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<ri:Resource created="2024-07-09T08:19:55Z" 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>OBe stellar masses</title><shortName>J/ApJ/936/112</shortName><identifier>ivo://CDS.VizieR/J/ApJ/936/112</identifier><altIdentifier>doi:10.26093/cds/vizier.19360112</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dallas M.M.</name></creator><creator><name>Oey M.S.</name></creator><creator><name>Castro N.</name></creator><date role="Updated">2024-11-12T20:10:52Z</date><date role="Created">2024-07-09T08:19:55Z</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>multiple-stars</subject><subject>ob-stars</subject><subject>stellar-masses</subject><description>Massive binaries play an important role in fields ranging from gravitational- wave astronomy to stellar evolution. We provide several lines of evidence that classical OBe stars in the Small Magellanic Cloud (SMC) obtain their rapid rotation from mass and angular momentum transfer in massive binaries, which predicts that the subsequent supernovae should often eject OBe stars into the field. We find that (1) OBe stars have a higher field frequency than OB stars; (2) our cumulative distribution function (CDF) of stellar distances from O stars shows that OBe stars are indeed much more isolated than ordinary OB stars of corresponding spectral types; (3) the CDFs of OBe stars approach that of high-mass X-ray binaries (HMXBs), which are confirmed post-supernova objects; and (4) Oe stars are as isolated from clusters as Be stars, implying that their final masses are relatively independent of their initial masses, consistent with major mass transfer. Lastly, we also find that the spatial distribution of supergiant OBe stars differs from that of classical OBe stars, consistent with the different mechanisms responsible for their emission-line spectra.</description><source format="bibcode">2022ApJ...936..112D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/936/112</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/23">III/23 : MK Classification for OB Stars (Lesh 1968)</relatedResource><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/J/A+AS/102/451">J/A+AS/102/451 : Emission-line stars and PNe in the SMC (Meyssonnier+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/393/887">J/A+A/393/887 : SMC Be stars candidates (Mennickent+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/353/601">J/MNRAS/353/601 : 2dF survey of the Small Magellanic Cloud (Evans+, 2004)</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/A+A/456/623">J/A+A/456/623 : VLT-FLAMES survey of massive stars (Evans+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/320">J/ApJ/663/320 : IR-through-UV extinction curve (Fitzpatrick+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/472/577">J/A+A/472/577 : NGC 330 Be stars and binaries (Martayan+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/462/683">J/A+A/462/683 : Velocities in SMC field of NGC 330 (Martayan+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/416">J/AJ/140/416 : IR photometry of massive stars in the SMC (Bonanos+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/509/A11">J/A+A/509/A11 : Ha emission-line objects in SMC clusters (Martayan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/1925">J/MNRAS/424/1925 : Spectroscopic Binarity of O and B type stars (Chini+, 2012)</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/ApJ/763/101">J/ApJ/763/101 : Massive field OB stars in the SMC (Lamb+, 2013)</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 spectro survey of SMC field OB stars (Lamb+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A66">J/A+A/624/A66 : Massive runaway and walkaway stars models (Renzo+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/641/A42">J/A+A/641/A42 : Main-sequence comp to massive Be stars (Bodensteiner+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/634/A51">J/A+A/634/A51 : NGC 330 seen by MUSE (Bodensteiner+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/903/43">J/ApJ/903/43 : Kinematic &amp; 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