J/A+A/433/185ivo://CDS.VizieR/J/A+A/433/185doi:10.26093/cds/vizier.34330185CDSBensby T.Feltzing S.Lundstroem I.Ilyin I.2017-12-06T07:38:52Z2005-05-05T14:01:38ZCDS support team

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

cds-question@unistra.frdwarf-starschemical-abundancesFrom a detailed elemental abundance analysis of 102 F and G dwarf stars we present abundance trends in the Galactic thin and thick disks for 14 elements (O, Na, Mg, Al, Si, Ca, Ti, Cr, Fe, Ni, Zn, Y, Ba, and Eu). Stellar parameters and elemental abundances (except for Y, Ba and Eu) for 66 of the 102 stars were presented in our previous studies (Bensby et al. 2003, <J/A+A/410/527>, 2004, <J/A+A/415/155>). The 36 stars that are new in this study extend and confirm our previous results and allow us to draw further conclusions regarding abundance trends. The s-process elements Y and Ba, and the r-element Eu have also been considered here for the whole sample for the first time. To make it easier to gather the elemental abundances for all 102 stars we have included the abundance data from Bensby et al. (2003, Cat. <J/A+A/410/527>) and from Bensby et al. (2004, Cat. <J/A+A/415/155>) in table9.dat2005A&A...433..185Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/433/185CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)J/A+A/415/155 : Oxygen abundances in the Galactic disk (Bensby+, 2004)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/433/185https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/433/185http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/433/185https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/433/185https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/433/185http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/433/185GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/433/185/abund (Abundances of the studied stars (tables 8 and 9 of the paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/433/185/abund?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/433/185/abund?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/433/185/abund?GETtext/xml+votable180.050000true2.17057636.6271250.0055555555555555566/314 379 517 706 944 1452 5062 6171 6539 12621 13474 13697 14207 14419 14502 15177 16386 16679 17171 17301 17576 17606 18035 18067 18123 18614 18821 18860 19345 19547 20145 20365 20402 20446 20593 21177 21179 21809 22765 22823 23096 23201 24183 28763 28987 29210 29721 30665 30848 31029 31130 31132 31172 31619 31768 32205 32473 32552 32617 33456 33717 33774 33910 34204 34442 34446 34864 35064 35080 35533 35576 35968 36035 36126 36365 36693 37408 38918 40716 40722 41272 41764 41941 42042 42115 42248 42326 42486 42760 45364 45485 45669 46076 46593 46681 47073 47377 48065 48105 48283 48687 49114https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/433/185?format=asciiOpticaldefaultJ/A+A/433/185/table4Atomic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.intElElementcharIonIonisationcharLambdaWavelengthdoubleLEPLower excitation potentialeVfloatdgamma6? Correction factor to Unsoeld broadening (1)floatnullableDMP[SU] Method for collisional broadening (2)chargammaRadRadiation damping constants**-1doubleloggflog of oscillator strengthfloatr_loggfReference to loggf (3)charJ/A+A/433/185/abundAbundances of the studied stars (tables 8 and 9 of the paper)recnoRecord number assigned by the VizieR team. Should Not be used for identification.intHIPHipparcos (Cat. <I/239>) numberintMem[1/3] Population membership (G1)intAge? Stellar ageGyrfloatnullableAgeMin? Lower limit on stellar ageGyrfloatnullableAgeMax? Upper limit on stellar ageGyrfloatnullableSimbadSimbad column added by the CDScharInst[SFU] Instrument (1)char[Fe/H]IAbundance [Fe/H] from Fe I lineslog(Sun)float[Fe/H]IIAbundance [Fe/H] from Fe II lineslog(Sun)float[Na/H]Abundance [Na/H]log(Sun)float[Mg/H]Abundance [Mg/H]log(Sun)float[Al/H]Abundance [Al/H]log(Sun)float[Si/H]Abundance [Si/H]log(Sun)float[Ca/H]Abundance [Ca/H]log(Sun)float[Ti/H]IAbundance [Ti/H] from Ti I lineslog(Sun)float[Ti/H]IIAbundance [Ti/H] from Ti II lineslog(Sun)float[Cr/H]IAbundance [Cr/H] from Cr I lineslog(Sun)float[Cr/H]IIAbundance [Cr/H] from Cr II lineslog(Sun)float[Ni/H]Abundance [Ni/H]log(Sun)float[Zn/H]Abundance [Zn/H]log(Sun)float[Y/H]Abundance [Y/H]log(Sun)float[Ba/H]Abundance [Ba/H]log(Sun)floats[Fe/H]Ispread in [Fe/H] from Fe I lineslog(Sun)floats[Fe/H]IIspread in [Fe/H] from Fe II lineslog(Sun)floats[Na/H]spread in [Na/H]log(Sun)floats[Mg/H]spread in [Mg/H]log(Sun)floats[Al/H]spread in [Al/H]log(Sun)floats[Si/H]spread in [Si/H]log(Sun)floats[Ca/H]spread in [Ca/H]log(Sun)floats[Ti/H]Ispread in [Ti/H] from Ti I lineslog(Sun)floats[Ti/H]IIspread in [Ti/H] from Ti II lineslog(Sun)floats[Cr/H]Ispread in [Cr/H] from Cr I lineslog(Sun)floats[Cr/H]IIspread in [Cr/H] from CR II lineslog(Sun)floats[Ni/H]spread in [Ni/H]log(Sun)floats[Zn/H]spread in [Zn/H]log(Sun)floats[Y/H]spread in [Y/H]log(Sun)floats[Ba/H]spread in [Ba/H]log(Sun)floato_[Fe/H]Inumber of Fe I lines used for [Fe/H]into_[Fe/H]IInumber of Fe II lines used for [Fe/H]into_[Na/H]number of lines used for [Na/H]into_[Mg/H]number of lines used for [Mg/H]into_[Al/H]number of lines used for [Al/H]into_[Si/H]number of lines used for [Si/H]into_[Ca/H]number of lines used for [Ca/H]into_[Ti/H]Inumber of Ti I lines used for [Ti/H]into_[Ti/H]IInumber of Ti II lines used for [Ti/H]into_[Cr/H]Inumber of Cr I lines used for [Cr/H]into_[Cr/H]IInumber of Cr II lines used for [Cr/H]into_[Ni/H]number of lines used for [Ni/H]into_[Zn/H]number of lines used for [Zn/H]into_[Y/H]number of lines used for [Y/H]into_[Ba/H]number of lines used for [Ba/H]int[O/H]6300? [O/H] from forbidden O line at 630.0nm (2)log(Sun)floatnullable[O/H]6363? [O/H] from forbidden O line at 636.3nmlog(Sun)floatnullable[O/H]7771? [O/H] from permitted O line at 777.1nmlog(Sun)floatnullable[O/H]7773? [O/H] from permitted O line at 777.3nmlog(Sun)floatnullable[O/H]7774? [O/H] from permitted O line at 777.4nmlog(Sun)floatnullable[Eu/H]6645? [Eu/H] from europium line at 664.5nmlog(Sun)floatnullable[Eu/H]4129? [Eu/H] from europium line at 412.9nmlog(Sun)floatnullable_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main