-01-09T07:11:47Z" status="active" updated="2025-06-13T15:25:00Z" 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>TW Hya association candidate members</title><shortName>J/AJ/165/269</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/269</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Luhman K.L.</name></creator><date role="Updated">2024-01-26T06:26:20Z</date><date role="Created">2024-01-09T07:11:47Z</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>stellar-associations</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>infrared-photometry</subject><subject>stellar-spectral-types</subject><subject>proper-motions</subject><subject>trigonometric-parallax</subject><description>I have used high-precision photometry and astrometry from the third data release of Gaia to perform a survey for members of the TW Hya association (TWA). I have identified candidate members that appear to share similar kinematics and ages with bona fide members compiled by Gagne et al. (2017), and I have assessed their membership using radial velocities and spectroscopic diagnostics of age from various sources. My new catalog of adopted members contains 67 Gaia sources in 55 systems. The histogram of spectral types for TWA peaks near M5 (~0.15M{sun}), resembling the distributions measured for other nearby young associations. The UVW velocities of its members indicate that the association is expanding. The rate of expansion corresponds to an age of 9.6_-0.8_^+0.9^Myr. In a Gaia color-magnitude diagram, the members of TWA exhibit well-defined sequences of single stars and unresolved binary stars. The combined sequence of low-mass stars in TWA is indicative of an age of 11.4_-1.2_^+1.3^Myr when compared to the sequence for Upper Centaurus Lupus/Lower Centaurus Crux, for which an age of 20Myr is assumed. Based on these expansion and isochronal ages, I have adopted an age of 10{+/-}2Myr for TWA. Finally, I have used mid-infrared photometry from the Wide-field Infrared Survey Explorer to check for excess emission from circumstellar disks among the TWA members. Fourteen members have detected disks, all of which have been reported in previous studies. The fraction of members at &lt;~M6&gt;~0.1M{sun}) that have full, transitional, or evolved disks is 10/52=0.19_-0.06_^+0.08^. That value is similar to the fraction previously measured for the Upper Sco association, which is roughly coeval with TWA.</description><source format="bibcode">2023AJ....165..269L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/269</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/III/135">III/135 : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/352">I/352 : Distances to 1.47 billion stars in Gaia EDR3 (Bailer-Jones+, 2021)</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/ApJS/99/135">J/ApJS/99/135 : Rotation and Spectral Peculiarities (Abt+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/525/466">J/ApJ/525/466 : Young low-mass stars &amp; brown dwarfs in IC348 (Luhman+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/ARA+A/42.685">J/other/ARA+A/42.685 : Young stars near the Sun (Zuckerman+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/620/1010">J/ApJ/620/1010 : Spitzer 24{mu}m photometry of A dwarfs (Rieke+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/132/866">J/AJ/132/866 : New M dwarfs in solar neighborhood (Riaz+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/460/695">J/A+A/460/695 : Search Associations Containing Young stars (Torres+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/662/1067">J/ApJ/662/1067 : Sptizer observations of sigma Orionis (Hernandez+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1290">J/AJ/136/1290 : Ultracool dwarfs from the 2MASS (Reid+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/111">J/ApJS/186/111 : Spitzer observations of Taurus members (Luhman+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/517/A76">J/A+A/517/A76 : Near-IR spectrum of 2M1207b (Patience+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/758/31">J/ApJ/758/31 : IR photometry for members of Upper Sco (Luhman+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/551/A107">J/A+A/551/A107 : Xshooter spectra of 24 young stellar objects (Manara+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/208/9">J/ApJS/208/9 : Intrinsic colors &amp; temperatures of PMS stars (Pecaut+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A127">J/A+A/562/A127 : NIR integral field spectra of 15 M-Ldwarfs (Bonnefoy+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A26">J/A+A/568/A26 : SACY. 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V component of space velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_V</name><description>[0.01/6.05]? Error in V</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W</name><description>[-11.3/-0.37]? W component of space velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W</name><description>[0.01/2.91]? Error in W</description><unit>km/s</unit><ucd>stat.error;pos.cartesian.z</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Gmag</name><description>[5.42/20.6] Gaia DR3 G magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Gmag</name><description>[0.003/0.07] Error in Gmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GBPmag</name><description>[5.44/21.7]? Gaia DR3 GBP magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_GBPmag</name><description>[0.003/0.3]? Error in GBPmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>GRPmag</name><description>[5.35/19]? Gaia DR3 GRP magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_GRPmag</name><description>[0.004/0.3]? Error in GRPmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>RUWE</name><description>[0.87/10.5]? Gaia DR3 renormalized unit weight error</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>2M</name><description>Closest 2MASS source within 3 arcsec</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>2Msep</name><description>[0.01/2]? Angular separation between Gaia DR3 (epoch 2000) and 2MASS</description><unit>arcsec</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>2Mclose</name><description>Is this Gaia source the closest match for the 2MASS source?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>wise</name><description>Closest WISE source within 3 arcsec</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="25*">char</dataType></column><column><name>Hmag</name><description>[5.352/14.608]? 2MASS H magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Hmag</name><description>[0.022/0.067]? Error in Hmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Ksmag</name><description>[5.235/14.04]? 2MASS Ks magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.K</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ksmag</name><description>[0.017/0.06]? Error in Ksmag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W1mag</name><description>[5.212/13.64]? WISE W1 magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W1mag</name><description>[0.022/0.079]? Error in W1mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>W2mag</name><description>[4.996/13.204]? WISE W2 magnitude</description><unit>mag</unit><ucd>phot.mag;em.IR.4-8um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W2mag</name><description>[0.019/0.054]? Error in W2mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W2mag</name><description>Flag on W2mag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>W3mag</name><description>[3.11/11.785]? WISE W3 magnitude</description><unit>mag</unit><ucd>phot.flux.density;em.IR.8-15um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W3mag</name><description>[0.013/0.212]? Error in W3mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W3mag</name><description>Flag on W3mag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>W4mag</name><description>[0.202/8.853]? WISE W4 magnitude</description><unit>mag</unit><ucd>phot.flux.density;em.IR.15-30um</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_W4mag</name><description>[0.009/0.404]? Error in W4mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_W4mag</name><description>Flag on W4mag (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>ExcW2</name><description>? Excess present in W2?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ExcW3</name><description>? Excess present in W3?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ExcW4</name><description>? Excess present in W4?</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>DiskType</name><description>? Disk Type (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>bfmem</name><description>Bona fide member of TWA (Gagne et al. 2017)</description><ucd>meta.code.member</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>outlier</name><description>Spatial outlier</description><ucd>meta.cryptic</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>New</name><description>New spectral classification (table1)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/AJ/165/269/figure3</name><description>Combined table from original tables</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Gaia</name><description>Gaia DR3 identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>lambda</name><description>Wavelength ({AA})</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F7500</name><description>Flux ratio (F{lambda}/F7500{AA})</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/AJ/165/269/refs</name><description>References used</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>[1/51] Reference code</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Author</name><description>Main author (et al.)</description><ucd>meta.bib.author</ucd><dataType xsi:type="vs:VOTableType" arraysize="21*">char</dataType></column><column><name>BIB</name><description>BIBcode</description><ucd>meta.bib.bibcode</ucd><dataType xsi:type="vs:VOTableType" arraysize="19*">char</dataType></column><column><name>Cat.</name><description>Catalog in VizieR</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>Note</name><description>Additional note</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column></table></schema></tableset></ri:Resource>