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<ri:Resource created="2018-06-12T13:40:46Z" 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>WD+dMs from the SUPERBLINK proper motion survey</title><shortName>J/AJ/154/118</shortName><identifier>ivo://CDS.VizieR/J/AJ/154/118</identifier><altIdentifier>doi:10.26093/cds/vizier.51540118</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Skinner J.N.</name></creator><creator><name>Morgan D.P.</name></creator><creator><name>West A.A.</name></creator><creator><name>Lepine S.</name></creator><creator><name>Thorstensen J.R.</name></creator><date role="Updated">2018-08-23T06:48:01Z</date><date role="Created">2018-06-12T13:40:46Z</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>multiple-stars</subject><subject>white-dwarf-stars</subject><subject>dwarf-stars</subject><subject>m-stars</subject><subject>proper-motions</subject><subject>ultraviolet-photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>stellar-spectral-types</subject><subject>radial-velocity</subject><subject>stellar-distance</subject><description>We present an activity and kinematic analysis of high proper motion white dwarf-M dwarf binaries (WD+dMs) found in the SUPERBLINK survey, 178 of which are new identifications. To identify WD+dMs, we developed a UV-optical-IR color criterion and conducted a spectroscopic survey to confirm each candidate binary. For the newly identified systems, we fit the two components using model white dwarf spectra and M dwarf template spectra to determine physical parameters. We use H{alpha} chromospheric emission to examine the magnetic activity of the M dwarf in each system, and investigate how its activity is affected by the presence of a white dwarf companion. We find that the fraction of WD+dM binaries with active M dwarfs is significantly higher than their single M dwarf counterparts at early and mid-spectral types. We corroborate previous studies that find high activity fractions at both close and intermediate separations. At more distant separations, the binary fraction appears to approach the activity fraction for single M dwarfs. Using derived radial velocities and the proper motions, we calculate 3D space velocities for the WD+dMs in SUPERBLINK. For the entire SUPERBLINK WD+dMs, we find a large vertical velocity dispersion, indicating a dynamically hotter population compared to high proper motion samples of single M dwarfs. We compare the kinematics for systems with active M dwarfs and those with inactive M dwarfs, and find signatures of asymmetric drift in the inactive sample, indicating that they are drawn from an older population.</description><source format="bibcode">2017AJ....154..118S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/154/118</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/I/298">I/298 : LSPM-North Catalog (Lepine+ 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/124/1190">J/AJ/124/1190 : Northern high proper motion stars in DSS (Lepine+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/2621">J/AJ/125/2621 : SDSS WD-M binary parameters (Raymond+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/586/1356">J/ApJ/586/1356 : White dwarfs with cool companions (Wachter+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/2428">J/AJ/129/2428 : M dwarf-white dwarf binary systems (Silvestri+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/161/394">J/ApJS/161/394 : Low-luminosity companions to white dwarfs (Farihi+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/26">J/AJ/134/26 : Binaries with white dwarf in 2MASS (Hoard+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/2177">J/AJ/135/2177 : High proper motion stars in the DSS. 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photometry of nearby white dwarfs</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/570/A107">J/A+A/570/A107 : WDMS from LAMOST DR1 (Ren+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/445/1331">J/MNRAS/445/1331 : White-dwarf + main-sequence binaries in SDSS DR9 (Li+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/219/19">J/ApJS/219/19 : Census of nearby white dwarfs from SUPERBLINK</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/AJ/154/118</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/154/118</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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>PM</name><description>SUPERBLINK identifier (PM IHHMMm+DDMMW) (G1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="12*">char</dataType></column><column><name>UVel</name><description>[-690.83/385.93] System heliocentric space velocity component U</description><unit>km/s</unit><ucd>pos.cartesian.x;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_UVel</name><description>[0.82/186.73] Uncertainty in UVel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>VVel</name><description>[-627.83/425.48] System heliocentric space velocity component V</description><unit>km/s</unit><ucd>pos.cartesian.y;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_VVel</name><description>[2.05/134.23] Uncertainty in VVel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>WVel</name><description>[-436.28/477.82] System heliocentric space velocity component W</description><unit>km/s</unit><ucd>pos.cartesian.z;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_WVel</name><description>[1.43/382.27] Uncertainty in WVel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table><table><name>J/AJ/154/118/table1</name><description>Astrometric and Photometric Properties of the WD+dMs in the SUPERBLINK Proper Motion Survey</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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