J/A+A/537/A83ivo://CDS.VizieR/J/A+A/537/A83doi:10.26093/cds/vizier.35370083CDSCaliskan S.Christlieb N.Grebel E.K.2017-12-18T07:57:20Z2012-01-13T09:19:55ZCDS support team

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

cds-question@unistra.frglobular-star-clusterschemical-abundancesgiant-starsChemical abundances of 25 elements, which include {alpha}-, iron peak-, and neutron-capture elements, in the outer halo globular cluster Palomar 14 have been determined for the nine red giants observed with the FLAMES/UVES spectrograph. The abundance pattern of Pal 14 is similar to the inner halo GCs, halo field stars, and GCs of recognized extragalactic origin, but differs from what is customarily found in dSphs field stars. The abundance properties of Pal 14 as well as those of the other outer halo GCs are thus compatible with an accretion origin from dSphs. The neutron-capture elements show an r-process signature.2012A&A...537A..83Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/537/A83CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/448/171 : BV photometry of 3 globular clusters (Hilker+, 2006)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/537/A83https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/537/A83http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/537/A83https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/537/A83https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/537/A83http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/537/A83GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/537/A83/stars (Properties and stellar parameters of target stars)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/537/A83/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/537/A83/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/537/A83/stars?GETtext/xml+votable180.050000true242.774208314.96252780.0055555555555555566/31722-317233.322582951404819e-19 3.852589004194616e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/537/A83?format=asciiOpticaldefaultJ/A+A/537/A83/starsProperties and stellar parameters of target starsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential number (<Cl* Palomar 14 H NNN> in Simbad)meta.recordintprimaryONameOther name (1)meta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainVmagV magnitudemagphot.mag;em.opt.VfloatExpTimeExposure time (in the form NNxssss)stime.duration;obs.exposurecharRVRadial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloatS/N1Signal-to-noise ratio at 5500{AA} (all spectra)stat.snrintS/N2Signal-to-noise ratio at 6630{AA} (all spectra)stat.snrintTeffEffective temperatureKphys.temperature.effectiveintloggGravity surfacelog(cm.s**-2)phys.gravityfloatxiMicroturbulent velocity {xi}km/sphys.velocfloatSimbadSimbad column added by the CDScharJ/A+A/537/A83/tableaLinelist for the 9 red giants targeted with FLAMES/UVES (individual equivalent widths and abundances, table A1 & A2)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential number (<Cl* Palomar 14 H NNN> in Simbad)meta.recordintIonElement and ionization stage (I for neutral, II for ionized species)phys.atmol.ionStage;phys.atmol.ionizationcharlambdaWavelength in Angstrom0.1nmem.wlfloatEPExcitation PotentialeVphys.atmol.excitationfloatloggflog of oscillator strengthphys.atmol.oscStrengthfloatEW? Equivalent width of Ionpmspect.line.eqWidthfloatnullablen_EW[syn] s when EW derived from spectral synthesis rather than equivalent width fittingmeta.notecharAbund? Abundancelog(Sun)phys.abundfloatnullable