J/A+A/516/A46ivo://CDS.VizieR/J/A+A/516/A46doi:10.26093/cds/vizier.35160046CDSMashonkina L.Christlieb N.Barklem P.S.Hill V.Beers T.C.,Velichko A.2010-11-27T07:26:41Z2010-11-05T14:11:36ZCDS support team

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

cds-question@unistra.frgiant-starsspectroscopychemical-abundancesline-intensitiesWe present a detailed abundance analysis of a strongly r-process enhanced giant star discovered in the HERES project, HE 2327-5642, for which [Fe/H]=-2.78, [r/Fe]=+0.99 [r = elements from r-process]. We determined the stellar parameters and element abundances by analyzing the high-quality VLT/UVES spectra. The surface gravity was calculated from the non-local thermodynamic equilibrium (NLTE) ionization balance between FeI, and FeII, and CaI and CaII.2010A&A...516A..46Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/516/A46CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJS/168/128 : UBVRcIc photometry of FHB and metal-poor stars (Beers+, 2007)J/A+A/439/129 : HERES II. Spectroscopic analysis (Barklem+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/516/A46https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/516/A46http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/516/A46https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/516/A46https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/516/A46http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/516/A46GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/516/A46/refsReferencesComCommentsmeta.notecharAutAuthor's namemeta.bib.authorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRefReference codemeta.notecharBibCodeBibCodemeta.bib.bibcodecharJ/A+A/516/A46/table5Summary of the abundances of HE 2327-5642recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZAtomic numbermeta.id;meta.mainintElAtom/molecule \linkRole{details of the lines }phys.atmol.ionStagecharprimaryepsSunSolar photosphere abundance ({epsilon}(H)=12)phys.abundfloatNlinesNumber of lines used to determine abundancemeta.numberintepsAbundance of the element in HE 2327-5642phys.abundfloatn_eps[N] N when NLTE abundancemeta.notechare_eps? rms uncertainty on epsstat.errorfloatnullable[X/Fe]? Abundance relative to ironphys.abundfloatnullableJ/A+A/516/A46/table8Line data and abundances from an analysis of HE 2327-5642recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintZAtomic numbermeta.id;meta.mainintElAtom/moleculephys.atmol.ionStagecharlambdaWavelength0.1nmem.wlfloatlambda2? Second wavelength when interval0.1nmem.wlfloatnullableEexc? Excitation energyeVphys.atmol.excitationfloatnullableloggf? Adopted gf-valuephys.absorption.coefffloatnullabler_loggfReference for loggf, in refs.dat filemeta.ref;pos.framecharepsSunSolar photosphere abundance ({epsilon}(H)=12)phys.abundfloatepsLTE? LTE abundance ({epsilon}(H)=12)phys.abundfloatnullableepsNLTE? NLTE abundance (1)({epsilon}(H)=12)phys.abundfloatnullable[X/Fe]? Abundance relative to ironphys.abundfloatnullableEW? Equivalent width (m{AA})0.1pmspect.line.eqWidthfloatnullablen_EW[Syn ] from synthetic spectrummeta.notecharG6/NH? van der Waals damping constant log({Gamma}_6_/N_H_) at 10000K.log(rad.s**-1.cm**-3)arith.zpfloatnullableModel1Model used (3)meta.id;stat.fitcharr_Model1Reference for Model1, in refs.dat filemeta.ref;pos.framecharModel2Model used (3)meta.id;stat.fitcharr_Model2Reference for Model2, in refs.dat filemeta.ref;pos.framechar