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<ri:Resource created="2015-01-13T07:58:51Z" 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>The ELM survey. V. White dwarf binaries</title><shortName>J/ApJ/769/66</shortName><identifier>ivo://CDS.VizieR/J/ApJ/769/66</identifier><altIdentifier>doi:10.26093/cds/vizier.17690066</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brown W.R.</name></creator><creator><name>Kilic M.</name></creator><creator><name>Allende Prieto C.</name></creator><creator><name>Gianninas A.</name></creator><creator><name>Kenyon S.J.</name></creator><date role="Updated">2017-06-12T08:25:13Z</date><date role="Created">2015-01-13T07:58:51Z</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>white-dwarf-stars</subject><subject>radial-velocity</subject><subject>stellar-distance</subject><subject>stellar-masses</subject><subject>visible-astronomy</subject><subject>sloan-photometry</subject><description>We present the discovery of 17 low-mass white dwarfs (WDs) in short-period (P&lt;=1 day) binaries. Our sample includes four objects with remarkable logg=~5 surface gravities and orbital solutions that require them to be double degenerate binaries. All of the lowest surface gravity WDs have metal lines in their spectra implying long gravitational settling times or ongoing accretion. Notably, six of the WDs in our sample have binary merger times &lt;10Gyr. Four have &gt;~0.9M_{sun}_ companions. If the companions are massive WDs, these four binaries will evolve into stable mass transfer AM CVn systems and possibly explode as underluminous supernovae. If the companions are neutron stars, then these may be millisecond pulsar binaries. These discoveries increase the number of detached, double degenerate binaries in the Extremely low mass (ELM) Survey to 54; 31 of these binaries will merge within a Hubble time.</description><source format="bibcode">2013ApJ...769...66B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/769/66</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 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/547/A96">J/A+A/547/A96 : Low-mass He-core WDs seismic properties (Corsico+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/751/55">J/ApJ/751/55 : MMT hypervelocity star survey. II. (Brown+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/743/138">J/ApJ/743/138 : Spectroscopic survey of bright WDs (Gianninas+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/536/A43">J/A+A/536/A43 : SDSS WD main-sequence binaries (Nebot Gomez-Moran+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/723/1072">J/ApJ/723/1072 : The ELM survey. I. Low-mass white dwarfs (Brown+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/402/620">J/MNRAS/402/620 : SDSS WD main-sequence binaries (Rebassa-Mansergas+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/513/L7">J/A+A/513/L7 : Post common envelope binaries from SDSS (Schreiber+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2070">J/AJ/136/2070 : SEGUE stellar parameter pipeline III. (Allende Prieto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/1708">J/ApJ/671/1708 : Hypervelocity stars. 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