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<ri:Resource created="2015-12-14T13:18:35Z" 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>XO-2S and XO-2N chemical composition</title><shortName>J/ApJ/808/13</shortName><identifier>ivo://CDS.VizieR/J/ApJ/808/13</identifier><altIdentifier>doi:10.26093/cds/vizier.18080013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ramirez I.</name></creator><creator><name>Khanal S.</name></creator><creator><name>Aleo P.</name></creator><creator><name>Sobotka A.</name></creator><creator><name>Liu F.</name></creator><creator><name>Casagrande L.,Melendez J.</name></creator><creator><name>Yong D.</name></creator><creator><name>Lambert D.L.</name></creator><creator><name>Asplund M.</name></creator><date role="Updated">2017-01-23T22:00:00Z</date><date role="Created">2015-12-14T13:18:35Z</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>line-intensities</subject><subject>multiple-stars</subject><subject>spectroscopy</subject><description>Using high-quality spectra of the twin stars in the XO-2 binary system, we have detected significant differences in the chemical composition of their photospheres. The differences correlate strongly with the elements' dust condensation temperature. In XO-2N, volatiles are enhanced by about 0.015dex and refractories are overabundant by up to 0.090dex. On average, our error bar in relative abundance is 0.012dex. We present an early metal-depletion scenario in which the formation of the gas giant planets known to exist around these stars are responsible for a 0.015 dex offset in the abundances of all elements while 20M_{Earth}_ of non-detected rocky objects that formed around XO-2S explain the additional refractory-element difference. An alternative explanation involves the late accretion of at least 20M_{Earth}_of planet-like material by XO-2N, allegedly as a result of the migration of the hot Jupiter detected around that star. Dust cleansing by a nearby hot star as well as age or Galactic birthplace effects can be ruled out as valid explanations for this phenomenon.</description><source format="bibcode">2015ApJ...808...13R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/808/13</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/ApJ/801/L10">J/ApJ/801/L10 : XO-2N and XO-2S equivalent widths (Teske+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/583/A135">J/A+A/583/A135 : XO-2N and XO-2S spectra (Biazzo+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/575/A111">J/A+A/575/A111 : GAPS V: Global analysis of the XO-2 system (Damasso+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A71">J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/561/A7">J/A+A/561/A7 : Abundances for stars with planets (Ramirez+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A106">J/A+A/558/A106 : Chemical abundances for 83 transit hosts (Mortier+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/770/36">J/ApJ/770/36 : APOSTLE transits of XO-2 system (Kundurthy+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/768/L12">J/ApJ/768/L12 : Abundances in host stars XO-2S and XO-2N (Teske+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A6">J/A+A/552/A6 : Abundances of F-G MS stars (Gonzalez Hernandez+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/757/161">J/ApJ/757/161 : Spectroscopy of 56 exoplanet host stars (Torres+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/141/175">J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/55">J/ApJ/732/55 : Abundances of stars with planets (Schuler+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/715/1050">J/ApJ/715/1050 : Predicted abundances for extrasolar planets. 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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>f_lambda</name><description>[-] -: no equivalent width values</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>lambda</name><description>[4218.7/8092.7] Wavelength in Angstroms</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Sp</name><description>[6/106] Numeric species code (1)</description><ucd>phys.atmol.ionStage</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExPot</name><description>[0/9.2] 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>[-6.3/0.6] Log of the oscillator strength</description><ucd>phys.atmol.oscStrength</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>XO-2N</name><description>[6/217]? Equivalent width in XO-2N (2)</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>XO-2S</name><description>[7/210]? Equivalent width in XO-2S (2)</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sun</name><description>[3/158]? Equivalent width in the Sun (2)</description><unit>1e-13m</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>