J/ApJ/958/45ivo://CDS.VizieR/J/ApJ/958/45doi:10.26093/cds/vizier/ba-xy-1dCDSKirby E.N.Ji A.P.Kovalev M.2026-07-02T12:01:01Z2026-02-06T17:13:18ZCDS support team

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

cds-question@unistra.frvisible-astronomyspectroscopychemical-abundancesline-intensitiestwo-color-diagramsradial-velocityWhereas light-element abundance variations are a hallmark of globular clusters, there is little evidence for variations in neutron-capture elements. A significant exception is M15, which shows a star-to-star dispersion in neutron-capture abundances of at least one order of magnitude. The literature contains evidence both for and against a neutron-capture dispersion in M92. We conducted an analysis of archival Keck/HIRES spectra of 35 stars in M92, 29 of which are giants, which we use exclusively for our conclusions. M92 conforms to the abundance variations typical of massive clusters. Like other globular clusters, its neutron-capture abundances were generated by the r-process. We confirm a star-to-star dispersion in r-process abundances. Unlike M15, the dispersion is limited to "first-generation" (low-Na, high-Mg) stars, and the dispersion is smaller for Sr, Y, and Zr than for Ba and the lanthanides. This is the first detection of a relation between light-element and neutron-capture abundances in a globular cluster. We propose that a source of the main r-process polluted the cluster shortly before or concurrently with the first generation of star formation. The heavier r-process abundances were inhomogeneously distributed while the first-generation stars were forming. The second-generation stars formed after several crossing times (~0.8Myr); hence, the second generation shows no r-process dispersion. This scenario imposes a minimum temporal separation of 0.8 Myr between the first and second generations.2023ApJ...958...45Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/958/45CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/195 : Globular Clusters in the Milky Way (Harris, 1996)VII/202 : Globular Clusters in the Milky Way (Harris, 1997)II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)I/355 : Gaia DR3 Part 1. Main source (Gaia Collaboration, 2022)I/357 : Gaia DR3 Part 3. Non-single stars (Gaia Collaboration, 2022)J/AJ/109/218 : Catalogue of globular cluster profiles (Trager+ 1995)J/ApJ/617/1091 : La and Eu abundances in 85 stars (Simmerer+, 2004)J/AJ/129/303 : Abundances of stars in M3 and M13 (Cohen+, 2005)J/ApJS/161/304 : Star clusters in the MW and satellites (McLaughlin+, 2005)J/AJ/133/1041 : Velocities and CMT2 phot. in globular M92 (Drukier+, 2007)J/ApJ/682/1217 : Abundances in red giants in 7 GCs (Kirby+, 2008)J/A+A/490/777 : Abundances of Population II stars in NGC 6397 (Lind+, 2008)J/A+A/497/497 : Physical param. from JHK flux (Gonzalez-Hernandez+, 2009)J/ApJ/705/328 : Abundance measurements in Sculptor dSph (Kirby+, 2009)J/A+A/503/541 : Li in late-type stars non-LTE calculations (Lind+, 2009)J/ApJ/740/60 : EWs for NGC2419 and NGC7099 RGB stars (Cohen+, 2011)J/AJ/142/22 : Heavy-element dispersion in M92 (Roederer+, 2011)J/AJ/141/175 : Abundances in M15 RGB/RHB stars (Sobeck+, 2011)J/A+A/546/A90 : NLTE analysis of Sr lines (Bergemann+, 2012)J/ApJ/760/86 : Equivalent widths for 13 NGC2419 RGB stars (Cohen+, 2012)J/ApJ/769/40 : Potassium abundance in red giants of GCs (Carretta+, 2013)J/ApJ/769/57 : Equivalent widths of metal-poor stars (Frebel+, 2013)J/ApJ/778/149 : Abundances for 3 stars in Sgr dSph (McWilliam+, 2013)J/ApJ/801/125 : Carbon in red giants in GCs and dSph galaxies (Kirby+, 2015)J/A+A/581/A70 : Grid of NLTE EW & NLTE corr. BaII lines (Korotin+, 2015)J/MNRAS/450/815 : Red giants in NGC 5286 (Marino+, 2015)J/MNRAS/449/3889 : Abundances of 15 stars in NGC 4833 (Roederer+, 2015)J/ApJ/817/41 : Abundances of 4 metal-poor red giants in BooII (Ji+, 2016)J/A+A/600/A104 : Potassium abundance in 3 GCs (Mucciarelli+, 2017)J/A+A/616/A10 : Open clusters GaiaDR2 HR diagrams (Gaia Collaboration, 2018)J/MNRAS/482/5138 : Gal. GC mean proper motions & velocities (Baumgardt+, 2019)J/A+A/631/A80 : Mn lines 3D NLTE formation in stars (Bergemann+, 2019)J/A+A/622/A191 : 885 globular cluster giants abundances (Masseron+, 2019)J/A+A/627/A177 : Non-LTE analysis of K I in late-type stars (Reggiani+, 2019)J/ApJS/249/30 : R-Process Alliance: metal-poor star sp. (Holmbeck+, 2020)J/AJ/160/181 : Chemical abundances in red giants with Magellan (Ji+, 2020)J/MNRAS/492/1641 : APOGEE southern GCs with the BACCHUS code (Meszaros+, 2020)J/ApJ/928/L11 : Atmospheric param. of giants in o Cen (Alvarez Garay+, 2022)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/958/45https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/958/45http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/958/45https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/958/45https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/958/45http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/958/45GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/958/45/stars (Photometry (Table 1), model atmosphere parameters (Table 3) and abundance trends (Table 5))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/958/45/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/958/45/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/958/45/stars?GETtext/xml+votable180.050000true259.340458343.21483330.0055555555555555566/9664 9666https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/958/45?format=asciiOpticaldefaultJ/ApJ/958/45/starsPhotometry (Table 1), model atmosphere parameters (Table 3) and abundance trends (Table 5)SimbadSimbad column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar identifiermeta.id;meta.maincharprimaryf_Star[*] * = AGB starmeta.codecharGaiaGaia DR3 identifiermeta.idRAJ2000[17] Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000[43] Degree of Declination (J2000)pos.eq.dec;meta.mainG0mag[11.5/18.2] Extinction corrected Gaia DR3 G-band magnitude (1)magphot.mag;arith.diff;em.opt.BfloatBP-RP0[0.5/1.6] Extinction corrected Gaia DR3 BP-RP color (1)magphot.color;em.opt.B;em.opt.Rfloatf_BP-RP0A = BP-RP0 Color used for calculating Teffmeta.codecharBP-Ks0[2/3.4]? Extinction corrected Gaia BP-Ks 2MASS color (1)phot.color;em.opt;em.IR.Kfloatnullablef_BP-Ks0A = BP-Ks0 Color used for Teffmeta.codecharRVel[-132.5/-110.6] Measured radial velocity, {nu}_r_km/sspect.dopplerVelocdoubleTeff[4187/6573] Surface effective temperatureKphys.temperature.effectiveinte_Teff[50/98] Uncertainty in TeffKstat.error;phys.temperature.effectiveintlogg[0.48/4.1] log of surface gravitylog(cm.s**-2)phys.gravityfloate_logg[0.1] Uncertainty in logglog(cm.s**-2)stat.error;phys.gravityfloatvt[1.2/3] Microturbulent velocitykm/sphys.velocfloate_vt[0.06/0.4] Uncertainty in vtkm/sstat.error;phys.velocfloat[Fe1/H][-2.71/-2.29] Metallicity (3)phys.abund.Fefloatdeps/dlogRW[0/0.01] Slope of abundances, {epsilon}, measured from Fe I lines vs logRWarith.grad;phys.abundfloatdeps/dEP[-0.07/0.01] Slope of abundances, {epsilon}, measured from Fe I lines vs Excitation Potentialarith.grad;phys.abundfloatdepsFe[-0.22/0.07] Difference, mean iron abundance between neutral (Fe I) and singly ionized Fe lines (Fe II)phys.abund.Fe;arith.difffloatNObsNumber of archival observations for this star (link to Table 2)meta.numberintnullableNabundNumber of abundance measurements for this star (link to Table 6)meta.numberintnullableEWsDisplay the equivalent width measurements for this star (link to Table 4)meta.ref.urlcharJ/ApJ/958/45/table2Archival observationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStar identifiermeta.id;meta.maincharf_Star[*] * : AGB starmeta.codecharDateDate of observation (UT)time.epochnullablePIPI of the observationobs.observercharSlit[0.86/1.15] Slit widtharcsecinstr.setupfloatExpIndividual Exposure timestime.duration;obs.exposurecharTExp[13/577] Total exposure timemintime.duration;obs.exposureintS/N[47/181] Signal-to-noise ratio between 4650 and 4800{AA} (2)pixel**-1stat.snrintJ/ApJ/958/45/table4Line list with equivalent widths and abundancesEW7[1.8/332.2]? Equivalent width in star XII-80.1pmspect.line.eqWidthfloatnullableweight16[0.2/76.9]? Line weight in star XII-34stat.weight;spect.linefloatnullableabund26[-0.9/7.14]? Abundance in star G17181_0638phys.abundfloatnullableweight26[1.4/37.4]? Line weight in star G17181_0638stat.weight;spect.linefloatnullablel_abund34Upper limit flag on abund34meta.code.errorcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElementElementphys.atmol.elementcharIonIonization statephys.atmol.ionStagecharlambda[3729.8/7789] Wavelength in Angstrom0.1nmem.wlfloatEP[0/5.1] Excitation potentialeVphys.atmol.excitationfloatloggf[-10.2/0.6] Log of oscillator strengthphys.atmol.oscStrengthfloatl_EW1Upper limit flag on EW1meta.code.errorcharEW1[2/388.2]? Equivalent width in star III-13 in m{AA}0.1pmspect.line.eqWidthfloatnullablel_abund1Upper limit flag on abund1meta.code.errorcharabund1[-1.75/6.1]? Abundance in star III-13phys.abundfloatnullableweight1[0.26/86.8]? Line weight in star III-13stat.weight;spect.linefloatnullablel_EW2Upper limit flag on EW2meta.code.errorcharEW2[1.5/408]? Equivalent width in star VII-180.1pmspect.line.eqWidthfloatnullablel_abund2Upper limit flag on abund2meta.code.errorcharabund2[-1.64/6.15]? Abundance in star VII-18phys.abundfloatnullableweight2[0.36/85.33]? Line weight in star VII-18stat.weight;spect.linefloatnullablel_EW3Upper limit flag on EW3meta.code.errorcharEW3[5.3/356]? Equivalent width in star X-490.1pmspect.line.eqWidthfloatnullablel_abund3Upper limit flag on abund3meta.code.errorcharabund3[-1.9/5.8]? Abundance in star X-49phys.abundfloatnullableweight3[0.1/85]? Line weight in star X-49stat.weight;spect.linefloatnullablel_EW4Upper limit flag on EW4meta.code.errorcharEW4[2.3/360.4]? Equivalent width in star III-650.1pmspect.line.eqWidthfloatnullablel_abund4Upper limit flag on abund4meta.code.errorcharabund4[-1.63/5.9]? Abundance in star III-65phys.abundfloatnullableweight4[0.3/85.5]? Line weight in star III-65stat.weight;spect.linefloatnullablel_EW5Upper limit flag on EW5meta.code.errorcharEW5[6.2/396.7]? Equivalent width in star VII-1220.1pmspect.line.eqWidthfloatnullablel_abund5Upper limit flag on abund5meta.code.errorcharabund5[-1.76/7.22]? Abundance in star VII-122phys.abundfloatnullableweight5[0.06/82.51]? Line weight in star VII-122stat.weight;spect.linefloatnullablel_EW6Upper limit flag on EW6meta.code.errorcharEW6[1.1/358]? Equivalent width in star II-530.1pmspect.line.eqWidthfloatnullablel_abund6Upper limit flag on abund6meta.code.errorcharabund6[-1.7/6.61]? Abundance in star II-53phys.abundfloatnullableweight6[0.28/84]? Line weight in star II-53stat.weight;spect.linefloatnullablel_abund7Upper limit flag on abund7meta.code.errorcharabund7[-1.6/7]? Abundance in star XII-8phys.abundfloatnullableweight7[0.01/85.14]? Line weight in star XII-8stat.weight;spect.linefloatnullablel_EW8Upper limit flag on EW8meta.code.errorcharEW8[2.3/337]? Equivalent width in star V-450.1pmspect.line.eqWidthfloatnullablel_abund8Upper limit flag on abund8meta.code.errorcharabund8[-1.8/6.93]? Abundance in star V-45phys.abundfloatnullableweight8[0.06/81.7]? Line weight in star V-45stat.weight;spect.linefloatnullablel_EW9Upper limit flag on EW9meta.code.errorcharEW9[2.9/310.1]? Equivalent width in star XI-190.1pmspect.line.eqWidthfloatnullablel_abund9Upper limit flag on abund9meta.code.errorcharabund9[-1.65/6.9]? Abundance in star XI-19phys.abundfloatnullableweight9[0.34/84.31]? Line weight in star XI-19stat.weight;spect.linefloatnullablel_EW10Upper limit flag on EW10meta.code.errorcharEW10[2.3/316.2]? Equivalent width in star XI-800.1pmspect.line.eqWidthfloatnullablel_abund10Upper limit flag on abund10meta.code.errorcharabund10[-1.71/6.5]? Abundance in star XI-80phys.abundfloatnullableweight10[0.19/78.8]? Line weight in star XI-80stat.weight;spect.linefloatnullablel_EW11Upper limit flag on EW11meta.code.errorcharEW11[4.2/335.6]? Equivalent width in star II-700.1pmspect.line.eqWidthfloatnullablel_abund11Upper limit flag on abund11meta.code.errorcharabund11[-1.65/7.1]? Abundance in star II-70phys.abundfloatnullableweight11[0.23/75]? Line weight in star II-70stat.weight;spect.linefloatnullablel_EW12Upper limit flag on EW12meta.code.errorcharEW12[1.8/291]? Equivalent width in star IV-940.1pmspect.line.eqWidthfloatnullablel_abund12Upper limit flag on abund12meta.code.errorcharabund12[-1.6/6.81]? Abundance in star IV-94phys.abundfloatnullableweight12[0.12/76.31]? Line weight in star IV-94stat.weight;spect.linefloatnullablel_EW13Upper limit flag on EW13meta.code.errorcharEW13[2.3/305.6]? Equivalent width in star I-670.1pmspect.line.eqWidthfloatnullablel_abund13Upper limit flag on abund13meta.code.errorcharabund13[-1.5/5.75]? Abundance in star I-67phys.abundfloatnullableweight13[0.1/71]? Line weight in star I-67stat.weight;spect.linefloatnullablel_EW14Upper limit flag on EW14meta.code.errorcharEW14[2.7/278.6]? Equivalent width in star III-820.1pmspect.line.eqWidthfloatnullablel_abund14Upper limit flag on abund14meta.code.errorcharabund14[-1.67/6.65]? Abundance in star III-82phys.abundfloatnullableweight14[0.08/80.53]? Line weight in star III-82stat.weight;spect.linefloatnullablel_EW15Upper limit flag on EW15meta.code.errorcharEW15[1/365]? Equivalent width in star IV-100.1pmspect.line.eqWidthfloatnullablel_abund15Upper limit flag on abund15meta.code.errorcharabund15[-1.96/7.13]? Abundance in star IV-10phys.abundfloatnullableweight15[0.34/73.54]? Line weight in star IV-10stat.weight;spect.linefloatnullablel_EW16Upper limit flag on EW16meta.code.errorcharEW16[0.9/256.5]? Equivalent width in star XII-340.1pmspect.line.eqWidthfloatnullablel_abund16Upper limit flag on