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<ri:Resource created="2022-06-08T07:42:31Z" 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 VLBA Survey of Radio Stars in the ONC. II.</title><shortName>J/ApJ/906/24</shortName><identifier>ivo://CDS.VizieR/J/ApJ/906/24</identifier><altIdentifier>doi:10.26093/cds/vizier.19060024</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dzib S.A.</name></creator><creator><name>Forbrich J.</name></creator><creator><name>Reid M.J.</name></creator><creator><name>Menten K.M.</name></creator><date role="Updated">2022-10-14T13:03:26Z</date><date role="Created">2022-06-08T07:42:31Z</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>open-star-clusters</subject><subject>radio-sources</subject><subject>radio-astronomy</subject><subject>astrometry</subject><description>From Very Long Baseline Array (VLBA) observations we previously identified a population of 123 young stellar systems with nonthermal radio emission toward the core of the Orion Nebula Cluster (ONC). We find optical sources in the Gaia DR2 catalog for 34 of them within 0.2 of the radio positions. Most of the radio sources are likely companions of Gaia detections. However, there are 11 stars whose VLBA positions differ from Gaia by &lt;1.6mas, and some of these radio sources probably are the direct counterparts of the optical stars. We are able to obtain radio proper motions for 23 stars. Combining the stellar proper motions derived from the VLBA and Gaia DR2 data we find the global motion and velocity dispersion of the ONC to be ({mu}{alpha}*,{mu}{delta})=(1.20{+/-}0.09,0.18{+/-}0.09)mas/yr and ({sigma}_{mu}_{alpha}__,{sigma}_{mu}_{delta}__)=(0.84{+/-}0.09,1.30{+/ -}0.09)mas/yr. Finally, we looked for ordered motions by estimating the means of scalar and vectorial products, which results in \overline{nu}.r=-0.61{+/-}1.00km/s and {nu}xr=0.57{+/-}0.95km/s. These do not show indications that the young stellar cluster is in expansion, contraction, or rotation.</description><source format="bibcode">2021ApJ...906...24D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/906/24</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/J/AJ/113/1733">J/AJ/113/1733 : Orion Nebula Cluster population (Hillenbrand 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/160/353">J/ApJS/160/353 : Membership of the Orion nebula population (Getman+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/14">J/ApJ/748/14 : ONC population data from WFI observations (Da Rio+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/146/85">J/AJ/146/85 : Spectral types 1576 optical stars in ONC (Hillenbrand+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/790/49">J/ApJ/790/49 : Gould's Belt VLA survey. III. Orion region (Kounkel+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/822/93">J/ApJ/822/93 : The population compact radio sources in ONC (Forbrich+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A153">J/A+A/587/A153 : VISION I. VISTA Orion A Survey (Meingast+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/834/142">J/ApJ/834/142 : Gould's Belt Distances Survey. II. OMC (Kounkel+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/467/L71">J/MNRAS/467/L71 : Significance of VLBI/Gaia position offsets (Petrov+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/157/109">J/AJ/157/109 : Stellar proper motions in the Orion Nebula Cluster (Kim+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/870/32">J/ApJ/870/32 : Kinematics in young star clusters &amp; associations (Kuhn+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/159/272">J/AJ/159/272 : Orion Nebula Cluster PMs HST Treasury Program (Platais+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/906/23">J/ApJ/906/23 : A VLBA Survey of radio stars in the ONC. I. (Forbrich+, 2021)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/906/24</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/906/24</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/906/24</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/906/24</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/906/24</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/906/24</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/906/24/table2 (Positions of detected sources in the VLBA images and their formal errors as derived from Imfit)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/906/24/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/906/24/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/906/24/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>83.733231075</ra><dec>-5.38695115</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/21439</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/906/24?format=ascii</footprint><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/906/24/table2</name><description>Positions of detected sources in the VLBA images and their formal errors as derived from Imfit</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Error on SepRA</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SepDE</name><description>[-150/181]? Separation between the Gaia and VLBA in DE direction</description><unit>mas</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_SepDE</name><description>[0.2/7]? Error in SepDE</description><unit>mas</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>pm</name><description>Proper motion available (table3)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table><table><name>J/ApJ/906/24/table3</name><description>Sources with determined proper motions from VLBA observations</description><column><name>[FRM2016]</name><description>Source identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>pmRA-Gaia</name><description>[-1.45/3.77]? Proper motion in RA, Gaia DR2</description><unit>mas/yr</unit><ucd>pos.pm;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_pmRA-Gaia</name><description>[0.1/0.6]? 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