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<ri:Resource created="2022-01-20T11:58:02Z" 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>Binary red supergiants. II. B-type companions</title><shortName>J/ApJ/875/124</shortName><identifier>ivo://CDS.VizieR/J/ApJ/875/124</identifier><altIdentifier>doi:10.26093/cds/vizier.18750124</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Neugent K.F.</name></creator><creator><name>Levesque E.M.</name></creator><creator><name>Massey P.</name></creator><creator><name>Morrell N.I.</name></creator><date role="Updated">2022-11-03T06:37:17Z</date><date role="Created">2022-01-20T11:58:02Z</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>supergiant-stars</subject><subject>multiple-stars</subject><subject>b-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>spectroscopy</subject><subject>effective-temperature</subject><description>The percentage of massive main-sequence OB stars in binary systems is thought to be as high as 100%. However, very few Galactic binary red supergiants (RSGs) have been identified, despite the fact that these stars are the evolved descendants of OB stars. As shown in our recent paper, binary RSGs will likely have B-type companions, as dictated by stellar evolution considerations. Such a system will have a very unique photometric signature due to the shape of the spectral energy distribution. Using photometric cutoffs, it should therefore be possible to detect candidate RSG+B star binary systems. Here we present our spectroscopic follow-up observations of such candidates. Out of our initial list of 280 candidates in M31 and M33, we observed 149 and confirmed 63 as newly discovered RSG+B star binary systems. Additional spectra of four candidate systems in the Small Magellanic Cloud confirmed all of them as new RSG+B star binaries including the first known RSG+Be star system. By fitting BSTAR06 and MARCS model atmospheres to the newly obtained spectra, we place estimates on the temperatures and subtypes of both the B stars and RSGs. Overall, we have found 87 new RSG+B star binary systems in M31, M33 and the Small and Large Magellanic Clouds. Our future studies are aimed at determining the binary fraction of RSGs.</description><source format="bibcode">2019ApJ...875..124N</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/875/124</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/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/118/2211">J/AJ/118/2211 : M31F eclipsing binaries and Cepheids (Mochejska+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/188">J/A+A/383/188 : Spectrophotometric atlas of symbiotic stars (Munari+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/123/855">J/AJ/123/855 : Magellanic Clouds Photometric Survey: SMC (Zaritsky+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/128/1606">J/AJ/128/1606 : Magellanic Clouds Photometric Survey: LMC (Zaritsky+, 2004)</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/ApJ/689/461">J/ApJ/689/461 : Circumstellar disk of {chi} Oph (Tycner+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/703/420">J/ApJ/703/420 : Red supergiants in M31 (Massey+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/140/14">J/AJ/140/14 : Variability of luminous stars in LMC (Szczygiel+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/532/A138">J/A+A/532/A138 : V838 Mon spectrum in 2009 (Tylenda+, 2011)</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/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/ApJ/900/118">J/ApJ/900/118 : RSGs in the LMC &amp; 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