J/AJ/156/94ivo://CDS.VizieR/J/AJ/156/94doi:10.26093/cds/vizier.51560094CDSSchiappacasse-Ulloa J.Tang B.Fernandez-Trincado J.G.Zamora O.,Geisler D.Frinchaboy P.Schultheis M.Dell'Agli F.Villanova S.,Masseron T.Meszaros S.Souto D.Hasselquist S.Cunha K.Smith V.V.,Garcia-Hernandez D.A.Vieira K.Robin A.C.Minniti D.Zasowski G.,Moreno E.Perez-Villegas A.Lane R.R.Ivans I.I.Pan K.Nitschelm C.,Santana F.A.Carrera R.Roman-Lopes A.2019-03-21T12:43:23Z2019-03-06T07:06:22ZCDS support team

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

cds-question@unistra.frmilky-way-galaxyopen-star-clustersstellar-populationsinfrared-photometryeffective-temperaturechemical-abundancesvisible-astronomytrigonometric-parallaxradial-velocityproper-motionsIC 166 is an intermediate-age open cluster (OC) (~1 Gyr) that lies in the transition zone of the metallicity gradient in the outer disk. Its location, combined with our very limited knowledge of its salient features, make it an interesting object of study. We present the first high-resolution spectroscopic and precise kinematical analysis of IC 166, which lies in the outer disk with R_GC_~12.7 kpc. High-resolution H-band spectra were analyzed using observations from the SDSS-IV Apache Point Observatory Galactic Evolution Experiment survey. We made use of the Brussels Automatic Stellar Parameter code to provide chemical abundances based on a line-by-line approach for up to eight chemical elements (Mg, Si, Ca, Ti, Al, K, Mn, and Fe). The {alpha}-element (Mg, Si, Ca, and whenever available Ti) abundances, and their trends with Fe abundances have been analyzed for a total of 13 high-likelihood cluster members. No significant abundance scatter was found in any of the chemical species studied. Combining the positional, heliocentric distance, and kinematic information, we derive, for the first time, the probable orbit of IC 166 within a Galactic model including a rotating boxy bar, and found that it is likely that IC 166 formed in the Galactic disk, supporting its nature as an unremarkable Galactic OC with an orbit bound to the Galactic plane.2018AJ....156...94Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/156/94CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toI/345 : Gaia DR2 (Gaia Collaboration, 2018)J/AJ/144/95 : Abundance in stars of the outer galactic disk. IV.J/PAZh/38/571 : Astrophysical parameters for 593 open clustersJ/A+A/564/A79 : Proper motions of open clusters from UCAC4 (Dias+, 2014)J/A+A/585/A101 : Milky Way global survey of star clusters. V.J/AJ/151/144 : ASPCAP weights for the 15 APOGEE chemical elementsJ/AZh/93/49 : Abundances in Galactic open clusters (Marsakov+, 2016)J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)J/A+A/619/A155 : Open cluster kinematics with Gaia DR2 (Soubiran+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/156/94https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/156/94http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/156/94https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/156/94https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/156/94http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/156/94GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/156/94/table1 (Summary table of likely members of IC 166)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/156/94/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/156/94/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/156/94/table1?GETtext/xml+votable180.050000true27.9572961161.848778060.005555555555555556Cone search capability for table J/AJ/156/94/table5 (IC 166 data from Gaia DR2 and APOGEE)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/156/94/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/156/94/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/156/94/table5?GETtext/xml+votable180.050000true27.957291761.84877780.0055555555555555566/36338.650015785639275e-20 1.7003137259100215e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/156/94?format=asciiOpticalInfrareddefaultJ/AJ/156/94/table1Summary table of likely members of IC 166SimbadNameSimbad column added by the