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<ri:Resource created="2021-11-12T07:10:38Z" 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>~17000 runaways stars from the Orion Nebula Cluster</title><shortName>J/ApJ/900/14</shortName><identifier>ivo://CDS.VizieR/J/ApJ/900/14</identifier><altIdentifier>doi:10.26093/cds/vizier.19000014</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Farias J.P.</name></creator><creator><name>Tan J.C.</name></creator><creator><name>Eyer L.</name></creator><date role="Updated">2022-03-14T08:53:06Z</date><date role="Created">2021-11-12T07:10:38Z</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>astrometry</subject><subject>radial-velocity</subject><description>We use Gaia DR2 to hunt for runaway stars from the Orion Nebula Cluster (ONC). We search a region extending 45{deg} around the ONC and out to 1 kpc to find sources that have overlapped in angular position with the cluster in the last ~10Myr. We find ~17000 runaway/walkaway candidates that satisfy this 2D traceback condition. Most of these are expected to be contaminants, e.g., caused by Galactic streaming motions of stars at different distances. We thus examine six further tests to help identify real runaways, namely: (1) possessing young stellar object (YSO) colors and magnitudes based on Gaia optical photometry; (2) having IR excess consistent with YSOs based on 2MASS and Wide-field Infrared Survey Explorer photometry; (3) having a high degree of optical variability; (4) having closest approach distances well-constrained to within the cluster half-mass radius; (5) having ejection directions that avoid the main Galactic streaming contamination zone; and (6) having a required radial velocity (RV) for 3D overlap of reasonable magnitude (or, for the 7% of candidates with measured RVs, satisfying 3D traceback). Thirteen sources, not previously noted as Orion members, pass all these tests, while another twelve are similarly promising, except they are in the main Galactic streaming contamination zone. Among these 25 ejection candidates, ten with measured RVs pass the most restrictive 3D traceback condition. We present full lists of runaway/walkaway candidates, estimate the high-velocity population ejected from the ONC, and discuss its implications for cluster formation theories via comparison with numerical simulations.</description><source format="bibcode">2020ApJ...900...14F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/900/14</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/II/332">II/332 : c2d Spitzer final data release (DR4) (Evans+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/337">I/337 : Gaia DR1 (Gaia Collaboration, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/360">II/360 : Gaia DR2 x AllWISE catalogue (Marton+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/48/35">J/AcA/48/35 : All Sky Automated Survey variable stars (Pojmamski 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/119/3026">J/AJ/119/3026 : Circumstellar disk candidates in Orion (Rebull+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/502/883">J/A+A/502/883 : photometry very low mass ONC stars (Rodriguez-Ledesma+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/1092">J/ApJ/722/1092 : Optical photometry of the ONC. II. (Da Rio+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/192">J/AJ/144/192 : Spitzer survey of Orion A &amp; B. I. YSO catalog (Megeath+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/32">J/ApJS/209/32 : Probable young stars in the MYStIX project (Broos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/818/59">J/ApJ/818/59 : IN-SYNC. IV. YSOs in Orion A (Da Rio+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/229/28">J/ApJS/229/28 : SFiNCs: X-ray, IR and membership catalogs (Getman+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/84">J/AJ/156/84 : APOGEE-2 survey of Orion Complex. II. (Kounkel+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/271">J/AJ/156/271 : The stellar membership of the Taurus SFR (Luhman, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/620/A172">J/A+A/620/A172 : Solar neighbourhood young stars 3D mapping (Zari+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/627/A57">J/A+A/627/A57 : ONC binary and triple stars (Jerabkova+, 2019)</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/ApJ/884/6">J/ApJ/884/6 : Known members of Orion A with Gaia DR2 data (McBride+, 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Uncertainty in dmin3D</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><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 DR2 source identifier</description><ucd>meta.id;meta.main</ucd></column><column><name>Label</name><description>Source label and score; see Sec. 5.1</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>GLON</name><description>[160/258] Gaia DR2 Galactic longitude (J2015.5)</description><unit>deg</unit><ucd>pos.galactic.lon</ucd><flag>indexed</flag></column><column><name>GLAT</name><description>[-64.3/24.6] Gaia DR2 Galactic latitude (J2015.5)</description><unit>deg</unit><ucd>pos.galactic.lat</ucd><flag>indexed</flag></column><column><name>dONC</name><description>[0.36/738] 3D distance to the ONC</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>theta</name><description>[0.002/45.2] Angular distance to the ONC</description><unit>deg</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>vt0</name><description>[0.06/605] Transverse velocity in the ONC frame</description><unit>km/s</unit><ucd>phys.veloc.transverse</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>tback</name><description>[0.001/40.7] 2D traceback time</description><unit>Myr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>vrOpt</name><description>[-160584/53149] Median optimal radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>b_vrOpt</name><description>[-161544/30219] The 16th percentile uncertainty in vrOpt</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>B_vrOpt</name><description>[-159682/118973] The 84th percentile uncertainty in vrOpt</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RVel</name><description>[-133/296]? Gaia DR2 radial velocity</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_RVel</name><description>[0.1/18]? Uncertainty in RVel</description><unit>km/s</unit><ucd>stat.error;spect.dopplerVeloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Vi</name><description>[-0.91/5.45]? Intrinsic variability; see Sec. 4.3</description><ucd>meta.code;src.var</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>Dmin</name><description>[0.001/68.2] Closest approach ONC; 2D traceback</description><unit>arcmin</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Dmin</name><description>[0.01/852] Uncertainty in Dmin</description><unit>arcmin</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>PA</name><description>[0.08/360] Position Angle from the ONC</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>R</name><description>[0.114/0.95]? Probability being real source (1)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>SY</name><description>[0/1]? YSO proba. using 2 AllWISE bands (1)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>LY</name><description>[0/1]? YSO proba. using 4 AllWISE bands (1)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>d</name><description>[6.42/1000] Gaia DR2 parallax distance</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>E_d</name><description>[6.42/1245] Upper uncertainty in d</description><unit>pc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_d</name><description>[6.41/982] Lower uncertainty in d</description><unit>pc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>v3DONC</name><description>[2.57/410]? Space velocity in ONC frame of reference</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>tback3D</name><description>[-26.9/19.4]? 3D traceback time</description><unit>Myr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>e_tback3D</name><description>[0.003/11]? Uncertainty in tback3D</description><unit>Myr</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>dmin3D</name><description>[0.2/641]? Closest approach to ONC 3D traceback</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>YSOFlag</name><description>[-1/1] YSO flag: +1 pass, -1 fail</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>WYSOFlag</name><description>[-1/1] WYSO flag: +1 pass, -1 fail, 0 not evaluated</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>VARFlag</name><description>[-1/1] VAR flag: +1 pass, -1 fail, 0 not evaluated</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CAFlag</name><description>[-1/1] CA flag: +1 pass, -1 fail</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PAFlag</name><description>[-1/1] PA flag: +1 pass, -1 fail</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>RVFlag</name><description>[-1/1] RV flag: +1 pass, -1 fail</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data. The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table></schema></tableset></ri:Resource>