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<ri:Resource created="2011-09-21T11:47:03Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Abundances in two Galactic bulge stars</title><shortName>J/ApJ/699/66</shortName><identifier>ivo://CDS.VizieR/J/ApJ/699/66</identifier><altIdentifier>doi:10.26093/cds/vizier.16990066</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Cohen J.G.</name></creator><creator><name>Thompson I.B.</name></creator><creator><name>Sumi T.</name></creator><creator><name>Bond I.</name></creator><creator><name>Gould A.</name></creator><creator><name>Johnson J.A.,Huang W.</name></creator><creator><name>Burley G.</name></creator><date role="Updated">2011-10-14T14:27:09Z</date><date role="Created">2011-09-21T11:47:03Z</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>gravitational-lensing</subject><subject>dwarf-stars</subject><description>We present abundance analyses based on high dispersion and high signal-to-noise ratio Magellan spectra of two highly microlensed Galactic bulge stars in the region of the main-sequence turnoff with T_eff_~5650K. We find that MOA-2008-BLG-310S has [Fe/H]^8^=+0.41+/-0.09dex and MOA-2008-BLG-311S has +0.26+/-0.09dex. The abundance ratios for the ~20 elements for which features could be detected in the spectra of each of the two stars follow the trends with [Fe/H] found among samples of bulge giants. Combining these two bulge dwarfs with the results from previous abundance analysis of four other Galactic bulge turnoff region stars, all highly magnified by microlensing, gives a mean [Fe/H] of +0.29dex. This implies that there is an inconsistency between the Fe-metallicity distribution of the microlensed bulge dwarfs and that derived by the many previous estimates based on surveys of cool, luminous bulge giants, which have mean [Fe/H]~-0.1dex.</description><source format="bibcode">2009ApJ...699...66C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/699/66</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A41">J/A+A/512/A41 : Abundances of microlensed stars in the Bulge (Bensby+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/499/737">J/A+A/499/737 : Abundances of microlensed dwarf and subgiant stars (Bensby+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/1029">J/ApJ/682/1029 : Abundances in OGLE-2007-BLG-349S (Cohen+, 2008)</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/699/66</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/699/66</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/699/66</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/699/66</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/699/66</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/699/66</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/699/66/table4</name><description>W_{lambda}_ for the sample extremely metal-poor (EMP) stars from the Hamburg/ESO Survey (HES)</description><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 designation (MOA-2008-BLG-310S or MOA-2008-BLG-311S)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>lambda</name><description>Wavelength in Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ion</name><description>Species identification</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>ExPot</name><description>Excitation potential</description><unit>eV</unit><ucd>phys.atmol.excitation</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>log(gf)</name><description>Log of the oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW</name><description>? Equivalent width in milli-Angstroms</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>