J/A+A/562/A146ivo://CDS.VizieR/J/A+A/562/A146doi:10.26093/cds/vizier.35620146CDSIshigaki M.N.Aoki W.Arimoto N.Okamoto S.2018-01-30T07:18:08Z2014-02-24T07:05:07ZCDS support team

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

cds-question@unistra.frgiant-starsline-intensitieschemical-abundancesWe determine chemical compositions of six red giant stars in the Bootes I dwarf spheroidal galaxy, based on the high-resolution spectra obtained with the High Dispersion Spectrograph mounted on the Subaru Telescope. Abundances of 12 elements, including C, Na, alpha, Fe-peak, and neutron capture elements, were determined for the sample stars. The abundance results were compared to those in field Milky Way halo stars previously obtained using an abundance analysis technique similar to the present study. We confirm the low metallicity of Boo-094 ([Fe/H]=-3.4). Except for this star, the abundance ratios ([X/Fe]) of elements lighter than zinc are generally homogeneous with small scatter around the mean values in the metallicities spanned by the other five stars (-2.7<[Fe/H]<-1.8). Specifically, all of the sample stars with [Fe/H]>-2.7 show no significant enhancement of carbon. The [Mg/Fe] and [Ca/Fe] ratios are almost constant with a modest decreasing trend with increasing [Fe/H] and are slightly lower than the field halo stars. The [Sr/Fe] and [Sr/Ba] ratios also tend to be lower in the Bootes I stars than in the halo stars. Our results of small scatter in the [X/Fe] ratios for elements lighter than zinc suggest that these abundances were homogeneous among the ejecta of prior generation(s) of stars in this galaxy.2014A&A...562A.146Ihttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/562/A146CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/562/A146https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/562/A146http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/562/A146https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/562/A146https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/562/A146http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/562/A146GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/562/A146/stars (List of studied stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/562/A146/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/562/A146/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/562/A146/stars?GETtext/xml+votable180.050000true209.953333314.32863890.0055555555555555566/8745 18553 40222https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/562/A146?format=asciiOpticaldefaultJ/A+A/562/A146/starsList of studied starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName, as in table4.datmeta.id;meta.maincharprimaryRAJ2000Simbad Hour of Right Ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Simbad Degree of Declination (J2000.0)pos.eq.dec;meta.mainBmag? Simbad B band magnitudemagphot.mag;em.opt.BfloatnullableVmag? Simbad V band magnitudemagphot.mag;em.opt.VfloatnullableSNameSimbad namemeta.idcharJ/A+A/562/A146/table4Equivalent widths and abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameObject namemeta.id;meta.maincharZ[11/56] Atomic numbermeta.idintIonState of ionization (1=neutral)phys.atmol.ionStageintlambdaWavelength of line ({AA})0.1nmem.wl;spect.linefloatchi.exExcitation potential {chi}eVphys.atmol.excitationfloatloggfOscillator strengthphys.atmol.oscStrengthfloatEWEquivalent width (m{AA})0.1pmspect.line.eqWidthfloatAbundAbsolute abundance (log scale, A(H)=12)phys.abundfloat