J/AJ/133/2464ivo://CDS.VizieR/J/AJ/133/2464doi:10.26093/cds/vizier.51332464CDSLuck R.E.Heiter U.2017-07-04T07:08:05Z2009-06-21T12:10:07ZCDS support team

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

cds-question@unistra.frchemical-abundancesspectroscopygiant-starsWe present parameter and abundance data for a sample of 298 nearby giants. The spectroscopic data for this work have a resolution of R~60000S/N>150, and spectral coverage from 475 to 685nm. Overall trends in the Z>10 abundances are dominated by Galactic chemical evolution, while the light-element abundances are influenced by stellar evolution, as well as Galactic evolution. We find several super-Li stars in our sample and confirm that Li abundances in the first giant branch are related to mixing depths.2007AJ....133.2464Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/133/2464CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/657/241 : Spectroscopy of Leo I red giants (Koch+, 2007)J/MNRAS/382/553 : Abundances of nearby red clump giants (Liu+, 2007)J/PASJ/57/109 : Late-G giants abundances (Takeda+, 2005)J/A+A/430/165 : Radial velocities for 6691 K and M giants (Famaey+, 2005)J/A+A/409/251 : Li abundances and velocities in F and G stars (Mallik+, 2003)J/A+A/363/239 : Lithium abundances in single giant stars (de Medeiros+, 2000)J/A+AS/139/433 : RV and vsini of evolved stars (de Medeiros+ 1999)J/A+A/333/231 : O-M stars model atmospheres (Bessell+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/133/2464https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/133/2464http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/133/2464https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/133/2464https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/133/2464http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/133/2464GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/133/2464/stars (Program star parameters)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/133/2464/stars?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/133/2464/stars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/133/2464/stars?GETtext/xml+votable180.050000true1.0824756-16.52903610.0055555555555555566/4 79 210 327 329 405 737 915 946 1082 1249 1296 1360 1535 1770 1819 1877 2202 2229 2324 2440 2834 3077 3094 3208 3335 3390 3619 3755 3878 3969 4286 4574 4599 4690 4711 4761 4969 5059 5239 5530 5676 5694 5776 5950 5982 5983 5997 6166 6201 6219 6298 6361 6381 6827 7101 7113 7422 7542 7760 7771 8080 8198 8354 8523 8536 8724 8767 8845 8986 9061 9083 9127 9219 9774 10007 10161 10217 10354 10490 10549 10632 10980 11015 11370 11633 11734 12030 12176 12449 12612 12735 13099 13114 13138 13211 13643 13731 13882 14005 14109 14365 14427 14496 14557 14953 15012 15226 15237 15363 15426 15629 15882 16013 16023 16035 16100 16148 16150 16554 16667 16704 16763 17061 17159 17285 17391 17568 17608 17656 17676 17854 18166 18227 18276 18315 18619 18688 18846 18893 18907 18972 19405 19414 19427 19797 19874 19940 19985 20102 20269 20308 20677 20909 21026 21182 21221 21317 21423 21469 21612 21738 21768 21792 21885 21940 22199 22360 22453 22988 23283 23299 23547 23705 23753 23822 23875 24228 24262 24484 24820 24838 24921 24931 25092 25410 25473 25608 25741 25910 25941 25997 26137 26287 26302 26544 26552 26562 26629 26758 27366 27444 27448 27520 27752 27993 28014 28044 28104 28257 28276 28324 28634 28792 28838 28892 28934 29001 29280 29391 29521 29552 29748 29774 30024 30037 30064 30344 