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<ri:Resource created="2019-07-10T13:50:05Z" 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>GOBELINS. IV. VLBA obs. of Taurus</title><shortName>J/ApJ/859/33</shortName><identifier>ivo://CDS.VizieR/J/ApJ/859/33</identifier><altIdentifier>doi:10.26093/cds/vizier.18590033</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Galli P.A.B.</name></creator><creator><name>Loinard L.</name></creator><creator><name>Ortiz-Leon G.N.</name></creator><creator><name>Kounkel M.</name></creator><creator><name>Dzib S.A.,Mioduszewski A.J.</name></creator><creator><name>Rodriguez L.F.</name></creator><creator><name>Hartmann L.</name></creator><creator><name>Teixeira R.</name></creator><creator><name>Torres R.M.,Rivera J.L.</name></creator><creator><name>Boden A.F.</name></creator><creator><name>Evans II N.J.</name></creator><creator><name>Briceno C.</name></creator><creator><name>Tobin J.J.</name></creator><creator><name>Heyer M.</name></creator><date role="Updated">2020-02-14T07:44:33Z</date><date role="Created">2019-07-10T13:50:05Z</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>star-forming-regions</subject><subject>radio-sources</subject><subject>proper-motions</subject><subject>visible-astronomy</subject><subject>trigonometric-parallax</subject><subject>stellar-distance</subject><subject>young-stellar-objects</subject><subject>molecular-clouds</subject><description>We present new trigonometric parallaxes and proper motions of young stellar objects in the Taurus molecular cloud complex from observations collected with the Very Long Baseline Array as part of the Gould's Belt Distances Survey. We detected 26 young stellar objects and derived trigonometric parallaxes for 18 stars with an accuracy of 0.3% to a few percent. We modeled the orbits of six binaries and determined the dynamical masses of the individual components in four of these systems (V1023 Tau, T Tau S, V807 Tau, and V1000 Tau). Our results are consistent with the first trigonometric parallaxes delivered by the Gaia satellite and reveal the existence of significant depth effects. We find that the central portion of the dark cloud Lynds 1495 is located at d=129.5+/-0.3pc, while the B216 clump in the filamentary structure connected to it is at d=158.1+/-1.2pc. The closest and remotest stars in our sample are located at d=126.6+/-1.7pc and d=162.7+/-0.8pc, yielding a distance difference of about 36pc. We also provide a new distance estimate for HL Tau that was recently imaged. Finally, we compute the spatial velocity of the stars with published radial velocity and investigate the kinematic properties of the various clouds and gas structures in this region.</description><source format="bibcode">2018ApJ...859...33G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/859/33</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/B/wds">B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/7">VII/7 : Lynds' Catalogue of Dark Nebulae (LDN) (Lynds 1962)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/244">VII/244 : Atlas and Catalog of Dark Clouds (Dobashi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/578/914">J/ApJ/578/914 : Low-mass stars in Taurus (Hartmann, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AN/328/889">J/AN/328/889 : Mean Radial Velocities of open clusters (Kharchenko+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/186/259">J/ApJS/186/259 : Taurus Spitzer survey: new candidate members (Rebull+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/724/835">J/ApJ/724/835 : The Spitzer c2d survey of WTTSs. III. (Wahhaj+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/1542">J/ApJ/723/1542 : Optical high-resolution spectroscopy of WTTSs (Xing, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/751/115">J/ApJ/751/115 : Millimeter emission from Taurus bin. systems (Harris+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/745/119">J/ApJ/745/119 : Close companions to young stars I. ChaI &amp; Tau (Nguyen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/91">J/ApJ/801/91 : Gould's Belt Very Large Array survey IV. Taurus (Dzib+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/675">J/MNRAS/472/675 : Wide binaries in Tycho-Gaia: search method (Andrews+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/599/A14">J/A+A/599/A14 : Taurus ultra-wide pairs (Joncour+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/142">J/ApJ/834/142 : GOBELINS. II. OMC (Kounkel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/150">J/ApJ/838/150 : The Taurus-Auriga ecosystem. I. 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