The Chemical Compositions of Galactic Disk F and G Dwarfs
arXiv:astro-ph/0211551 · doi:10.1046/j.1365-8711.2003.06305.x
Abstract
Photospheric abundances are presented for 27 elements from carbon to europium in 181 F-G dwarfs from a differential LTE analysis of high-resolution and high signal-to-noise spectra. Stellar were adopted from an infrared flux method calibration of Strömgren photometry. Stellar log were calculated from {\it Hipparcos} parallaxes and stellar evolutionary tracks. Stellar space motions () and a Galactic potential were used to estimate Galactic orbital parameters. Results of -elements -- O, Mg, Si, Ca, and Ti -- show [/Fe] to increase slightly with decreasing [Fe/H]. Heavy elements with dominant contributions at solar metallicity from the -process show [/Fe] to decrease slightly with decreasing [Fe/H]. Scatter in [X/Fe] at a fixed [Fe/H] is entirely attributable to the small measurement errors, after excluding the few thick disc stars and the -process enriched CH subgiants. Tight limits are set on `cosmic' scatter. By combining our sample with published studies, thick disc stars are identified by their in the range to -100 km s. These are very old stars with origins in the inner Galaxy and metallicities [Fe/H] . At the same [Fe/H], the sampled thin disc stars have km s, and are generally younger with a birthplace at about the Sun's Galactocentric distance. In the range 0.35 [Fe/H] 0.70, well represented by present thin and thick disc samples, [X/Fe] of the thick disc stars is greater than that of thin disc stars for Mg, Al, Si, Ca, Ti, and Eu. [X/Fe] is very similar for the thin and thick disc for -- notably -- Na, and iron-group elements.
51 pages (includes 19 figures and 6 tables). To appear in MNRAS (paper has been replaced: typos added, In Table~1, [Fe/H]phot has been replaced by spectroscopic [Fe/H] that are used in the plots) (Table1, photometric[Fe/H] values are replaced by spectroscopically derived [Fe/H] that are used in the plots)
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- The Fe/Ni ratio in ionized nebulae: clues on dust depletion patterns
- Probing the low-redshift star formation rate as a function of metallicity through the local environments of type II supernovae
- Clues to the Metallicity Distribution in the Galactic Bulge: Abundances in MOA-2008-BLG310 and MOA-2008-BLG311
- The chemical DNA of the Magellanic Clouds -- I. The chemical composition of 206 Small Magellanic Cloud red giant stars
- Chemical compositions of stars in two stellar streams from the Galactic thick disk
- The Century Survey Galactic Halo Project I: Stellar Spectral Analysis
- OB Associations, Wolf-Rayet Stars, and the Origin of Galactic Cosmic Rays
- Pre-main-sequence Lithium Depletion
- Detailed Chemical Abundances of Four Stars in the Unusual Globular Cluster, Palomar 1
- NGC 5694: another foster son of the Galactic Halo
- Origin of chemical and dynamical properties of the Galactic thick disk
- Phosphorus Abundances in FGK Stars
- Chemical Study of the Metal-rich Globular Cluster NGC 5927
- Local associations and the barium puzzle
- Neutron-capture elements in dwarf galaxies II: Challenges for the s- and i-processes at low metallicity
- The vertical Na-O relation in the bulge globular cluster NGC 6553
- Combined APOGEE-GALAH stellar catalogues using the Cannon
- New Neutron-Capture Measurements in 23 Open Clusters. I. The R-Process
- Modelling the chemical evolution of the Galaxy halo
- HD 91669b: A New Brown Dwarf Candidate from the McDonald Observatory Planet Search
- A New Definition for the Ca4227 Feature: Is Calcium Really Underabundant in Early-type Galaxies?