30431 30535 30665 30670 30681 30688 30746 30845 30953 31071 31125 31428 31534 31688 31730 31784 31902 32023 32087 32096 32172 32243 32291 32433 32458 32509 32575 32659 32731 34666 35673 36032 36070 36181 36212 36228 36433 36502 36679 39879 40048 40090 40239 40336 40355 40408 40618 40667 40690 40750 40777 42921 42956 44214 44277 44347 44372 44722 44789 45032 47067 47098 47997 48504 48572 48615 48694 48816 48992 49004https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/133/2464?format=asciiOpticaldefaultJ/AJ/133/2464/starsProgram star parametersrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHIPThe Hipparcos identification numbermeta.idintHDThe HD identification numbermeta.id;meta.mainintprimaryHR? The HR identification numbermeta.idintnullableVmagApparent V band magnitudemagphot.mag;em.opt.VfloatVMAGAbsolute V band magnitude (1)magphys.magAbs;em.opt.VfloatSpTypeSpectral type (2)src.spTypecharplxParallaxmaspos.parallax.trigfloatDistDistance from parallaxpcpos.distance;pos.heliocentricfloatGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latfloatRVRadial velocitykm/sspect.dopplerVeloc;pos.heliocentricfloate_RVError in RVkm/sstat.errorfloatr_RV[LFM] Source for RV (3)meta.ref;pos.framecharSBDe Medeiros & Mayor (1999, cat. J/A+AS/139/433) spectroscopic binary classificationmeta.codecharSimbadSimbad column added by the CDScharSTeffSpectroscopically determined effective temperatureKphys.temperature.effectiveintSlog(g)Spectroscopically determined logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatSVtSpectroscopically determined microturbulent velocitykm/sphys.velocfloatS[Fe/H]Spectroscopically determined mean logarithmic iron abundancelog(Sun)phys.abund.Fefloate_S[Fe/H]Standard deviation about Sp-[Fe/H]log(Sun)stat.error;phys.abund.Fefloato_S[Fe/H]Number of Fe I lines used to determine Sp-[Fe/H]meta.numberintMTeff? MARCS75 derived effective temperatureKphys.temperature.effectiveintnullableMlog(g)? MARCS75 derived logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatnullableMVt? MARCS75 derived microturbulent velocitykm/sphys.velocfloatnullableM[Fe/H]? MARCS75 derived mean logarithmic iron abundancelog(Sun)phys.abund.FefloatnullablePTeff? Physical approach effective temperatureKphys.temperature.effectiveintnullablePlog(g)? Physical approach logarithmic surface gravitylog(cm.s**-2)phys.gravityfloatnullablePVt? Physical approach microturbulent velocitykm/sphys.velocfloatnullableP[FeI/H]? Physical approach mean logarithmic FeI abundancelog(Sun)phys.abund.FefloatnullableP[FeII/H]? Physical approach mean logarithmic FeII abundancelog(Sun)phys.abund.Fefloatnullablee_VMAGError in VMAGmagstat.errorfloatPMass? Physical approach mass estimate (3)(2)solMassphys.massfloatnullablePMbol? Physical approach absolute bolometic magnitude estimate (2)(3)magphot.mag.bolfloatnullablePLum? Physical approach luminosity estimate (3)(2)solLumphys.luminosityfloatnullableSIMassSpectroscopic inversion mass estimate (4)(2)solMassphys.massfloatSIMbolSpectroscopic inversion absolute bolometic magnitude estimate (2)(4)magphot.mag.bolfloatSILumSpectroscopic inversion luminosity estimate (4)(2)solLumphys.luminosityfloatSIlog(g)Spectroscopic inversion logarithmic surface gravity estimate (4)(2)log(cm.s**-2)phys.gravityfloatSTMass? Spectroscopic T_eff_ mass estimate (2)(3)solMassphys.massfloatnullableSTMbol? Spectroscopic T_eff_ absolute bolometic magnitude estimate (3)(2)magphot.mag.bolfloatnullableSTLum? Spectroscopic T_eff_ luminosity estimate (3)(2)solLumphys.luminosityfloatnullableSTlog(g)? Spectroscopic T_eff_ logarithmic surface gravity estimate (3)(2)log(cm.s**-2)phys.gravityfloatnullableVelMacroturbulent or rotational velocitykm/sphys.velocfloatn_Vel[GR] Gaussian macroturbulence or Rotation Velmeta.notecharEWLiLi Equivalent width in milliAngstroms (2)1e-13mspect.line.eqWidthfloatS-LiSpectrosopic analysis Li abundance (3)phys.abundfloatM-Li? MARCS75 analysis Li abundance (3)phys.abundfloatnullableP-Li? Physical analysis Li abundance (3)phys.abundfloatnullableQFit quality (4)meta.code.qualchar_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.mainJ/AJ/133/2464/CNOCNO abundances }recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintA[SMP] Type of analysis (G1)meta.id;stat.fitcharHIPThe Hipparcos identification numbermeta.idintHDThe HD identification numbermeta.id;meta.mainintHR? The HR identification numbermeta.idintnullableC? The C number abundance (2)phys.abundfloatnullableN? The N number abundance (2)phys.abundfloatnullableO? The O number abundance (2)phys.abundfloatnullable[C/H]? Log of C/H number abundance (3)log(Sun)phys.abundfloatnullable[N/H]? Log of N/H number abundance (3)log(Sun)phys.abundfloatnullable[O/H]? Log of O/H number abundance (3)log(Sun)phys.abundfloatnullable[C/Fe]? Log of C/Fe number abundance (3)log(Sun)phys.abundfloatnullable[N/Fe]? Log of C/Fe number abundance (3)log(Sun)phys.abundfloatnullable[O/Fe]? Log of C/Fe number abundance (3)log(Sun)phys.abundfloatnullableCNO? The C+N+O number abundance (2)phys.abundfloatnullable[CNO/H]? Log of (C+N+O)/H number abundance (3)log(Sun)phys.abundfloatnullable[CNO/Fe]? Log of (C+N+O)/Fe number abundance (3)log(Sun)phys.abundfloatnullableCN? The C+N number abundance (2)phys.abundfloatnullable[CN/H]? Log of (C+N)/H number abundance (3)log(Sun)phys.abundfloatnullable[CN/Fe]? Log of (C+N)/Fe number abundance (3)log(Sun)phys.abundfloatnullableC/O? Ratio of C to O abundance [10^(C minus O)] (2)phys.abund;arith.ratiofloatnullableJ/AJ/133/2464/tables4*Average AbundancesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHDThe HD identification numbermeta.id;meta.mainintA[SMP] Type of analysis (G1)meta.id;stat.fitcharNa? Average Na abundancelog(Sun)phys.abundfloatnullableMg? Average Mg abundancelog(Sun)phys.abundfloatnullableAl? Average Al abundancelog(Sun)phys.abundfloatnullableSi? Average Si abundancelog(Sun)phys.abundfloatnullableS? Average S abundancelog(Sun)phys.abundfloatnullableCa? Average Ca abundancelog(Sun)phys.abundfloatnullableSc? Average Sc abundancelog(Sun)phys.abundfloatnullableTi? Average Ti abundancelog(Sun)phys.abundfloatnullableV? Average V abundancelog(Sun)phys.abundfloatnullableCr? Average Cr abundancelog(Sun)phys.abundfloatnullableMn? Average Mn abundancelog(Sun)phys.abundfloatnullableFe? Average Fe abundancelog(Sun)phys.abundfloatnullableCo? Average Co abundancelog(Sun)phys.abundfloatnullableNi? Average Ni abundancelog(Sun)phys.abundfloatnullableCu? Average Cu abundancelog(Sun)phys.abundfloatnullableZn? Average Zn abundancelog(Sun)phys.abundfloatnullableSr? Average Sr abundancelog(Sun)phys.abundfloatnullableY? Average Y abundancelog(Sun)phys.abundfloatnullableBa? Average Ba abundancelog(Sun)phys.abundfloatnullableLa? Average La abundancelog(Sun)phys.abundfloatnullableCe? Average Ce abundancelog(Sun)phys.abundfloatnullablePr? Average Pr abundancelog(Sun)phys.abundfloatnullableNd? Average Nd abundancelog(Sun)phys.abundfloatnullableEu? Average Eu abundancelog(Sun)phys.abundfloatnullable