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Li abundances</title><shortName>J/A+A/508/833</shortName><identifier>ivo://CDS.VizieR/J/A+A/508/833</identifier><altIdentifier>doi:10.26093/cds/vizier.35080833</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>da Silva L.</name></creator><creator><name>Torres C.A.O.</name></creator><creator><name>de la Reza R.</name></creator><creator><name>Quast G.R.</name></creator><creator><name>Melo C.H.F.,Sterzik M.F.</name></creator><date role="Updated">2026-01-20T12:10:41Z</date><date role="Created">2012-08-22T09:09:14Z</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>stellar-associations</subject><subject>chemical-abundances</subject><subject>line-intensities</subject><description>Our study is a follow-up of the SACY project, an extended high spectral resolution survey of more than two thousand optical counterparts to X-ray sources in the southern hemisphere targeted to search for young nearby association. Nine associations have either been newly identified, or have had their member list revised. Groups belonging to the Sco-Cen-Oph complex are not considered in the present study. These nine associations, with ages of between about 6Myr and 70Myr, form an excellent sample to study the Li depletion in the pre-main sequence (PMS) evolution. In the present paper, we investigate the use of Li abundances as an independent clock to constrain the PMS evolution. Using our measurements of the equivalent widths of the Li resonance line and assuming fixed metallicities and microturbulence, we calculated the LTE Li abundances for 376 members of various young associations. 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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>Tab</name><description>[3/11] Table number for association (1)</description><ucd>meta.id;meta.dataset</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Star name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="15*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>W(Li)</name><description>? 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