J/MNRAS/465/501ivo://CDS.VizieR/J/MNRAS/465/501doi:10.26093/cds/vizier.74650501CDSSchiavon R.P.Zamora O.Carrera R.Lucatello S.Robin A.C.Ness M.,Martell S.L.Smith V.V.Garcia-Hernandez D.A.Manchado A.Schonrich R.,Bastian N.Chiappini C.Shetrone M.Mackereth J.T.Williams R.A.,Meszaros S.Allende Prieto C.Anders F.Bizyaev D.Beers T.C.,Chojnowski S.D.Cunha K.Epstein C.Frinchaboy P.M.Garcia Perez A.E.,Hearty F.R.Holtzman J.A.Johnson J.A.Kinemuchi K.Majewski S.R.,Muna D.Nidever D.L.Nguyen D.C.O'Connell R.W.Oravetz D.Pan K.,Pinsonneault M.Schneider D.P.Schultheis M.Simmons A.Skrutskie M.F.,Sobeck J.Wilson J.C.Zasowski G.2024-08-17T20:17:21Z2018-09-07T10:44:35ZCDS support team

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

cds-question@unistra.frmilky-way-galaxypeculiar-variable-starschemical-abundancesFormation of globular clusters (GCs), the Galactic bulge, or galaxy bulges in general is an important unsolved problem in Galactic astronomy. Homogeneous infrared observations of large samples of stars belonging to GCs and the Galactic bulge field are one of the best ways to study these problems. We report the discovery by APOGEE (Apache Point Observatory Galactic Evolution Experiment) of a population of field stars in the inner Galaxy with abundances of N, C, and Al that are typically found in GC stars. The newly discovered stars have high [N/Fe], which is correlated with [Al/Fe] and anticorrelated with [C/Fe]. They are homogeneously distributed across, and kinematically indistinguishable from, other field stars within the same volume. Their metallicity distribution is seemingly unimodal, peaking at [Fe/H]~-1, thus being in disagreement with that of the Galactic GC system. Our results can be understood in terms of different scenarios. N-rich stars could be former members of dissolved GCs, in which case the mass in destroyed GCs exceeds that of the surviving GC system by a factor of ~8. In that scenario, the total mass contained in so-called 'first-generation' stars cannot be larger than that in 'second-generation' stars by more than a factor of ~9 and was certainly smaller. Conversely, our results may imply the absence of a mandatory genetic link between 'second-generation' stars and GCs. Last, but not least, N-rich stars could be the oldest stars in the Galaxy, the by-products of chemical enrichment by the first stellar generations formed in the heart of the Galaxy.2017MNRAS.465..501Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/465/501CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)J/AJ/146/133 : Stellar parameters from SDSS-III APOGEE DR10 (Meszaros+, 2013)J/AJ/146/156 : APOGEE M-dwarf survey I First year velocities (Deshpande+, 2013)J/ApJ/819/2 : APOGEE kinematics. I. Galactic bulge overview (Ness+, 2016)J/ApJ/852/49 : Properties of metal-poor stars in APOGEE DR13 (Hayes+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/465/501https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/465/501http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/465/501https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/465/501https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/465/501http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/465/501GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/465/501/tablea1 (N-rich stars identified in the inner Galaxy)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/tablea1?GETtext/xml+votable180.050000true252.40240306-20.470730.005555555555555556Cone search capability for table J/MNRAS/465/501/bulge (Galactic bulge used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/bulge?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/bulge?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/bulge?GETtext/xml+votable180.050000true251.47773111-20.500071110.005555555555555556Cone search capability for table J/MNRAS/465/501/m3 (M3 used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/m3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/m3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/m3?GETtext/xml+votable180.050000true205.26312528.2108750.005555555555555556Cone search capability for table J/MNRAS/465/501/m5 (M5 used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/m5?