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<ri:Resource created="2012-01-03T15:00:39Z" 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>Volume-limited sample of M7-M9.5 dwarfs &lt;20pc</title><shortName>J/ApJ/705/1416</shortName><identifier>ivo://CDS.VizieR/J/ApJ/705/1416</identifier><altIdentifier>doi:10.26093/cds/vizier.17051416</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Reiners A.</name></creator><creator><name>Basri G.</name></creator><date role="Updated">2017-12-05T05:11:00Z</date><date role="Created">2012-01-03T15:00:39Z</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>m-stars</subject><subject>radial-velocity</subject><subject>dwarf-stars</subject><subject>stellar-distance</subject><description>In a volume-limited sample of 63 ultracool dwarfs of spectral type M7-M9.5, we have obtained high-resolution spectroscopy with UVES at the Very Large Telescope and HIRES at Keck Observatory. In this first paper we introduce our volume-complete sample from DENIS and 2MASS targets, and we derive radial velocities and space motion. Kinematics of our sample are consistent with the stars being predominantly members of the young disk. The kinematic age of the sample is 3.1Gyr. We find that six of our targets show strong Li lines implying that they are brown dwarfs younger than several hundred million years. Five of the young brown dwarfs were unrecognized before. Comparing the fraction of Li detections to later spectral types, we see a hint of an unexpected local maximum of this fraction at spectral type M9. It is not yet clear whether this maximum is due to insufficient statistics, or to a combination of physical effects including spectral appearance of young brown dwarfs, Li line formation, and the star formation rate at low masses.</description><source format="bibcode">2009ApJ...705.1416R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/705/1416</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/B/denis">B/denis : The DENIS database (DENIS Consortium, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/246">II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/404/1817">J/MNRAS/404/1817 : 2MASS/SDSS data for 806 ultracool dwarfs (Zhang+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/137/1">J/AJ/137/1 : Proper motions and astrometry of late-type dwarfs (Faherty+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/394/857">J/MNRAS/394/857 : UKIDSS-2MASS proper motion survey (Deacon+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1290">J/AJ/136/1290 : Ultracool dwarfs from the 2MASS (Reid+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/439">J/AJ/133/439 : Luminosity function of M7-L8 ultracool dwarfs (Cruz+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/446/515">J/A+A/446/515 : Distances of nearby ultracool dwarfs (Phan-Bao+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/441/653">J/A+A/441/653 : 32 DENIS nearby red dwarfs (Crifo+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2421">J/AJ/126/2421 : 2MASS-Selected sample of ultracool dwarfs (Cruz+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1526">J/AJ/126/1526 : IR photometry of ultracool dwarfs (Bouy+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/401/959">J/A+A/401/959 : 35 DENIS late-M dwarfs between 10 and 30pc (Phan-Bao+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/380/590">J/A+A/380/590 : 30 DENIS late-M dwarfs between 15 and 30pc (Phan-Bao+, 2001)</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/705/1416</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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