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<ri:Resource created="2020-12-15T07:46:29Z" 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>RV variability in SDSS dwarf carbon stars</title><shortName>J/ApJ/877/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/877/44</identifier><altIdentifier>doi:10.26093/cds/vizier.18770044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Roulston B.R.</name></creator><creator><name>Green P.J.</name></creator><creator><name>Ruan J.J.</name></creator><creator><name>MacLeod C.L.</name></creator><creator><name>Anderson S.F.,Badenes C.</name></creator><creator><name>Brownstein J.R.</name></creator><creator><name>Schneider D.P.</name></creator><creator><name>Stassun K.G.</name></creator><date role="Updated">2021-09-09T12:01:21Z</date><date role="Created">2020-12-15T07:46:29Z</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>carbon-stars</subject><subject>dwarf-stars</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>radial-velocity</subject><subject>sloan-photometry</subject><description>Dwarf carbon (dC) stars (main-sequence stars showing carbon molecular bands) were initially thought to be an oxymoron because only asymptotic giant branch (AGB) stars dredge carbon into their atmospheres. Mass transfer from a former AGB companion that has since faded to a white dwarf seems the most likely explanation. Indeed, a few types of giants known to show anomalous abundances- notably, the CH, Ba and CEMP-s stars-are known to have a high binary frequency. The dC stars may be the enhanced-abundance progenitors of most, if not all of these systems, but this requires demonstrating a high binary frequency for dCs. Here, for a sample of 240 dC stars targeted for repeat spectroscopy by the SDSS-IV's Time Domain Spectroscopic Survey, we analyze radial velocity (RV) variability to constrain the binary frequency and orbital properties. A handful of dC systems show large velocity variability (&gt;100km/s). We compare the dCs to a control sample with a similar distribution of magnitude, color, proper motion, and parallax. Using Markov chain Monte Carlo methods, we use the measured {Delta}RV distribution to estimate the binary fraction and the separation distribution assuming both a unimodal and bimodal distribution. We find the dC stars have an enhanced binary fraction of 95%, consistent with them being products of mass transfer. These models result in mean separations of less than 1 au corresponding to periods on the order of 1 yr. Our results support the conclusion that dC stars form from close binary systems via mass transfer.</description><source format="bibcode">2019ApJ...877...44R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/877/44</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/II/294">II/294 : SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/147">V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/366">J/A+A/375/366 : Carbon stars from the Hamburg/ESO survey (Christlieb+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/330/792">J/MNRAS/330/792 : Radial velocity in Draco (Kleyna+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2838">J/AJ/127/2838 : Faint high-lat. carbon stars SDSS photometry (Downes+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/12">J/ApJ/765/12 : Carbon stars and DQ WDs from SDSS-DR7+DR8 (Green, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/797/21">J/ApJ/797/21 : Carbon-enhanced metal-poor stars (Placco+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/RAA/15.1671">J/other/RAA/15.1671 : New carbon stars from LAMOST survey (Si+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/586/A158">J/A+A/586/A158 : Binary properties of CH and CEMP stars (Jorissen+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/252">J/AJ/155/252 : Astrometry &amp; photometry of dwarf carbon stars (Harris+, 2018)</relatedResource><relatedResource>http://www.sdss.org/ : SDSS home page</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/877/44</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/877/44</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/877/44</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/877/44</accessURL><mirrorURL title="VizieR at IUCAA: 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