J/A+A/583/A135ivo://CDS.VizieR/J/A+A/583/A135doi:10.26093/cds/vizier.35830135CDSBiazzo K.Gratton R.Desidera S.Lucatello S.Sozzetti A.Bonomo A.S.,Damasso M.Gandolfi D.Affer L.Boccato C.Borsa F.Claudi R.,Cosentino R.Covino E.Knapic C.Lanza A.F.Maldonado J.Marzari F.,Micela G.Molaro P.Pagano I.Pedani M.Pillitteri I.Piotto G.,Poretti E.Rainer M.Santos N.C.Scandariato G.Zanmar Sanchez R.2018-05-11T09:51:18Z2015-11-05T08:57:47ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frmultiple-starssolar-system-planetsspectroscopyBinary stars hosting exoplanets are a unique laboratory where chemical tagging can be performed to measure with high accuracy the elemental abundances of both stellar components, with the aim to investigate the formation of planets and their subsequent evolution. Here, we present a high-precision differential abundance analysis of the XO-2 wide stellar binary based on high resolution HARPS-N@TNG spectra. Both components are very similar K-dwarfs and host planets. Since they formed presumably within the same molecular cloud, we expect they should possess the same initial elemental abundances. We investigate if the presence of planets can cause some chemical imprints in the stellar atmospheric abundances. We measure abundances of 25 elements for both stars with a range of condensation temperature T_C_=40-1741K, achieving typical precisions of ~0.07dex. The North component shows abundances in all elements higher by +0.067+/-0.032dex on average, with a mean difference of +0.078dex for elements with T_C_>800K. The significance of the XO-2N abundance difference relative to XO-2S is at the 2{sigma} level for almost all elements. We discuss the possibility that this result could be interpreted as the signature of the ingestion of material by XO-2N or depletion in XO-2S due to locking of heavy elements by the planetary companions. We estimate a mass of several tens of M_{earth}_ in heavy elements. The difference in abundances between XO-2N and XO-2S shows a positive correlation with the condensation temperatures of the elements, with a slope of (4.7+/-0.9)x10^-5^dex/K, which could mean that both components have not formed terrestrial planets, but that first experienced the accretion of rocky core interior to the subsequent giant planets.2015A&A...583A.135Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/583/A135CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/770/36 : APOSTLE transits of XO-2 system (Kundurthy+, 2013)J/A+A/554/A28 : Qatar-1 differential light curve (Covino+, 2013)J/A+A/575/A111 : GAPS V: Global analysis of the XO-2 system (Damasso+, 2015)J/A+A/575/L15 : TrES-4b RV and Ic curves (Sozzetti+, 2015)J/A+A/578/A64 : tau Bootis A radial velocity curve (Borsa+, 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/583/A135https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/583/A135http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/583/A135https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/583/A135https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/583/A135http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/583/A135GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/583/A135/list (List of spectra)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/583/A135/list?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/583/A135/list?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/583/A135/list?GETtext/xml+votable180.050000true117.026958350.22583330.005555555555555556Associated datahttps://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/583/A1356/6638https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/583/A135?format=asciidefaultJ/A+A/583/A135/listList of spectrarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNxNumber of pointsmeta.numberintblambdaLower value of wavelength interval0.1nmem.wlintBlambdaUpper value of wavelength interval0.1nmem.wlintdlambdaSpectral resolution0.1nmspect.resolutionfloatsizeSize of the fits fileKibytephys.size;meta.fitsintspShow the spectrummeta.ref.urlcharFileNameName of the fits file in subdirectory fitsmeta.id;meta.fitscharTitleTitle of the filemeta.title;meta.filecharAssocDataAssociated Data web pagemeta.bib.pagechar