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<ri:Resource created="2012-08-16T12:56:45Z" 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>Optical high-resolution spectroscopy of WTTSs</title><shortName>J/ApJ/723/1542</shortName><identifier>ivo://CDS.VizieR/J/ApJ/723/1542</identifier><altIdentifier>doi:10.26093/cds/vizier.17231542</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Xing L.F.</name></creator><date role="Updated">2017-10-03T05:12:56Z</date><date role="Created">2012-08-16T12:56:45Z</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>chemical-abundances</subject><subject>line-intensities</subject><subject>effective-temperature</subject><subject>pre-main-sequence-stars</subject><subject>young-stellar-objects</subject><description>We present high-resolution spectroscopic observations for a sample of 19 weak-line T Tauri stars (WTTSs). Based on these observations and data of 108 WTTSs taken from the literature, we derive lithium abundances for 127 WTTSs. Investigation of a possible relation between lithium and rotation in WTTSs shows that: (1) rapidly rotating WTTSs have comparatively lower lithium abundances than their slower rotating counterparts; (2) in the spectral-type range G0-K0, most of the WTTSs share the same Li content irrespective of their Teff; and (3) active late-type binaries do not obey the correlation between lithium abundances and rotation periods, since the tidally locked rotation of the late-type binary system leads naturally to slower lithium destruction rates.</description><source format="bibcode">2010ApJ...723.1542X</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/723/1542</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/J/A+A/479/827">J/A+A/479/827 : UBVR light curves of weak-line T Tauri stars (Grankin+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/467/785">J/A+A/467/785 : SuperWASP/ROSAT periodic variable stars (Norton+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/667/308">J/ApJ/667/308 : Weak-line T Tauri in Spitzer c2d Survey. II. (Cieza+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/2294">J/AJ/129/2294 : Radial velocities of WTTS (Massarotti+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/130">J/A+A/375/130 : New PMS spectroscopic binaries in Orion (Covino+ 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/862">J/A+A/372/862 : Lithium abundances in IC 2602 and IC 2391 (Randich+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/145/187">J/A+AS/145/187 : uvby-{beta} photometry of WTTS (Chavarria-K+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/341/L79">J/A+A/341/L79 : Proper motions of faint ROSAT WTT stars (Terranegra+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/132/173">J/A+AS/132/173 : New weak-line T Tauri stars in Taurus-Auriga (Li+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/124/449">J/A+AS/124/449 : Young stars south of Taurus-Auriga (Magazzu+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/312/439">J/A+A/312/439 : New T Tauri stars in Taurus-Auriga (Wichmann+, 1996)</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/723/1542</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/723/1542</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/723/1542</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/723/1542</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/723/1542</mirrorURL><mirrorURL 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44059 44104</spatial><spectral>3.322582951404819e-19 3.852589004194616e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/723/1542?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/723/1542/table1</name><description>Photometric results and other parameters of our WTTSs sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Effective temperature determined from B-V</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Teff2</name><description>Effective temperature determined from the line-depth ratios of VI{lambda}6251.83 and FeI{lambda}6252.527</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Teff</name><description>? Effective temperature from literature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>r_Teff</name><description>Reference for Teff (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W(Li)</name><description>Equivalent width of Li (m{AA})</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logNLi</name><description>? Log of the Li number abundance (H=12)</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>log(g)</name><description>Log of the surface gravity</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Prot</name><description>? Rotational period (mainly derived by Xing et al. 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The (B-V) color index</description><unit>mag</unit><ucd>phot.color;em.opt.B;em.opt.V</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Teff</name><description>Effective temperature</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>r_Teff</name><description>Reference for Teff (3)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>W(Li)</name><description>Equivalent width of Li (m{AA})</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logNLi</name><description>? Log of the Li number abundance</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Prot</name><description>? 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