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<ri:Resource created="2015-07-29T13:18:13Z" 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>Cepheid Radial Velocities (CRaV) project</title><shortName>J/AJ/150/13</shortName><identifier>ivo://CDS.VizieR/J/AJ/150/13</identifier><altIdentifier>doi:10.26093/cds/vizier.51500013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Evans N.R.</name></creator><creator><name>Berdnikov L.</name></creator><creator><name>Lauer J.</name></creator><creator><name>Morgan D.</name></creator><creator><name>Nichols J.</name></creator><creator><name>Gunther H.M.,Gorynya N.</name></creator><creator><name>Rastorguev A.</name></creator><creator><name>Moskalik P.</name></creator><date role="Updated">2017-10-18T08:24:28Z</date><date role="Created">2015-07-29T13:18:13Z</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>variable-stars</subject><subject>radial-velocity</subject><description>We have examined high accuracy radial velocities of Cepheids to determine the binary frequency. The data are largely from the CORAVEL spectrophotometer and the Moscow version, with a typical uncertainty of {&lt;=}1km/s, and a time span from 1 to 20years. A systemic velocity was obtained by removing the pulsation component using a high order Fourier series. From this data we have developed a list of stars showing no orbital velocity larger than +/-1km/s. The binary fraction was analyzed as a function of magnitude, and yields an apparent decrease in this fraction for fainter stars. We interpret this as incompleteness at fainter magnitudes, and derive the preferred binary fraction of 29%+/-8% (20%+/-6% per decade of orbital period) from the brightest 40 stars. A comparison of this fraction in this period range (1-20years) implies a large fraction for the full period range. This is reasonable in that the high accuracy velocities are sensitive to the longer periods and smaller orbital velocity amplitudes in the period range sampled here. Thus the Cepheid velocity sample provides a sensitive detection in the period range between short period spectroscopic binaries and resolved companions. The recent identification of {delta} Cep as a binary with very low amplitude and high eccentricity underscores the fact that the binary fractions we derive are lower limits, to which other low amplitude systems will probably be added. The mass ratio (q) distribution derived from ultraviolet observations of the secondary is consistent with a flat distribution for the applicable period range (1-20years).</description><source format="bibcode">2015AJ....150...13E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/150/13</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/229">III/229 : Radial Velocities of Cepheids (Gorynya+ 1992-98)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/566/L10">J/A+A/566/L10 : Cepheid radial velocity amplitude modulations (Anderson, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/227">J/ApJS/156/227 : Radial velocities of 16 Galactic Cepheids (Barnes+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/415/531">J/A+A/415/531 : Radial velocities of 10 Galactic Cepheids (Storm+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/143/211">J/A+AS/143/211 : Galactic Cepheids BVRI photometry (Berdnikov+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/140/79">J/A+AS/140/79 : Radii of 22 galactic Cepheids (Imbert, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/108/25">J/A+AS/108/25 : Cepheids fundamental parameters II. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>Code of reference source (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Year</name><description>[1977/1998] Year of the observation</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>&lt;RV&gt;</name><description>[-3.27/5.33] Mean radial velocity (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>f_&lt;RV&gt;</name><description>[*] Indicates correction added in Table4 (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>e_&lt;RV&gt;</name><description>[0.01/5.05]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Cepheid identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Ref</name><description>Code of reference source (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Year</name><description>[1977/1998] Year of the observation</description><unit>yr</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>&lt;RV&gt;</name><description>[-3.27/5.33] Annual mean radial velocity (from the data and the Fourier curves) (1)</description><unit>km/s</unit><ucd>spect.dopplerVeloc;stat.mean</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_&lt;RV&gt;</name><description>[0.01/5.05]? The 1{sigma} error in &lt;RV&gt;</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>o_&lt;RV&gt;</name><description>[1/91] Number of observation in &lt;RV&gt;</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/AJ/150/13/table6</name><description>Multiplicity status</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Cepheid identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>&lt;Vmag&gt;</name><description>[1.982/9.053] Mean V-band magnitude (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Per</name><description>[1.949/68.464] Pulsation period</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Mult</name><description>Multiplicity status (x=single or bin=binary)</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>RV</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>l_Porb</name><description>[&gt;=] Lower limit flag on Porb</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Porb</name><description>[1/90]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Cepheid identifier</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType><flag>primary</flag></column><column><name>RV</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>Ref1</name><description>'gg' means data from Gorynya et al. 1992-98 (cat. III/229)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Ref2</name><description>'b9' means data from Bersier et al. 1994 (cat. J/A+AS/108/25)</description><ucd>meta.bib</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Ref3</name><description>'im' means data from Imbert 1999 (cat. 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