- Characterizing the companion AGBs using surface chemical composition of barium stars
- The Galactic Stellar Disc
- Small Planets in the Galactic Context: Host Star Kinematics, Iron, and Element Enhancement
- On the Interpolation of Model Atmospheres and High-Resolution Synthetic Stellar Spectra
- Chemical abundance analysis of the old, rich open cluster Trumpler 20
- The CARMENES search for exoplanets around M dwarfs: Not-so-fine hyperfine-split vanadium lines in cool star spectra
- Interstellar Krypton Abundances: The Detection of Kiloparsec-scale Differences in Galactic Nucleosynthetic History
- NLTE analysis of copper lines in different stellar populations
- The chemical composition of Cen AB revisited
- A homogeneous comparison between the chemical composition of the Large Magellanic Cloud and the Sagittarius dwarf galaxy
- The Gaia-ESO Survey: Detailed Abundances in the Metal-poor Globular Cluster NGC 4372
- A High-resolution Spectrum of the R CrB Star V2552 Ophiuchi
- Chemical enrichment of stars due to accretion from ISM during the Galaxy's assembly
- Calibration of LAMOST Stellar Surface Gravities Using the Kepler Asteroseismic Data
- Finding cool subdwarfs using a V-J reduced proper-motion diagram: Stellar parameters for 91 candidates
- Extreme r-process enhanced stars at high metallicity in Fornax
- A search for pulsations in the HgMn star HD 45975 with CoRoT photometry and ground-based spectroscopy
- Spectroscopic study of two new super Li rich red clump K giants
- Chemical abundances of two extragalactic young massive clusters
- The chemical composition of the Small Magellanic Cloud
- The old, metal-poor, anticentre open cluster Trumpler 5
- Predicted rates of merging neutron stars in galaxies
- The chemical connection between damped Lyman-α systems and Local Group dwarf galaxies
- Chemical abundance analysis of symbiotic giants - III. Metallicity and CNO abundance patterns in 24 southern systems
- The Kapteyn moving group is not tidal debris from Centauri
- Phosphorus Abundances in the Hyades and Galactic Disk
- Investigation of the Puzzling Abundance Pattern in the Stars of the Fornax Dwarf Spheroidal Galaxy
- On the Flaring of Thick Disc of Galaxies: Insights from Simulations
- Abundance analyses of Li-enriched and normal giants in the GALAH survey
- Neutron-capture elements in dwarf galaxies I: Chemical clocks & the short timescale of the r-process
- Beryllium Abundances in Stars of One-Solar-Mass
- Enrichment of the Galactic disc with neutron capture elements: Sr
- The Arcturus Moving Group: Its Place in the Galaxy
- Searching for GC-like abundance patterns in young massive clusters II. - Results from the Antennae galaxies
- Chemical compositions and kinematics of the Hercules stream
- Metallicities of Young Open Clusters I: NGC 7160 and NGC 2232
- Manganese Abundances in the Globular Cluster Omega Centauri
- Water content trends in K2-138 and other low-mass multiplanetary systems
- Testing abundance-age relations beyond solar analogues with Kepler LEGACY stars
- The chemical composition of the stellar cluster Gaia1: no surprise behind Sirius
- A Compiled Catalogue of Spectroscopically Determined Elemental Abundances for Stars with Accurate Parallaxes. I.Magnesium
- Chemical abundance analysis of red giant branch stars in the globular cluster E3
- Enrichment of the Galactic disc with neutron-capture elements: Mo and Ru
- Tracing the origin of the Aquarius Stream: I
- Not an open cluster after all: the NGC 6863 asterism in Aquila
- The uvbyHbeta Metallicity Calibration for G and K Dwarfs
- Probing the Local Bubble with Diffuse Interstellar Bands. II. The DIB properties in the Northern hemisphere
- Evidence for a chemical enrichment coupling of globular clusters and field stars in the Fornax dSph
- Galactic structure in the outer disk: the field in the line of sight to the intermediate-age open cluster Tombaugh 1
- The G-dwarf problem in the Galaxy
- Chlorine Abundances in Cool Stars
- GIANO-TNG spectroscopy of red supergiants in the young star cluster RSGC3
- Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
- Abundance study of the two solar-analogue CoRoT targets HD 42618 and HD 43587 from HARPS spectroscopy
- The chemical evolution of the solar neighbourhood for planet-hosting stars
- On the metal-poor edge of the Milky Way "thin disc"
- Detailed chemical abundance analysis of the thick disk star cluster Gaia 1
- Chemistry of multiple stellar populations in the mono-metallic, in situ, bulge globular cluster NGC 6388
- Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows II: Effect of Turbulence and Metal-Line Cooling
- Exoplanets Across Galactic Stellar Populations with PLATO: Estimating Exoplanet Yields Around FGK Stars for the Thin Disk, Thick Disk and Stellar Halo
- Abundance analysis of red clump stars in the old, inner disc, open cluster NGC 4337: a twin of NGC 752?
- Chemical Abundances of Globular Clusters in NGC 5128 (Centaurus A)
- Three new barium dwarfs with WD companions: BD+68 1027, RE J0702+129 and BD+80 670
- Fossil Imprints of Outflow from the Galactic Bulge in Elemental Abundances of Metal-Rich Disk Stars
- Stellar population astrophysics (SPA) with the TNG -- The Arcturus Lab
- Bayesian isochrone fitting and stellar ages
- The Interstellar Rubidium Isotope Ratio toward Rho Ophiuchi A
- Manganese evolution in Omega Centauri: a clue to the cluster formation mechanisms?