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/m5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/m5?GETtext/xml+votable180.050000true229.518748062.017523060.005555555555555556Cone search capability for table J/MNRAS/465/501/m71 (M71 used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/m71?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/m71?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/m71?GETtext/xml+votable180.050000true298.4061418.749910.005555555555555556Cone search capability for table J/MNRAS/465/501/m107 (M107 used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/m107?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/m107?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/m107?GETtext/xml+votable180.050000true248.10064611-13.0196150.005555555555555556Cone search capability for table J/MNRAS/465/501/n6760 (NGC 6760 used in the paper)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/465/501/n6760?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/465/501/n6760?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/465/501/n6760?GETtext/xml+votable180.050000true287.745966941.053958890.0055555555555555564/1803 5/7189 7194-7195 7205 7207 7211 7216 7219-7220 7222-7223 7226-7228 7230 7273 7275-7278 7290-7291 7297 7301-7302 7312 7315 7326 7329 7331 7361 7364-7365 7367 7376-7378 12010-12011 6/10336-10337 12943 28727 28733 28735 28764-28765 28770 28774-28775 28792 28794 28815 28819 28824 28826-28827 28837-28839 28842-28843 28869-28874 28896 28898-28900 28902-28903 28916 28918-28919 28924 28926-28929 28932 29066-29067 29070-29071 29088-29089 29097-29099 29116-29118 29154-29155 29158 29184-29185 29187 29196 29199 29201 29203 29212-29213 29221 29230-29233 29242 29252 29254-29257 29259 29265 29268-29269 29274 29285 29287 29296 29298-29299 29308 29328 29336 29348-29349 29440-29441 29443 29453 29464-29465 29516-29518 29537 29540 30321 30769 31416-31417 47869 47871 48034-48036 48038-48039 48056 480582.483060040379131e-20 1.7798557115773645e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/465/501?format=asciidefaultJ/MNRAS/465/501/tablea1N-rich stars identified in the inner GalaxyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainS/NSignal-to-noise ratiostat.snrintTeffEffective temperatureKphys.temperature.effectiveintloggSurface gravitylog(cm.s**-2)phys.gravityfloat[Fe/H]Metallicityphys.abund.Zfloate_[Fe/H]rms uncertainty on [Fe/H]stat.error;phys.abund.Fefloat[Al/Fe]Abundance [Al/Fe]phys.abundfloate_[Al/Fe]rms uncertainty on [Al/Fe]stat.error;phys.abundfloat[C/Fe]Abundance [Cl/Fe]phys.abundfloate_[C/Fe]rms uncertainty on [C/Fe]stat.error;phys.abundfloat[N/Fe]Abundance [N/Fe]phys.abundfloate_[N/Fe]rms uncertainty on [N/Fe]stat.error;phys.abundfloatDistDistancekpcpos.distancefloate_Distrms uncertainty on Distkpcstat.errorfloat2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharJ/MNRAS/465/501/bulgeGalactic bulge used in the paperNNumber of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmagJ magnitudemagphot.mag;em.IR.Jfloate_Jmagrms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JfloatHmagH magnitudemagphot.mag;em.IR.Hfloate_Hmagrms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HfloatKmagK magnitudemagphot.mag;em.IR.Kfloate_Kmagrms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainGLONGalactic longitudedegpos.galactic.lonGLATGalactic latitudedegpos.galactic.latdoubleHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVVelocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeffEffective temperatureKphys.temperature.effectivefloate_Teffrms uncertainty on TeffKstat.error;phys.temperature.effectivefloatloggSurface gravitylog(cm.s**-2)phys.gravitydoublee_loggrms uncertainty on logglog(cm.s**-2)stat.errordouble[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]Abundance [C/H]phys.abunddouble[Fe/H]Abundance [Fe/H]phys.abund.Fedouble[N/H]Abundance [N/H]phys.abunddoublee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]Abundance [C/H]stat.error;phys.abunddoublee_[Fe/H]Abundance [Fe/H]stat.error;phys.abund.Fedoublee_[N/H]Abundance [N/H]stat.error;phys.abunddoubleIRAC1? IRAC1 (3.6um) magnitudemagphot.mag;em.IR.3-4umdoublenullablee_IRAC1? rms