abund16meta.code.errorcharabund16[-1.63/6.65]? Abundance in star XII-34phys.abundfloatnullableEW17[1.7/304.7]? Equivalent width in star IV-790.1pmspect.line.eqWidthfloatnullablel_abund17Upper limit flag on abund17meta.code.errorcharabund17[-1.6/6.7]? Abundance in star IV-79phys.abundfloatnullableweight17[0.1/75.9]? Line weight in star IV-79stat.weight;spect.linefloatnullablel_EW18Upper limit flag on EW18meta.code.errorcharEW18[1.0/273.2]? Equivalent width in star IX-130.1pmspect.line.eqWidthfloatnullablel_abund18Upper limit flag on abund18meta.code.errorcharabund18[-1.57/5.61]? Abundance in star IX-13phys.abundfloatnullableweight18[0.07/66.7]? Line weight in star IX-13stat.weight;spect.linefloatnullablel_EW19Upper limit flag on EW19meta.code.errorcharEW19[0.9/254]? Equivalent width in star VIII-240.1pmspect.line.eqWidthfloatnullablel_abund19Upper limit flag on abund19meta.code.errorcharabund19[-1.71/5.9]? Abundance in star VIII-24phys.abundfloatnullableweight19[0.13/65.15]? Line weight in star VIII-24stat.weight;spect.linefloatnullablel_EW20Upper limit flag on EW20meta.code.errorcharEW20[2.3/248.2]? Equivalent width in star X-200.1pmspect.line.eqWidthfloatnullablel_abund20Upper limit flag on abund20meta.code.errorcharabund20[-1.45/7.11]? Abundance in star X-20phys.abundfloatnullableweight20[0.18/62.7]? Line weight in star X-20stat.weight;spect.linefloatnullablel_EW21Upper limit flag on EW21meta.code.errorcharEW21[0.5/288.2]? Equivalent width in star S27100.1pmspect.line.eqWidthfloatnullablel_abund21Upper limit flag on abund21meta.code.errorcharabund21[-1.65/7.4]? Abundance in star S2710phys.abundfloatnullableweight21[0.08/72.7]? Line weight in star S2710stat.weight;spect.linefloatnullablel_EW22Upper limit flag on EW22meta.code.errorcharEW22[0.7/209.7]? Equivalent width in star VI-900.1pmspect.line.eqWidthfloatnullablel_abund22Upper limit flag on abund22meta.code.errorcharabund22[-1.57/7.03]? Abundance in star VI-90phys.abundfloatnullableweight22[0.5/68.3]? Line weight in star VI-90stat.weight;spect.linefloatnullablel_EW23Upper limit flag on EW23meta.code.errorcharEW23[0.4/267.3]? Equivalent width in star S22650.1pmspect.line.eqWidthfloatnullablel_abund23Upper limit flag on abund23meta.code.errorcharabund23[-1.63/7.52]? Abundance in star S2265phys.abundfloatnullableweight23[0.01/64]? Line weight in star S2265stat.weight;spect.linefloatnullablel_EW24Upper limit flag on EW24meta.code.errorcharEW24[0.6/272]? Equivalent width in star VIII-450.1pmspect.line.eqWidthfloatnullablel_abund24Upper limit flag on abund24meta.code.errorcharabund24[-1.4/6.8]? Abundance in star VIII-45phys.abundfloatnullableweight24[0.04/66]? Line weight in star VIII-45stat.weight;spect.linefloatnullablel_EW25Upper limit flag on EW25meta.code.errorcharEW25[0.7/248.5]? Equivalent width in star VII-280.1pmspect.line.eqWidthfloatnullablel_abund25Upper limit flag on abund25meta.code.errorcharabund25[-1.5/6.9]? Abundance in star VII-28phys.abundfloatnullableweight25[0.01/62.55]? Line weight in star VII-28stat.weight;spect.linefloatnullablel_EW26Upper limit flag on EW26meta.code.errorcharEW26[1.7/253.1]? Equivalent width in star G17181_06380.1pmspect.line.eqWidthfloatnullablel_abund26Upper limit flag on abund26meta.code.errorcharl_EW27Upper limit flag on EW27meta.code.errorcharEW27[0.1/235.4]? Equivalent width in star C17333_08320.1pmspect.line.eqWidth;em.UV.100-200nmfloatnullablel_abund27Upper limit flag on abund27meta.code.errorcharabund27[-1.41/7.41]? Abundance in star C17333_0832phys.abundfloatnullableweight27[0.16/59.71]? Line weight in star C17333_0832stat.weight;spect.linefloatnullablel_EW28Upper limit flag on EW28meta.code.errorcharEW28[0.7/268]? Equivalent width in star S31080.1pmspect.line.eqWidthfloatnullablel_abund28Upper limit flag on abund28meta.code.errorcharabund28[-1.25/8.01]? Abundance in star S3108phys.abundfloatnullableweight28[0.36/52.6]? Line weight in star S3108stat.weight;spect.linefloatnullablel_EW29Upper limit flag on EW29meta.code.errorcharEW29[1.2/286.3]? Equivalent width in star S6520.1pmspect.line.eqWidthfloatnullablel_abund29Upper limit flag on abund29meta.code.errorcharabund29[-1.3/7.6]? Abundance in star S652phys.abundfloatnullableweight29[0.17/51.04]? Line weight in star S652stat.weight;spect.linefloatnullablel_EW30Upper limit flag on EW30meta.code.errorcharEW30[1.2/202.8]? Equivalent width in star S190.1pmspect.line.eqWidthfloatnullablel_abund30Upper limit flag on abund30meta.code.errorcharabund30[-1.1/8.62]? Abundance in star S19phys.abundfloatnullableweight30[0.2/61]? Line weight in star S19stat.weight;spect.linefloatnullablel_EW31Upper limit flag on EW31meta.code.errorcharEW31[1.3/181.7]? Equivalent width in star D210.1pmspect.line.eqWidthfloatnullablel_abund31Upper limit flag on abund31meta.code.errorcharabund31[-0.77/7.95]? Abundance in star D21phys.abundfloatnullableweight31[0.44/54.2]? Line weight in star D21stat.weight;spect.linefloatnullablel_EW32Upper limit flag on EW32meta.code.errorcharEW32[1.5/165.3]? Equivalent width in star S38800.1pmspect.line.eqWidthfloatnullablel_abund32Upper limit flag on abund32meta.code.errorcharabund32[-0.83/8.56]? Abundance in star S3880phys.abundfloatnullableweight32[0.08/52.42]? Line weight in star S3880stat.weight;spect.linefloatnullablel_EW33Upper limit flag on EW33meta.code.errorcharEW33[1.0/162.6]? Equivalent width in star S40380.1pmspect.line.eqWidthfloatnullablel_abund33Upper limit flag on abund33meta.code.errorcharabund33[-0.87/8.27]? Abundance in star S4038phys.abundfloatnullableweight33[0.3/43.01]? Line weight in star S4038stat.weight;spect.linefloatnullablel_EW34Upper limit flag on EW34meta.code.errorcharEW34[1/123.3]? Equivalent width in star S610.1pmspect.line.eqWidthfloatnullableabund34[-0.97/8.13]? Abundance in star S61phys.abundfloatnullableweight34[0.17/51.38]? Line weight in star S61stat.weight;spect.linefloatnullablel_EW35Upper limit flag on EW35meta.code.errorcharEW35[2.2/138.7]? Equivalent width in star S1620.1pmspect.line.eqWidthfloatnullablel_abund35Upper limit flag on abund35meta.code.errorcharabund35[-0.74/9.01]? Abundance in star S162phys.abundfloatnullableweight35[0.15/49]? Line weight in star S162stat.weight;spect.linefloatnullablel_EW7Upper limit flag on EW7meta.code.errorcharl_EW17Upper limit flag on EW17meta.code.errorcharJ/ApJ/958/45/table6AbundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStarStarmeta.id;meta.maincharf_Star[*] * = AGB starmeta.codecharElElement or featurephys.atmol.elementcharIonState, I-neutral; II-singly ionizedphys.atmol.ionStagecharsynElements measured with spectral synthesismeta.codecharNl[0/53]? Number of lines used in the abundance determinationsmeta.numberintnullablel_[X/Fe]Limit flag for [X/Fe]meta.code.error;phys.abundchar[X/Fe][-3.36/2.79]? Abundances relative to Fe (1)log(Sun)phys.abundfloatnullablee_[X/Fe][0.03/0.43]? Uncertainty in [X/Fe]log(Sun)stat.error;phys.abundfloatnullable