- Probing M subdwarf metallicity with an esdK5+esdM5.5 binary
- Seismic analysis of HD43587Aa, a solar-like oscillator in a multiple system
- Probing the Local Bubble with Diffuse Interstellar Bands. III. The Northern hemisphere data and catalog
- Sun-like stars unlike the Sun: Clues for chemical anomalies of cool stars
- Magnesium abundances in mildly metal-poor stars from different indicators
- Europium as a lodestar: diagnosis of radiogenic heat production in terrestrial exoplanets
- GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
- Near-infrared chemical abundances of stars in the Sculptor dwarf galaxy
- M Subdwarf Research. II. Atmospheric Parameters and Kinematics
- A Spectroscopic Survey of Field Red Horizontal-Branch Stars
- Clustering in the Stellar Abundances Space
- NGC 1252: a high altitude, metal poor open cluster remnant
- Galactic r-process abundance feature shaped by radial migration
- Palladium and silver abundances in stars with [Fe/H] > -2.6
- High Resolution HDS/SUBARU chemical abundances of the young stellar cluster Palomar 1
- Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies
- On the Origin of Metal-poor Stars in the Solar Neighborhood
- Properties of the open cluster Tombaugh 1 from high resolution spectroscopy and uvbyCaH photometry
- Populating The Milky Way: Characterising Planet Demographics by Combining Galaxy Formation Simulations and Planet Population Synthesis Models
- Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
- The in situ origin of the globular cluster NGC 6388 from abundances of Sc, V, and Zn of a large sample of stars
- Chemical Compositions of Red Giant Stars from Habitable Zone Planet Finder Spectroscopy
- Chemical analysis of the Bulge Globular Cluster NGC 6553
- NLTE Analysis of Copper Abundances in the Galactic Bulge Stars
- Close to the Dredge: Precise X-ray C and N Abundances in lambda Andromeda and its Precocious RGB Mixing Problem
- High Resolution Spectroscopy of the high galactic latitude RV Tauri star CE Virginis
- IP Eri: A surprising long-period binary system hosting a He white dwarf
- Chemical abundances of primary stars in the Sirius-like binary systems
- Stellar substructures in the solar neighbourhood. III. Kinematic group 2 in the Geneva-Copenhagen survey
- High-resolution spectroscopic observations of the new CEMP-s star CD-50776
- A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia
- The Aquarius Co-Moving Group is Not a Disrupted Classical Globular Cluster
- Chemical Tagging N-rich Field Stars with High-resolution Spectroscopy
- More pieces of the puzzle: Chemistry and substructures in the Galactic thick disk
- Chemical abundance analysis of symbiotic giants - II. AE Ara, BX Mon, KX TrA, and CL Sco
- A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
- The s-process enriched star HD 55496: origin from a globular cluster or from the tidal disruption of a dwarf galaxy?
- Heavy elements in old very metal-rich stars
- Stellar substructures in the solar neighbourhood IV. Kinematic Group 1 in the Geneva-Copenhagen survey
- Enrichment of the Galactic disc with neutron-capture elements: Gd, Dy, and Th
- Diversity of Type Ia Supernovae Imprinted in Chemical Abundances
- Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc
- Stellar substructures in the solar neighbourhood. II. Abundances of neutron-capture elements in the kinematic Group 3 of the Geneva-Copenhagen survey
- Elemental abundances of intermediate age open cluster NGC 3680
- High-resolution spectroscopic analysis of four new chemically peculiar stars
- Distributions of Long-Lived Radioactive Nuclei Provided by Star Forming Environments
- The Galactic Disk-Halo transition - Evidence from Stellar Abundances
- Turn-off of Deuterium Astration in the Recent Star Formation of the Galaxy Disk
- Stellar population astrophysics (SPA) with the TNG -- The chemical content of the red supergiant population in the Perseus complex
- First Evidence of Globular Cluster Formation from the Ejecta of Prompt Type Ia Supernovae
- s-process Enriched Evolved Binaries in the Galaxy and the Magellanic Clouds
- Chemical abundances of Young Massive Clusters in NGC 1313
- Exploring giant barium stars: ratio and elemental abundances of carbon, nitrogen, and oxygen
- Triangulum-Andromeda overdensity: a region with a complex stellar population
- Stellar Population Astrophysics (SPA) with the TNG: NLTE atmospheric parameters and abundances of giant stars in 33 Open Clusters
- Correlating Intrinsic Stellar Parameters with Mg II Self-Reversal Depths
- Radial velocity comparison of Gaia DR2 and RAVE DR5 survey: a systematic offset in radial velocities among a group of highly accurate radial velocity stars
- Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
- Chemical composition of the young massive cluster NGC 1569-B
- The Space Interferometry Mission Astrometric Grid Giant-Star Survey. III. Basic Stellar Parameters for an Extended Sample
- Vertical kinematics of the thick disc at 4.5 < R < 9.5 kpc
- Type Ia Supernovae and their Explosive Nucleosynthesis: Constraints on Progenitors
- SDSS J1059+4251, a highly magnified z ~ 2.8 star-forming galaxy: ESI observations of the rest-frame UV spectrum
- Very metal-poor stars in the solar vicinity: kinematics and abundance analysis
- [Rb/Zr] ratio in Ba stars as diagnostics of the companion AGB stellar mass
- Stellar substructures in the Galactic disc and halo: Properties, origins, and evolution
- Rediscovering the Milky Way with orbit superposition approach and APOGEE data III. Panoramic view of the bulge
- The Stellar Population of the Thin Disk
- A test field for Gaia. Radial velocity catalogue of stars in the South Ecliptic Pole
- Concerning Li-rich status of KIC~9821622: A Kepler field RGB star reported as Li-rich Giant
- Modelling the chemical evolution of the Milky Way
- Complexity in small-scale dwarf spheroidal galaxies
- Unprecedented accurate abundances: signatures of other Earths?
- Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
- Characterisation of the Galactic thick disk
- A Theoretical Study of the Structure and Elemental Abundances of HD 20794
- An abundance study of the red giants in the seismology fields of the CoRoT satellite
- APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina