J/AZh/96/267ivo://CDS.VizieR/J/AZh/96/267CDSMarsakov V.A.Koval' V.V.Gozha M.L.2019-05-10T12:19:20Z2019-05-06T09:29:00ZCDS support team

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

cds-question@unistra.frmilky-way-galaxyglobular-star-clusterschemical-abundancesradial-velocityFor the catalog, we compiled the abundances of 28 chemical elements: alpha-elements (O, Mg, Si, Ca, Ti), carbon, iron-peak elements(Sc, V, Cr, Mn, Fe, Co, Ni, Cu, Zn), slow and rapid neutron-capture elements (Sr, Y, Zr, Mo, Ba, La, Ce, Nd, Eu, Dy) and three odd-Z elements(Na, Al, K) in the stars of 69 globular clusters. The data are taken from 101 papers published from 1986 to 2018. The abundances of chemical elements in stars of the clusters in almost all the used papers are determined from high-resolution spectra obtained mainly for the atmospheres of red giants. The spectra are analyzed with the local thermodynamic equilibrium approximation.2019AZh....96..267Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AZh/96/267CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/271 : Properties of Galactic Globular Clusters (Francis+, 2014)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AZh/96/267https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AZh/96/267http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AZh/96/267https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AZh/96/267https://vizier.iucaa.in/viz-bin/votable?-source=J/AZh/96/267http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AZh/96/267GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AZh/96/267/table1 (The catalogue data for 157 globular clusters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AZh/96/267/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AZh/96/267/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AZh/96/267/table1?GETtext/xml+votable180.050000true6.0223292-72.08144440.0055555555555555566/1133 3950 6212 6389 9436 9666 10008 10321 10336 12405 12425 12531 12943 14489 16647 17121 17711 19091 20001 21017 24843 25873 27237 27852 27981 27986 28067 28577 28705 28717 28741 28751 28768 28769 28778 28781 28805 28808 28815 28817 28833 28835 28838 28855 28867 28868 28876 28877 28882 28889 28895 28903 28905 28959 28962 28970 28973 28974 29077 29090 29097 29113 29184 29187 29195 29202 29216 29222 29231 29233 29248 29267 29289 29294 29318 29377 29626 29632 29636 29637 29816 29870 30269 30321 30323 30378 30769 30998 31019 31043 31095 31115 31128 31398 31417 31723 32083 33321 33330 33635 34242 34317 34811 36971 37294 38465 39642 39954 41011 41257 41304 41507 41522 41847 41852 42076 42152 42204 42278 42314 42320 42361 42466 42528 42700 42761 42789 42841 42862 42955 42958 42990 43125 43193 43227 43894 44086 44220 44427 47125 47620 47745 47777 47825 47866 47868 47903 47916 47935 47971 48035 48434 48444 48698 48952https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AZh/96/267?format=asciidefaultJ/AZh/96/267/table2The catalogue (continuation)e_[La/Fe]? Dispersion for [La/Fe]log(Sun)stat.error;phys.abundfloatnullablee_[Ba/Fe]? Dispersion for [Ba/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ce/Fe]? Abundance [Ce/Fe]log(Sun)phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster identification numbermeta.id;phys.atmol.numbercharNameOther commonly used cluster namemeta.id;meta.mainchar[Co/Fe]? Abundance [Co/Fe]log(Sun)phys.abundfloatnullablee_[Co/Fe]? Dispersion for [Co/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ni/Fe]? Abundance [Ni/Fe]log(Sun)phys.abundfloatnullablee_[Ni/Fe]? Dispersion for [Ni/Fe]log(Sun)stat.error;phys.abundfloatnullable[Cu/Fe]? Abundance [Cu/Fe]log(Sun)phys.abundfloatnullablee_[Cu/Fe]? Dispersion for [Cu/Fe]log(Sun)stat.error;phys.abundfloatnullable[Zn/Fe]? Abundance [Zn/Fe]log(Sun)phys.abundfloatnullablee_[Zn/Fe]? Dispersion for [Zn/Fe]log(Sun)stat.error;phys.abundfloatnullable[Sr/Fe]? Abundance [Sr/Fe]log(Sun)phys.abundfloatnullablee_[Sr/Fe]? Dispersion for [Sr/Fe]log(Sun)stat.error;phys.abundfloatnullable[Y/Fe]? Abundance [Y/Fe]log(Sun)phys.abundfloatnullablee_[Y/Fe]? Dispersion for [Y/Fe]log(Sun)stat.error;phys.abundfloatnullable[Zr/Fe]? Abundance [Zr/Fe]log(Sun)phys.abundfloatnullablee_[Zr/Fe]? Dispersion for [Zr/Fe]log(Sun)stat.error;phys.abundfloatnullable[Mo/Fe]? Abundance [Mo/Fe]log(Sun)phys.abundfloatnullablee_[Mo/Fe]? Dispersion