uncertainty on IRAC1magstat.errordoublenullableIRAC2? IRAC2 (4.5um) magnitudemagphot.mag;em.IR.4-8umdoublenullablee_IRAC2? rms uncertainty on IRAC2magstat.errordoublenullableIRAC3? IRAC3 (5.8um) magnitudemagphot.flux.density;em.IR.4-8umdoublenullablee_IRAC3? rms uncertainty on IRAC3magstat.errordoublenullableIRAC4? IRAC4 (8.0um) magnitudemagphot.flux.density;em.IR.8-15umdoublenullablee_IRAC4? rms uncertainty on IRAC4magstat.errordoublenullableEKsKs-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.KdoubleDiso1APOGEE distance 1pos.distancedoubleDiso2APOGEE distance 2pos.distancedoubleDiso3APOGEE distance 3pos.distancedoublee_DisoError in distancestat.errordouble2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharJ/MNRAS/465/501/m3M3 used in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmag? J magnitudemagphot.mag;em.IR.Jdoublenullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JdoublenullableHmag? H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HdoublenullableKmag? K magnitudemagphot.mag;em.IR.Kfloatnullablee_Kmag? rms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatnullableRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainN[1/5] Number of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrfloatHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVHeliocentric velocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeff? Effective temperatureKphys.temperature.effectivedoublenullablelogg? Surface gravitylog(cm.s**-2)phys.gravitydoublenullablee_Teff? rms uncertainty on TeffKstat.error;phys.temperature.effectivefloatnullablee_logg? rms uncertainty on logglog(cm.s**-2)stat.errordoublenullable[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]? Abundance [C/H]phys.abunddoublenullable[Fe/H]? Abundance [Fe/H]phys.abund.Fedoublenullable[N/H]? Abundance [N/H]phys.abunddoublenullablee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]? Abundance [C/H]stat.error;phys.abunddoublenullablee_[Fe/H]? Abundance [Fe/H]stat.error;phys.abund.Fedoublenullablee_[N/H]? Abundance [N/H]stat.error;phys.abunddoublenullableEKs? Ks-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.Kdoublenullable2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharJ/MNRAS/465/501/m5M5 used in the paperN[1/5] Number of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrfloatHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVHeliocentric velocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeff? Effective temperatureKphys.temperature.effectivedoublenullablelogg? Surface gravitylog(cm.s**-2)phys.gravitydoublenullablee_Teff? rms uncertainty on TeffKstat.error;phys.temperature.effectivefloatnullablee_logg? rms uncertainty on logglog(cm.s**-2)stat.errordoublenullable[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]? Abundance [C/H]phys.abunddoublenullable[Fe/H]? Abundance [Fe/H]phys.abund.Fedoublenullable[N/H]? Abundance [N/H]phys.abunddoublenullablee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]? Abundance [C/H]stat.error;phys.abunddoublenullablee_[Fe/H]? Abundance [Fe/H]stat.error;phys.abund.Fedoublenullablee_[N/H]? Abundance [N/H]stat.error;phys.abunddoublenullableEKs? Ks-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.Kdoublenullable2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmag? J magnitudemagphot.mag;em.IR.Jdoublenullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JdoublenullableHmag? H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HdoublenullableKmag? K magnitudemagphot.mag;em.IR.Kfloatnullablee_Kmag? rms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatnullableJ/MNRAS/465/501/m71M71 used in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmag? J magnitudemagphot.mag;em.IR.Jdoublenullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JdoublenullableHmag? H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HdoublenullableKmag? K magnitudemagphot.mag;em.IR.Kfloatnullablee_Kmag? rms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatnullableRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainN[1/5] Number of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrfloatHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVHeliocentric velocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeff? Effective temperatureKphys.temperature.effectivedoublenullablelogg? Surface gravitylog(cm.s**-2)phys.gravitydoublenullablee_Teff? rms uncertainty on TeffKstat.error;phys.temperature.effectivefloatnullablee_logg? rms uncertainty on logglog(cm.s**-2)stat.errordoublenullable[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]? Abundance [C/H]phys.abunddoublenullable[Fe/H]? Abundance [Fe/H]phys.abund.Fedoublenullable[N/H]? Abundance [N/H]phys.abunddoublenullablee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]? Abundance [C/H]stat.error;phys.abunddoublenullablee_[Fe/H]? Abundance [Fe/H]stat.error;phys.abund.Fedoublenullablee_[N/H]? Abundance [N/H]stat.error;phys.abunddoublenullableEKs? Ks-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.Kdoublenullable2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharJ/MNRAS/465/501/m107M107 used in the paperrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmag? J magnitudemagphot.mag;em.IR.Jdoublenullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JdoublenullableHmag? H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HdoublenullableKmag? K magnitudemagphot.mag;em.IR.Kfloatnullablee_Kmag? rms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatnullableRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainN[1/5] Number of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrfloatHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVHeliocentric velocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeff? Effective temperatureKphys.temperature.effectivedoublenullablelogg? Surface gravitylog(cm.s**-2)phys.gravitydoublenullablee_Teff? rms uncertainty on TeffKstat.error;phys.temperature.effectivefloatnullablee_logg? rms uncertainty on logglog(cm.s**-2)stat.errordoublenullable[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]? Abundance [C/H]phys.abunddoublenullable[Fe/H]? Abundance [Fe/H]phys.abund.Fedoublenullable[N/H]? Abundance [N/H]phys.abunddoublenullablee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]? Abundance [C/H]stat.error;phys.abunddoublenullablee_[Fe/H]? Abundance [Fe/H]stat.error;phys.abund.Fedoublenullablee_[N/H]? Abundance [N/H]stat.error;phys.abunddoublenullableEKs? Ks-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.Kdoublenullable2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlcharJ/MNRAS/465/501/n6760NGC 6760 used in the paper[Fe/H]? Abundance [Fe/H]phys.abund.FedoublenullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAPOGEE designation (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharJmag? J magnitudemagphot.mag;em.IR.Jdoublenullablee_Jmag? rms uncertainty on Jmagmagstat.error;phot.mag;em.IR.JdoublenullableHmag? H magnitudemagphot.mag;em.IR.Hfloatnullablee_Hmag? rms uncertainty on Hmagmagstat.error;phot.mag;em.IR.HdoublenullableKmag? K magnitudemagphot.mag;em.IR.Kfloatnullablee_Kmag? rms uncertainty on Kmagmagstat.error;phot.mag;em.IR.KfloatnullableRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainN[1/5] Number of visitsmeta.numberintS/NSignal-to-noise ratiostat.snrfloatHVavgAverage heliocentric velocitykm/sphys.veloc;pos.heliocentricdoublesigmaScatter of individual visit HVs around averagekm/sstat.error;stat.meandoublee_HVHeliocentric velocity errorkm/sstat.errordoublee_HVmedMedian of individual visit HVs around averagekm/sstat.errordoubleTeff? Effective temperatureKphys.temperature.effectivedoublenullablelogg? Surface gravitylog(cm.s**-2)phys.gravitydoublenullablee_Teff? rms uncertainty on TeffKstat.error;phys.temperature.effectivefloatnullablee_logg? rms uncertainty on logglog(cm.s**-2)stat.errordoublenullable[Al/H]? Abundance [Al/H]phys.abunddoublenullable[C/H]? Abundance [C/H]phys.abunddoublenullable[N/H]? Abundance [N/H]phys.abunddoublenullablee_[Al/H]? Abundance [Al/H]stat.error;phys.abunddoublenullablee_[C/H]? Abundance [C/H]stat.error;phys.abunddoublenullablee_[Fe/H]? Abundance [Fe/H]stat.error;phys.abund.Fedoublenullablee_[N/H]? Abundance [N/H]stat.error;phys.abunddoublenullableEKs? Ks-band extinction from APOGEE Targeting (AK_TARG)magphys.absorption;em.IR.Kdoublenullable2MDisplay the 2MASS data (Cutri et al. 2003, Cat. II/246)meta.ref.urlchar