Astrophysical Journal, ISSN 0004-637X, 08/2017, Volume 844, Issue 2, p. 145
Nine Ce II lines have been identified and characterized within the spectral window observed by the Apache Point Observatory Galactic Evolution Experiment...
stars: abundances | GALACTIC EVOLUTION EXPERIMENT | NEUTRON-CAPTURE ELEMENTS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | HIGH-RESOLUTION | RED GIANTS | INNER GALAXY | CHEMICAL ABUNDANCES | DISTANT UNIVERSE | MILKY-WAY | Fysik | Astronomi, astrofysik och kosmologi | Physical Sciences | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
stars: abundances | GALACTIC EVOLUTION EXPERIMENT | NEUTRON-CAPTURE ELEMENTS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | HIGH-RESOLUTION | RED GIANTS | INNER GALAXY | CHEMICAL ABUNDANCES | DISTANT UNIVERSE | MILKY-WAY | Fysik | Astronomi, astrofysik och kosmologi | Physical Sciences | Naturvetenskap | Natural Sciences | Astronomy, Astrophysics and Cosmology
Journal Article
Astronomical Journal, ISSN 0004-6256, 06/2016, Volume 151, Issue 6, p. 144
The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has built the largest moderately high-resolution (R approximate to 22,500) spectroscopic...
stars: atmospheres Supporting material: machine-readable table | methods: data analysis | Galaxy: structure | stars: abundances | Galaxy: center | stars: atmospheres | GALACTIC EVOLUTION EXPERIMENT | SPECTROSCOPY | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | STARS | SYSTEMS | MILKY-WAY | SPECTRA | DATA RELEASE | ATMOSPHERIC PARAMETERS | Databases | Pipelines | Stars | Minimization | Spectra | Apogees | Atmospherics | Optimization | Physics - Solar and Stellar Astrophysics | GALACTIC EVOLUTION | METALLICITY | COMPARATIVE EVALUATIONS | ATMOSPHERES | ABUNDANCE | ACCURACY | DATA ANALYSIS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MINIMIZATION | ASTROPHYSICS | EMISSION SPECTRA | GRAVITATION | COMPUTER CODES | MILKY WAY | SURFACES
stars: atmospheres Supporting material: machine-readable table | methods: data analysis | Galaxy: structure | stars: abundances | Galaxy: center | stars: atmospheres | GALACTIC EVOLUTION EXPERIMENT | SPECTROSCOPY | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | STARS | SYSTEMS | MILKY-WAY | SPECTRA | DATA RELEASE | ATMOSPHERIC PARAMETERS | Databases | Pipelines | Stars | Minimization | Spectra | Apogees | Atmospherics | Optimization | Physics - Solar and Stellar Astrophysics | GALACTIC EVOLUTION | METALLICITY | COMPARATIVE EVALUATIONS | ATMOSPHERES | ABUNDANCE | ACCURACY | DATA ANALYSIS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MINIMIZATION | ASTROPHYSICS | EMISSION SPECTRA | GRAVITATION | COMPUTER CODES | MILKY WAY | SURFACES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 466, Issue 1, pp. 1010 - 1018
We report chemical abundances obtained by Sloan Digital Sky Survey (SDSS)-III/Apache Point Observatory Galactic Evolution Experiment for giant stars in five...
Stars: abundances | Galaxy: bulge | Globular clusters: general | HORIZONTAL-BRANCH STARS | RESOLUTION INFRARED-SPECTRA | MULTIPLE STELLAR POPULATIONS | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | SYSTEM TERZAN 5 | globular clusters: general | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SELF-ENRICHMENT | UV LEGACY SURVEY | MILKY-WAY | Physics - Astrophysics of Galaxies | Physics | Astrophysics
Stars: abundances | Galaxy: bulge | Globular clusters: general | HORIZONTAL-BRANCH STARS | RESOLUTION INFRARED-SPECTRA | MULTIPLE STELLAR POPULATIONS | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | SYSTEM TERZAN 5 | globular clusters: general | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SELF-ENRICHMENT | UV LEGACY SURVEY | MILKY-WAY | Physics - Astrophysics of Galaxies | Physics | Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2016, Volume 456, Issue 4, pp. 3655 - 3670
We show that the masses of red giant stars can be well predicted from their photospheric carbon and nitrogen abundances, in conjunction with their...