CDSmeta.idcharAPOGEEAPOGEE identifier (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStar[1/13] Star numbermeta.idintprimarymoreindicates data in Tables 2 and 5 for this starmeta.ref.urlcharRAJ2000Right Ascension in decimal degrees (J2000)degpos.eq.ra;meta.mainDEJ2000Declination in decimal degrees (J2000)degpos.eq.dec;meta.mainJmag[12.649/13.487] 2MASS J band magnitudemagphot.mag;em.IR.JfloatKsmag[11.603/12.503] 2MASS K_s_ band magnitudemagphot.mag;em.IR.KfloatMemb[63/96]? Membership probability from Dias et al. (2014, J/A+A/564/A79)%statintnullableAbundDisplay the atomic lines used and derived abundances from Table 7meta.ref.urlcharJ/AJ/156/94/table2Stellar parameters obtained from FERRE/MARCSrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintStar[1/13] Star numbermeta.idintTeff[4825/5170] Effective temperature from this workKphys.temperature.effectiveintlogg[2.87/3.22] Surface gravity from this worklog(cm.s**-2)phys.gravityfloat[Fe/H][-0.11/-0.01] Metallicity from this workphys.abund.Zfloatksi[0.93/1.69] Microturbulent velocity from this work {ksi}km/sphys.velocfloatTeffA[4775/5175] Effective temperature from ASPCAPKphys.temperature.effectiveintloggA[2.75/3.15] Surface gravity from ASPCAPlog(cm.s**-2)phys.gravityfloat[Fe/H]A[-0.09/-0.03] Metallicity from ASPCAPphys.abund.FefloatksiA[1.1/1.7] Microturbulent velocity from ASPCAP {ksi}km/sphys.velocfloatJ/AJ/156/94/table5IC 166 data from Gaia DR2 and APOGEErecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAPOGEEAPOGEE identifier (2MHHMMSSss+DDMMSSs)meta.id;meta.maincharStar[1/13] Star number (from Table 1)meta.idintRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainPlx[0.092/0.305] Parallaxmaspos.parallaxfloate_Plx[0.034/0.059] Uncertainty in Plxmasstat.error;pos.parallaxfloatRV[-44.142/-37.449] Radial velocitykm/sphys.veloc;pos.heliocentricfloate_RV[0.033/0.688] Uncertainty in RVkm/sstat.errorfloatpmRA[-1.58/-1.236] Proper motion in right ascension direction (pmRA*cosDE)mas/yrpos.pm;pos.eq.rafloate_pmRA[0.036/0.065] Uncertainty in pmRAmas/yrstat.error;pos.pm;pos.eq.rafloatpmDE[0.996/1.291] Proper motion in declination directionmas/yrpos.pm;pos.eq.decfloate_pmDE[0.05/0.088] Uncertainty in pmDEmas/yrstat.error;pos.pm;pos.eq.decfloatJ/AJ/156/94/table7Atomic lines used and derived abundancesAbund13[-0.17/7.55]? Abundance for star 13phys.abundfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElement(s)phys.atmol.elementcharlambda[15159.2/16828.2]? Wavelength in air {lambda}_air_ ({AA})0.1nmem.wldoublenullableAbund1[-0.16/7.64]? Abundance for star 1phys.abundfloatnullablee_Abund1[0.01/0.14]? Uncertainty in Abund1stat.errorfloatnullableAbund2[-0.25/7.73]? Abundance for star 2phys.abundfloatnullablee_Abund2[0.03/0.14]? Uncertainty in Abund2stat.errorfloatnullableAbund3[-0.16/7.55]? Abundance for star 3phys.abundfloatnullablee_Abund3[0.01/0.18]? Uncertainty in Abund3stat.errorfloatnullableAbund4[-0.23/7.79]? Abundance for star 4phys.abundfloatnullablee_Abund4[0.04/0.15]? Uncertainty in Abund4stat.errorfloatnullableAbund5[-0.19/7.73]? Abundance for star 5phys.abundfloatnullablee_Abund5[0.02/0.1]? Uncertainty in Abund5stat.errorfloatnullableAbund6[-0.19/7.73]? Abundance for star 6phys.abundfloatnullablee_Abund6[0.01/0.13]? Uncertainty in Abund6stat.errorfloatnullableAbund7[-0.17/7.59]? Abundance for star 7phys.abundfloatnullablee_Abund7[0.04/0.1]? Uncertainty in Abund7stat.errorfloatnullableAbund8[-0.23/7.55]? Abundance for star 8phys.abundfloatnullablee_Abund8[0.03/0.14]? Uncertainty in Abund8stat.errorfloatnullableAbund9[-0.22/7.56]? Abundance for star 9phys.abundfloatnullablee_Abund9[0.04/0.18]? Uncertainty in Abund9stat.errorfloatnullableAbund10[-0.18/7.74]? Abundance for star 10phys.abundfloatnullablee_Abund10[0.01/0.11]? Uncertainty in Abund10stat.errorfloatnullableAbund11[-0.17/7.66]? Abundance for star 11phys.abundfloatnullablee_Abund11[0.02/0.13]? Uncertainty in Abund11stat.errorfloatnullableAbund12[-0.13/7.88]? Abundance for star 12phys.abundfloatnullablee_Abund12[0.01/0.2]? Uncertainty in Abund12stat.errorfloatnullablee_Abund13[0.04/0.13]? Uncertainty in Abund13stat.errorfloatnullable