for [Mo/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ba/Fe]? Abundance [Ba/Fe]log(Sun)phys.abundfloatnullable[La/Fe]? Abundance [La/Fe]log(Sun)phys.abundfloatnullablee_[Ce/Fe]? Dispersion for [Ce/Fe]log(Sun)stat.error;phys.abundfloatnullable[Nd/Fe]? Abundance [Nd/Fe]log(Sun)phys.abundfloatnullablee_[Nd/Fe]? Dispersion for [Nd/Fe]log(Sun)stat.error;phys.abundfloatnullable[Eu/Fe]? Abundance [Eu/Fe]log(Sun)phys.abundfloatnullablee_[Eu/Fe]? Dispersion for [Eu/Fe]log(Sun)stat.error;phys.abundfloatnullable[Dy/Fe]? Abundance [Dy/Fe]log(Sun)phys.abundfloatnullablee_[Dy/Fe]? Dispersion for [Dy/Fe]log(Sun)stat.error;phys.abundfloatnullableRefReferences for abundances, in refs.dat filemeta.refcharJ/AZh/96/267/table3Space-kinematic parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster identification numbermeta.id;phys.atmol.numbercharNameOther commonly used cluster namemeta.id;meta.maincharXHeliocentric distance towards Gal. centerkpcpos.cartesian.x;pos.galacticfloatYHeliocentric distance towards Gal. rotationkpcpos.cartesian.y;pos.galacticfloatZHeliocentric distance towards North Galactic Polekpcpos.cartesian.z;pos.galacticfloatRCRemoval from the rotation axis of the Galaxykpcpos.distancefloatRGCDistance from Galactic centerkpcpos.distance;pos.galactocentricfloatVR? Galactocentric cylindrical velocity component towards Galactic anticenterkm/sphys.veloc;pos.galactocentricintnullableVtheta? Galactocentric cylindrical velocity component towards Galactic rotationkm/sphys.veloc.rotat;pos.galactocentricintnullableVZ? Galactocentric cylindrical velocity component towards N. Galactic Polekm/sphys.veloc;pos.galactocentricintnullableHBR? Horizontal branch indexphot.mag;arith.difffloatnullableVMAG? Absolute visual magnitudemagphys.magAbs;em.opt.VfloatnullableSubSsy[1/3]? Subsystem (1)meta.codeintnullableRel[G] Genetically relatedmeta.codecharJ/AZh/96/267/refsReferences for abundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRef[1/101] Reference numbermeta.id;meta.mainintBibCodeBibCodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorcharJ/AZh/96/267/table1The catalogue data for 157 globular clustersSimbadNameSimbad column added by the CDSmeta.idcharRefReferences for abundances, in refs.dat filemeta.refcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCluster identification numbermeta.id;phys.atmol.numbercharNameOther commonly used cluster namemeta.id;meta.mainchar[Fe/H]? Abundance [Fe/H]log(Sun)phys.abund.Fefloatnullablee_[Fe/H]? Dispersion for [Fe/H]log(Sun)stat.error;phys.abund.Fefloatnullable[C/Fe]? Abundance [C/Fe]log(Sun)phys.abundfloatnullablee_[C/Fe]? Dispersion for [C/Fe]log(Sun)stat.error;phys.abundfloatnullable[O/Fe]? Abundance [O/Fe]log(Sun)phys.abundfloatnullablee_[O/Fe]? Dispersion for [O/Fe]log(Sun)stat.error;phys.abundfloatnullable[Na/Fe]? Abundance [Na/Fe]log(Sun)phys.abundfloatnullablee_[Na/Fe]? Dispersion for [Na/Fe]log(Sun)stat.error;phys.abundfloatnullable[Mg/Fe]? Abundance [Mg/Fe]log(Sun)phys.abundfloatnullablee_[Mg/Fe]? Dispersion for [Mg/Fe]log(Sun)stat.error;phys.abundfloatnullable[Al/Fe]? Abundance [Al/Fe]log(Sun)phys.abundfloatnullablee_[Al/Fe]? Dispersion for [Al/Fe]log(Sun)stat.error;phys.abundfloatnullable[Si/Fe]? Abundance [Si/Fe]log(Sun)phys.abundfloatnullablee_[Si/Fe]? Dispersion for [Si/Fe]log(Sun)stat.error;phys.abundfloatnullable[K/Fe]? Abundance [K/Fe]log(Sun)phys.abundfloatnullablee_[K/Fe]? Dispersion for [K/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ca/Fe]? Abundance [Ca/Fe]log(Sun)phys.abundfloatnullablee_[Ca/Fe]? Dispersion for [Ca/Fe]log(Sun)stat.error;phys.abundfloatnullable[Sc/Fe]? Abundance [Sc/Fe]log(Sun)phys.abundfloatnullablee_[Sc/Fe]? Dispersion for [Sc/Fe]log(Sun)stat.error;phys.abundfloatnullable[Ti/Fe]? Abundance [Ti/Fe]log(Sun)phys.abundfloatnullablee_[Ti/Fe]? Dispersion for [Ti/Fe]log(Sun)stat.error;phys.abundfloatnullable[V/Fe]? Abundance [V/Fe]log(Sun)phys.abundfloatnullablee_[V/Fe]? Dispersion for [V/Fe]log(Sun)stat.error;phys.abundfloatnullable[Cr/Fe]? Abundance [Cr/Fe]log(Sun)phys.abundfloatnullablee_[Cr/Fe]? Dispersion for [Cr/Fe]log(Sun)stat.error;phys.abundfloatnullable[Mn/Fe]? Abundance [Mn/Fe]log(Sun)phys.abundfloatnullablee_[Mn/Fe]? Dispersion for [Mn/Fe]log(Sun)stat.error;phys.abundfloatnullable_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