Stars: Evolution | Stars: Fundamental parameters | Stars: Abundances | stars: evolution | METAL-POOR GIANTS | MAIN-SEQUENCE | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | COROT ASTEROSEISMOLOGY FIELDS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | SOLAR-LIKE OSCILLATIONS | STELLAR POPULATIONS | MILKY-WAY | GLOBULAR-CLUSTERS
Stars: Evolution | Stars: Fundamental parameters | Stars: Abundances | stars: evolution | METAL-POOR GIANTS | MAIN-SEQUENCE | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | COROT ASTEROSEISMOLOGY FIELDS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | SOLAR-LIKE OSCILLATIONS | STELLAR POPULATIONS | MILKY-WAY | GLOBULAR-CLUSTERS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 01/2017, Volume 597, p. A30
With the advent of the space missions CoRoT and Kepler, it has recently become feasible to determine precise asteroseismic masses and relative ages for large...
Galaxy: evolution | Galaxy: disk | Stars: fundamental parameters | Galaxy: abundances | Asteroseismology | MILKY-WAY DISK | STELLAR AGES | METAL-RICH STARS | CHEMICAL EVOLUTION | asteroseismology | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | AGE-METALLICITY RELATION | stars: fundamental parameters | GENEVA-COPENHAGEN SURVEY | SOLAR-LIKE OSCILLATIONS | EVOLUTION EXPERIMENT APOGEE | Red giant stars | Uncertainty | Stars | Samples | Milky Way Galaxy | Statistical methods | Stellar age | Age | Physics | Astrophysics
Galaxy: evolution | Galaxy: disk | Stars: fundamental parameters | Galaxy: abundances | Asteroseismology | MILKY-WAY DISK | STELLAR AGES | METAL-RICH STARS | CHEMICAL EVOLUTION | asteroseismology | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | AGE-METALLICITY RELATION | stars: fundamental parameters | GENEVA-COPENHAGEN SURVEY | SOLAR-LIKE OSCILLATIONS | EVOLUTION EXPERIMENT APOGEE | Red giant stars | Uncertainty | Stars | Samples | Milky Way Galaxy | Statistical methods | Stellar age | Age | Physics | Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2016, Volume 823, Issue 1, pp. 30 - 30
The spatial structure of stellar populations with different chemical abundances in the Milky Way (MW) contains a wealth of information on Galactic evolution...
Galaxy: evolution | Galaxy: disk | Galaxy: structure | Galaxy: formation | Galaxy: abundances | Galaxy: fundamental parameters | MILKY-WAY DISK | DARK-MATTER UNIVERSE | CHEMICAL EVOLUTION | THICK DISK | MONO-ABUNDANCE SUBPOPULATIONS | RED CLUMP STARS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | RADIAL MIGRATION | CHEMODYNAMICAL EVOLUTION | Stellar populations | Maps | Stars | Galactic disk | Flares | Disks | Apogees | Scale height | Physics - Astrophysics of Galaxies
Galaxy: evolution | Galaxy: disk | Galaxy: structure | Galaxy: formation | Galaxy: abundances | Galaxy: fundamental parameters | MILKY-WAY DISK | DARK-MATTER UNIVERSE | CHEMICAL EVOLUTION | THICK DISK | MONO-ABUNDANCE SUBPOPULATIONS | RED CLUMP STARS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | RADIAL MIGRATION | CHEMODYNAMICAL EVOLUTION | Stellar populations | Maps | Stars | Galactic disk | Flares | Disks | Apogees | Scale height | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2017, Volume 840, Issue 1, p. 17
In the updated APOGEE-Kepler catalog, we have asteroseismic and spectroscopic data for over 3000 first ascent red giants. Given the size and accuracy of this...
