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<ri:Resource created="2015-08-07T09:45:53Z" 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>VLTS. B stars multiplicity</title><shortName>J/A+A/580/A93</shortName><identifier>ivo://CDS.VizieR/J/A+A/580/A93</identifier><altIdentifier>doi:10.26093/cds/vizier.35800093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Dunstall P.R.</name></creator><creator><name>Dufton P.L.</name></creator><creator><name>Sana H.</name></creator><creator><name>Evans C.J.</name></creator><creator><name>Howarth I.D.,Simon-Diaz S.</name></creator><creator><name>de Mink S.E.</name></creator><creator><name>Langer N.</name></creator><creator><name>Maiz Apellaniz J.</name></creator><creator><name>Taylor W.D.</name></creator><date role="Updated">2017-12-22T05:32:55Z</date><date role="Created">2015-08-07T09:45:53Z</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>magellanic-clouds</subject><subject>b-stars</subject><subject>spectroscopic-binary-stars</subject><subject>radial-velocity</subject><description>We investigate the multiplicity properties of 408 B-type stars observed in the 30 Doradus region of the Large Magellanic Cloud with multi-epoch spectroscopy from the VLT-FLAMES Tarantula Survey (VFTS). We use a cross-correlation method to estimate relative radial velocities from the helium and metal absorption lines for each of our targets. Objects with significant radial-velocity variations (and with an amplitude larger than 16km/s) are classified as spectroscopic binaries. We find an observed spectroscopic binary fraction (defined by periods of &lt;10^3.5^d and mass ratios &gt;0.1) for the B-type stars, f_B_(obs)=0.25+/-0.02, which appears constant across the field of view, except for the two older clusters (Hodge 301 and SL 639). These two clusters have significantly lower binary fractions of 0.08+/-0.08 and 0.10+/-0.09, respectively. Using synthetic populations and a model of our observed epochs and their potential biases, we constrain the intrinsic multiplicity properties of the dwarf and giant (i.e. relatively unevolved) B-type stars in 30 Dor. We obtain a present-day binary fraction f_B_(true)=0.58+/-0.11, with a flat period distribution. Within the uncertainties, the multiplicity properties of the B-type stars agree with those for the O stars in 30 Dor from the VFTS.</description><source format="bibcode">2015A&amp;A...580A..93D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/580/A93</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/J/A+A/530/A108">J/A+A/530/A108 : VLT-FLAMES Tarantula Survey (Evans+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A107">J/A+A/550/A107 : VLTS. RV catalogue of O stars in 30 Doradus (Sana+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A108">J/A+A/550/A108 : DIB in VLT-FLAMES Tarantula Survey (van Loon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A109">J/A+A/550/A109 : VLTS: vsini measures (Dufton+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A134">J/A+A/558/A134 : VLTS. 30 Dor luminous stars (Doran+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A29">J/A+A/560/A29 : O-stars in VLT-FLAMES Tarantula Survey (Ramirez-Agudelo+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A39">J/A+A/564/A39 : VLTS. OVz stars in 30 Dor (Sabin-Sanjulian+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/A40">J/A+A/564/A40 : VFTS. O-type stellar content of 30 Dor (Walborn+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/564/L7">J/A+A/564/L7 : VLT-FLAMES Tarantula Survey: VFTS 822 (Kalari+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/575/A70">J/A+A/575/A70 : VFTS. 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