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<ri:Resource created="2024-02-12T09:56:10Z" status="active" updated="2025-06-19T20:10:29Z" 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>182 RSGs and OB-stars in M31 and M33</title><shortName>J/ApJ/908/87</shortName><identifier>ivo://CDS.VizieR/J/ApJ/908/87</identifier><altIdentifier>doi:10.26093/cds/vizier.19080087</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neugent K.F.</name></creator><date role="Updated">2025-06-19T20:10:29Z</date><date role="Created">2024-02-12T09:56:10Z</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>supergiant-stars</subject><subject>multiple-stars</subject><subject>two-color-diagrams</subject><subject>visible-astronomy</subject><description>Recent work measuring the binary fraction of evolved red supergiants (RSGs) in the Magellanic Clouds points to a value between 15% and 30%, with the majority of the companions being unevolved B-type stars as dictated by stellar evolution. Here I extend this research to the Local Group galaxies M31 and M33 and investigate the RSG binary fraction as a function of metallicity. Recent near-IR photometric surveys of M31 and M33 have led to the identification of a complete sample of RSGs down to a limiting logL/L{sun}&gt;=4.2. To determine the binary fraction of these M31 and M33 RSGs, I used a combination of newly obtained spectroscopy to identify single RSGs and RSG+OB binaries, as well as archival UV, visible, and near-IR photometry to probabilistically classify RSGs as either single or binary based on their colors. I then adjusted the observed RSG+OB binary fraction to account for observational biases. The resulting RSG binary fraction in M33 shows a strong dependence on galactocentric distance, with the inner regions having a much higher binary fraction (41.2_-7.3_^+12.0^%) than the outer regions (15.9_-1.9_^+12.4^%). Such a trend is not seen in M31; instead, the binary fraction in lightly reddened regions remains constant at 33.5_-5.0_^+8.6^% . I conclude that the changing RSG binary fraction in M33 is due to a metallicity dependence, with higher-metallicity environments having higher RSG binary fractions. This dependence most likely stems not from changes in the physical properties of RSGs due to metallicity but from changes in the parent distribution of OB binaries.</description><source format="bibcode">2021ApJ...908...87N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/908/87</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/501/153">J/ApJ/501/153 : VRB photometry of red supergiants (Massey 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/2478">J/AJ/131/2478 : M31 and M33 UBVRI photometry (Massey+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/2474">J/AJ/134/2474 : Ha emission-line stars in 7 dwarfs galaxies (Massey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/733/123">J/ApJ/733/123 : The Wolf-Rayet content of M33 (NGC 598) (Neugent+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/750/97">J/ApJ/750/97 : The yellow and red supergiants of M33 (Drout+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/759/11">J/ApJ/759/11 : Wolf-Rayet content of M31 (Neugent+, 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/758/133">J/ApJ/758/133 : Metallicity profile of M31 HII regions &amp; PNe (Sanders+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A107">J/A+A/550/A107 : RV catalogue of O stars in 30 Doradus (Sana+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/10">J/ApJ/789/10 : M33 WR and Of-type Stars (Neugent+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/578/A3">J/A+A/578/A3 : Survey of supergiants in the MCs (Gonzalez-Fernandez+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/826/224">J/ApJ/826/224 : RSG and foreground candidates in M31 (Massey+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/616/A12">J/A+A/616/A12 : Gaia DR2 sources in GC and dSph (Gaia Collaboration+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/875/124">J/ApJ/875/124 : Binary red supergiants. 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B-type companions (Neugent+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/624/A129">J/A+A/624/A129 : 30 Dor red supergiant stars radial velocities (Patrick+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/629/A91">J/A+A/629/A91 : A source catalog for the SMC (Yang+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/900/118">J/ApJ/900/118 : RSGs in the LMC &amp; sp. follow-up for LMC &amp; SMC (Neugent+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/889/44">J/ApJ/889/44 : UKIRT obs. of red supergiants in M31 (Neugent+, 2020)</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/908/87</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/908/87</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/908/87</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/908/87</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/908/87</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/908/87</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/908/87/table1 (*Spectroscopically observed M31 and M33 stars)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/908/87/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/908/87/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/908/87/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>9.4348333</ra><dec>40.0670556</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/2154-2155 2241 2622-2623 2666 2705 2709 2752</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/908/87?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/908/87/table1</name><description>*Spectroscopically observed M31 and M33 stars</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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