stars: evolution | stars: fundamental parameters | OF-STATE TABLES | ASTROPHYSICAL APPLICATIONS | GALACTIC EVOLUTION EXPERIMENT | NUCLEAR-REACTIONS | SDSS-III/APOGEE SURVEY | EFFECTIVE TEMPERATURE | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | CHEMICAL ABUNDANCES | KEPLER RED GIANTS | STELLAR POPULATION SYNTHESIS | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics | CONVECTION | CATALOGS | CORRELATIONS | METALLICITY | COMPARATIVE EVALUATIONS | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | ACCURACY | FORECASTING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MIXING | STAR EVOLUTION | STARS | GIANT STARS
stars: evolution | stars: fundamental parameters | OF-STATE TABLES | ASTROPHYSICAL APPLICATIONS | GALACTIC EVOLUTION EXPERIMENT | NUCLEAR-REACTIONS | SDSS-III/APOGEE SURVEY | EFFECTIVE TEMPERATURE | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | CHEMICAL ABUNDANCES | KEPLER RED GIANTS | STELLAR POPULATION SYNTHESIS | Physics - Solar and Stellar Astrophysics | Physics | Astrophysics | CONVECTION | CATALOGS | CORRELATIONS | METALLICITY | COMPARATIVE EVALUATIONS | SIMULATION | THREE-DIMENSIONAL CALCULATIONS | ACCURACY | FORECASTING | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | MIXING | STAR EVOLUTION | STARS | GIANT STARS
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 08/2016, Volume 460, Issue 3, pp. 2611 - 2624
We present the effective temperatures (T-eff), metallicities, and colours in Sloan Digital Sky Survey (SDSS), Two Micron All Sky Survey, and Wide-field...
LOW-MASS STARS | surveys | INTRINSIC COLORS | MAIN-SEQUENCE | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | stars: late-type | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | MODEL ATMOSPHERE | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | stars: low-mass | CHEMICAL ABUNDANCES | MILKY-WAY | EFFECTIVE TEMPERATURE SCALE
LOW-MASS STARS | surveys | INTRINSIC COLORS | MAIN-SEQUENCE | stars: abundances | GALACTIC EVOLUTION EXPERIMENT | stars: late-type | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | MODEL ATMOSPHERE | ASTRONOMY & ASTROPHYSICS | stars: fundamental parameters | stars: low-mass | CHEMICAL ABUNDANCES | MILKY-WAY | EFFECTIVE TEMPERATURE SCALE
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2017, Volume 845, Issue 2, p. 162
The Apache Point Observatory Galactic Evolution Experiment provides the opportunity of measuring elemental abundances for C, N, O, Na, Mg, Al, Si, P, K, Ca, V,...
galaxies: dwarf | galaxies: individual (Sagittarius dSph) | galaxies: stellar content | METALLICITY DISTRIBUTION | PLANETARY-NEBULAE | S-PROCESS | GALACTIC EVOLUTION EXPERIMENT | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SPHEROIDAL GALAXY | INITIAL MASS FUNCTION | MILKY-WAY | GLOBULAR-CLUSTERS | Physics - Astrophysics of Galaxies | ISOCHRONOUS CYCLOTRONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ELEMENT ABUNDANCE | MASS | RESOLUTION | GALACTIC EVOLUTION | MILKY WAY | RED GIANT STARS | VISIBLE RADIATION | HYDROSTATICS | MAGELLANIC CLOUDS
galaxies: dwarf | galaxies: individual (Sagittarius dSph) | galaxies: stellar content | METALLICITY DISTRIBUTION | PLANETARY-NEBULAE | S-PROCESS | GALACTIC EVOLUTION EXPERIMENT | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | SPHEROIDAL GALAXY | INITIAL MASS FUNCTION | MILKY-WAY | GLOBULAR-CLUSTERS | Physics - Astrophysics of Galaxies | ISOCHRONOUS CYCLOTRONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ELEMENT ABUNDANCE | MASS | RESOLUTION | GALACTIC EVOLUTION | MILKY WAY | RED GIANT STARS | VISIBLE RADIATION | HYDROSTATICS | MAGELLANIC CLOUDS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 01/2016, Volume 817, Issue 1, p. 49
Determining the level of chemical homogeneity in open clusters is of fundamental importance in the study of the evolution of star-forming clouds and that of...
Galaxy: evolution | Galaxy: disk | Galaxy: structure | Galaxy: formation | Galaxy: abundances | Galaxy: fundamental parameters | MOLECULAR CLOUDS | STAR-CLUSTERS | GALACTIC EVOLUTION EXPERIMENT | STELLAR EVOLUTION | ABUNDANCE ANALYSIS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | EXPERIMENT APOGEE | GLOBULAR-CLUSTERS | Spectroscopy | Star formation | Homogeneity | Clusters | Abundance | Open clusters | Solar power generation | Constraining
Galaxy: evolution | Galaxy: disk | Galaxy: structure | Galaxy: formation | Galaxy: abundances | Galaxy: fundamental parameters | MOLECULAR CLOUDS | STAR-CLUSTERS | GALACTIC EVOLUTION EXPERIMENT | STELLAR EVOLUTION | ABUNDANCE ANALYSIS | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | EXPERIMENT APOGEE | GLOBULAR-CLUSTERS | Spectroscopy | Star formation | Homogeneity | Clusters | Abundance | Open clusters | Solar power generation | Constraining
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2016, Volume 833, Issue 2, p. 132
We report on the detection, from observations obtained with the Apache Point Observatory Galactic Evolution Experiment spectroscopic survey, of a metal-poor...
