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<ri:Resource created="2019-11-18T14:43:06Z" 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>Gaia kinematic data of runaway &amp; field OB stars in SMC</title><shortName>J/ApJ/867/L8</shortName><identifier>ivo://CDS.VizieR/J/ApJ/867/L8</identifier><altIdentifier>doi:10.26093/cds/vizier.18679008</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Oey M.S.</name></creator><creator><name>Jones J.D.</name></creator><creator><name>Castro N.</name></creator><creator><name>Zivick P.</name></creator><creator><name>Besla G.</name></creator><creator><name>Januszewski H.C.,Moe M.</name></creator><creator><name>Kallivayalil N.</name></creator><creator><name>Lennon D.J.</name></creator><date role="Updated">2020-03-26T14:19:11Z</date><date role="Created">2019-11-18T14:43:06Z</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>ob-stars</subject><subject>magellanic-clouds</subject><subject>radial-velocity</subject><subject>spectroscopic-binary-stars</subject><description>We use Gaia Data Release 2 proper motions of field OB stars from the Runaways and Isolated O-Type Star Spectroscopic Survey of the Small Magellanic Cloud (SMC) to study the kinematics of runaway stars. The data reveal that the SMC Wing has a systemic peculiar motion relative to the SMC Bar of (v_{alpha}_,v_{delta}_)=(62+/-7,-18+/-5)km/s and relative radial velocity +4.5+/-5.0km/s. This unambiguously demonstrates that these two regions are kinematically distinct: the Wing is moving away from the Bar, and towards the Large Magellanic Cloud with a 3D velocity of 64+/-10km/s. This is consistent with models for a recent, direct collision between the Clouds. We present transverse velocity distributions for our field OB stars, confirming that unbound runaways comprise on the order of half our sample, possibly more. Using eclipsing binaries and double-lined spectroscopic binaries as tracers of dynamically ejected runaways, and high-mass X-ray binaries (HMXBs) as tracers of runaways accelerated by supernova kicks, we find significant contributions from both populations. The data suggest that HMXBs have lower velocity dispersion relative to dynamically ejected binaries, consistent with the former group corresponding to less energetic supernova kicks that failed to unbind the components. Evidence suggests that our fast runaways are dominated by dynamical, rather than supernova, ejections.</description><source format="bibcode">2018ApJ...867L...8O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/867/L8</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/236">II/236 : UBVR CCD survey of the Magellanic clouds (Massey+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/331/949">J/A+A/331/949 : Wolf-Rayet and O-star runaways kinematics (Moffat+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1632">J/AJ/127/1632 : UBVR(UIT) photometry of O and OB stars in SMC (Oey+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/3358">J/AJ/137/3358 : Speckle interferometry of massive stars (Mason+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Sci/337.444">J/other/Sci/337.444 : RV curves of Galactic massive O stars (Sana+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/442/1663">J/MNRAS/442/1663 : Velocities of red giants in the SMC (Dobbie+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/810/61">J/ApJ/810/61 : Early-type EBs with intermediate periods (Moe+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/586/A81">J/A+A/586/A81 : High-mass X-ray binaries in the SMC (Haberl+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/113">J/ApJ/817/113 : RIOTS4: spec. survey of SMC field OB stars (Lamb+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AcA/66/421">J/AcA/66/421 : Eclipsing binaries in the Magellanic System (Pawlak+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/472/3887">J/MNRAS/472/3887 : Kinematic data for stars in OB-associations (Melnik+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/156/98">J/AJ/156/98 : Runaway stars in 30 Doradus region of LMC (Platais+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/868/57">J/ApJ/868/57 : HR diagram of OB stars in the SMC (Castro+, 2018)</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/867/L8</accessURL><mirrorURL title="VizieR at IUCAA: 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