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<ri:Resource created="2021-11-15T11:23:53Z" 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>Barium abundances from Keck/HIRES high res. spectra</title><shortName>J/ApJ/896/64</shortName><identifier>ivo://CDS.VizieR/J/ApJ/896/64</identifier><altIdentifier>doi:10.26093/cds/vizier.18960064</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu S.</name></creator><creator><name>Shi J.</name></creator><creator><name>Wu Z.</name></creator><date role="Updated">2022-09-21T09:25:48Z</date><date role="Created">2021-11-15T11:23:53Z</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>visible-astronomy</subject><description>Based on the high-resolution, high signal-to-noise-ratio spectra from the Keck/HIRES, we have analyzed the barium abundances of 602 stars. The parameter space of our sample are in the range of 4700&lt;Teff&lt;6100K, -0.1&lt;[Fe/H]&lt;0.6dex, and 2&lt;logg&lt;5dex. It is found that the nonlocal thermodynamic equilibrium (NLTE) effects are large for barium, and the barium abundances can be underestimated by up to 0.2dex compared to the the local thermodynamic equilibrium analysis for lines at 5853 and 6141{AA}. In addition, the average barium abundances of the high- and low-{alpha} stars are -0.10 and 0.00dex, respectively, and higher [Ba/Fe] corresponds to a lower [Mg/Fe] ratio. We note that there are 18 Ba-rich stars (with [Ba/Fe]&gt;0.3 in NLTE), which contains six dwarfs and 12 giants. The Ba-rich objects make up around 3% in our sample.</description><source format="bibcode">2020ApJ...896...64L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/896/64</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/MNRAS/404/1529">J/MNRAS/404/1529 : s-process in low-metallicity stars (Bisterzo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/511/L10">J/A+A/511/L10 : Abundances and space velocities of 94 stars (Nissen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/530/A15">J/A+A/530/A15 : Abundances 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xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</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="10*">char</dataType></column><column><name>Teff</name><description>[4702/6219] Stellar effective temperature (1)</description><unit>K</unit><ucd>phys.temperature.effective</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>logg</name><description>[2.7/4.83] Stellar surface gravity (1)</description><unit>log(cm.s**-2)</unit><ucd>phys.gravity</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Mg/Fe]</name><description>[-0.23/0.29] Magnesium-to-Iron abundance ratio, log</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>vt</name><description>[0.85/0.85] Microturbulent velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]LTE1</name><description>[-0.35/0.72] Relative abundance, 5853{AA} line, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]NLTE1</name><description>[-0.4/0.6] Relative abundance, 5853{AA} line, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]LTE2</name><description>[-0.45/0.8] Relative abundance, 6141{AA} line, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]NLTE2</name><description>[-0.55/0.69] Relative abundance, 6141{AA} line, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]LTE</name><description>[-0.34/0.76] Relative abundance, combined, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Ba/Fe]LTE</name><description>[0/0.16] Uncertainty in [Ba/Fe]-LTE</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>[Ba/Fe]NLTE</name><description>[-0.38/0.64] Relative abundance, combined, assuming LTE</description><ucd>phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_[Ba/Fe]NLTE</name><description>[0/0.19] Uncertainty in [Ba/Fe]-NLTE</description><ucd>stat.error;phys.abund</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>B16</name><description>Display data from Brewer+, 2016, J/ApJS/225/32</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>