globular clusters: general | stars: abundances | stars: Population II | GALACTIC EVOLUTION EXPERIMENT | STELLAR GENERATIONS | OMEGA-CENTAURI | SDSS-III/APOGEE SURVEY | EXTENDED TIDAL DEBRIS | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | MULTIPLE POPULATIONS | CHEMICAL-COMPOSITION | MILKY-WAY | EXPERIMENT APOGEE | Physics - Astrophysics of Galaxies
globular clusters: general | stars: abundances | stars: Population II | GALACTIC EVOLUTION EXPERIMENT | STELLAR GENERATIONS | OMEGA-CENTAURI | SDSS-III/APOGEE SURVEY | EXTENDED TIDAL DEBRIS | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | MULTIPLE POPULATIONS | CHEMICAL-COMPOSITION | MILKY-WAY | EXPERIMENT APOGEE | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 465, Issue 1, pp. 19 - 31
Multiple populations revealed in globular clusters (GCs) are important windows to the formation and evolution of these stellar systems. The metal-rich GCs in...
Stars: abundances | Stars: evolution | Galaxy: bulge | Globular clusters: individual: NGC 6553 | MILKY-WAY BULGE | HORIZONTAL-BRANCH STARS | stars: evolution | HUBBLE-SPACE-TELESCOPE | ELEMENT ABUNDANCES | MULTIPLE STELLAR POPULATIONS | stars: abundances | globular clusters: individual: NGC 6553 | GALACTIC BULGE | OMEGA-CENTAURI | SDSS-III/APOGEE SURVEY | ASTRONOMY & ASTROPHYSICS | UV LEGACY SURVEY | FLAMES-GIRAFFE SPECTRA | Physics | Astrophysics
Stars: abundances | Stars: evolution | Galaxy: bulge | Globular clusters: individual: NGC 6553 | MILKY-WAY BULGE | HORIZONTAL-BRANCH STARS | stars: evolution | HUBBLE-SPACE-TELESCOPE | ELEMENT ABUNDANCES | MULTIPLE STELLAR POPULATIONS | stars: abundances | globular clusters: individual: NGC 6553 | GALACTIC BULGE | OMEGA-CENTAURI | SDSS-III/APOGEE SURVEY | ASTRONOMY & ASTROPHYSICS | UV LEGACY SURVEY | FLAMES-GIRAFFE SPECTRA | Physics | Astrophysics
Journal Article
Astronomical Journal, ISSN 0004-6256, 03/2016, Volume 151, Issue 3, p. 85
In its three years of operation, the Sloan Digital Sky Survey Apache Point Observatory Galactic Evolution Experiment (APOGEE-1) observed >14,000 stars with...
binaries: close | Galaxy: stellar content | brown dwarfs | planetary systems | binaries: spectroscopic | PRECISE RADIAL-VELOCITIES | BROWN DWARF DESERT | SHORT-PERIOD | SOLAR-LIKE STARS | GALACTIC EVOLUTION EXPERIMENT | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | PLANET SEARCH | GIANT STARS | LOW-MASS STELLAR | Separation | Brown dwarf stars | Extrasolar planets | Stars | Orbits | Apogees | Catalogs | Desert environments
binaries: close | Galaxy: stellar content | brown dwarfs | planetary systems | binaries: spectroscopic | PRECISE RADIAL-VELOCITIES | BROWN DWARF DESERT | SHORT-PERIOD | SOLAR-LIKE STARS | GALACTIC EVOLUTION EXPERIMENT | SDSS-III/APOGEE SURVEY | DIGITAL SKY SURVEY | ASTRONOMY & ASTROPHYSICS | PLANET SEARCH | GIANT STARS | LOW-MASS STELLAR | Separation | Brown dwarf stars | Extrasolar planets | Stars | Orbits | Apogees | Catalogs | Desert environments
Journal Article