Abundances and Kinematics of Field Stars II: Kinematics and Abundance Relationships
arXiv:astro-ph/0110164 · doi:10.1086/324630
Abstract
As an investigation of the origin of ``-poor'' halo stars, we analyze kinematic and abundance data for 73 intermediate metallicity stars ( [Fe/H] ) selected from Paper I of this series. We find evidence for a connection between the kinematics and the enhancement of certain element-to-iron ([X/Fe]) ratios in these stars. Statistically significant correlations were found between [X/Fe] and galactic rest-frame velocities (\vrf{}) for Na, Mg, Al, Si, Ca and Ni, with marginally significant correlations existing for Ti and Y as well. We also find that the [X/Fe] ratios for these elements all correlate with a similar level of significance with [Na/Fe]. Finally, we compare the abundances of these halo stars against those of stars in nearby dSph galaxies. We find significant differences between the abundance ratios in the dSph stars and halo stars of similar metallicity. From this result, it is unlikely that the halo stars in the solar neighborhood, including even the ``-poor'' stars, were once members of disrupted dSph galaxies similar to those studied to date.
Accepted for publication in January 2002 AJ. 29 pages, 12 figures, 2 tables
References in corpus (4)
- Abundance Patterns in the Draco, Sextans and Ursa Minor Dwarf Spheroidal Galaxies
- Abundances and Kinematics of Field Halo and Disk Stars I: Observational Data and Abundance Analysis
- Kinematics of Metal-Poor Stars in the Galaxy. II. Proper Motions for a Large Non-Kinematically Selected Sample
- Evidence for the Hierarchical Formation of the Galactic Spheroid
Cited by in corpus (105)
- Stellar Chemical Signatures And Hierarchical Galaxy Formation
- Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
- VLT/UVES Abundances in Four Nearby Dwarf Spheroidal Galaxies: I. Nucleosynthesis and Abundance Ratios
- A Search for Stars of Very Low Metal Abundance. VI. Detailed Abundances of 313 Metal-Poor Stars
- Evolutionary synthesis of galaxies at high spectral resolution with the code PEGASE-HR
- The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5
- Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
- Abundances of Baade's Window Giants from Keck/HIRES Spectra: II. The Alpha- and Light Odd Elements
- The stellar halo of the Galaxy
- Lambda-Cold Dark Matter, Stellar Feedback, and the Galactic Halo Abundance Pattern
- A high resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy
- Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] < -2
- 'Sculptor'-ing the Galaxy? The Chemical Compositions of Red Giants in the Sculptor Dwarf Spheroidal Galaxy
- The Chemical Composition Contrast between M3 and M13 Revisited: New Abundances for 28 Giant Stars in M3
- Two distinct halo populations in the solar neighborhood. II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
- Chemical abundances of the Milky Way thick disk and stellar halo II.: sodium, iron-peak and neutron-capture elements
- Abundances In Very Metal Poor Dwarf Stars
- Complexity on Small Scales III: Iron and alpha Element Abundances in the Carina Dwarf Spheroidal Galaxy
- Detection of Elements at All Three r-process Peaks in the Metal-Poor Star HD 160617
- Abundances of refractory elements in the atmospheres of stars with extrasolar planets
- A 2MASS All-Sky View of the Sagittarius Dwarf Galaxy: Variation of the Metallicity Distribution Function Along the Sagittarius Stream
- Pal 12 As A Part of the Sgr Stream; the Evidence From Abundance Ratios
- Multi-Element Abundance Measurements from Medium-Resolution Spectra. IV. Alpha Element Distributions in Milky Way Dwarf Satellite Galaxies
- Accretion relicts in the solar neighbourhood: debris from omegaCen's parent galaxy
- The SEGUE Stellar Parameter Pipeline. V. Estimation of Alpha-Element Abundance Ratios From Low-Resolution SDSS/SEGUE Stellar Spectra
- Chemical Abundances in Field Red Giants from High-Resolution H-Band Spectra using the APOGEE Spectral Linelist
- Chemical Compositions of Red Giant Stars in Old Large Magellanic Cloud Globular Clusters
- Non-LTE line formation for heavy elements in four very metal-poor stars
- Chemical Abundances and Kinematics in Globular Clusters and Local Group Dwarf Galaxies and Their Implications for Formation Theories of the Galactic Halo
- Observational Properties of the Metal-Poor Thick Disk of the Milky Way Galaxy and Insights into Its Origins
- Chemical Evolution of the Galactic Bulge as Derived from High-Resolution Infrared Spectroscopy of K and M Red Giants
- High-precision stellar abundances of the elements - methods and applications
- Halo Star Streams in the Solar Neighborhood
- The Distribution of Alpha Elements in Ultra-Faint Dwarf Galaxies
- An inhomogeneous model for the Galactic halo: a possible explanation for the spread observed in s- and r-process elements
- Neutron-Capture Nucleosynthesis in the First Stars
- Principal Component Analysis on Chemical Abundances Spaces
- How many nucleosynthesis processes exist at low metallicity?
- Chemical abundances in 43 metal-poor stars
- Complexity on Small Scales II: Metallicities and Ages in the Leo II Dwarf Spheroidal Galaxy
- The Stellar Abundances for Galactic Archaeology (SAGA) Database III - Analysis of Enrichment Histories for Elements and Two Modes of Star Formation during the Early Evolution of Milky Way
- Exploring Halo Substructure with Giant Stars: Substructure in the Local Halo as Seen in the Grid Giant Star Survey Including Extended Tidal Debris from Omega Centauri
- Comparing CN and CH Line Strengths in a Homogeneous Spectroscopic Sample of 8 Galactic Globular Clusters
- Low-resolution spectroscopy of main sequence stars belonging to 12 Galactic globular clusters. I. CH and CN band strength variations
- Search for associations containing young stars (SACY):II. Chemical abundances of stars in 11 young Associations in the Solar neighborhood
- New PARSEC database of alpha-enhanced stellar evolutionary tracks and isochrones I. Calibration with 47 Tuc (NGC104) and the improvement on RGB bump
- Chemo-dynamics of outer halo dwarf stars, including \textit{Gaia}-Sausage and \textit{Gaia}-Sequoia candidates
- Beryllium and Alpha-Element Abundances in a Large Sample of Metal-Poor Stars
- Fe and Al Abundances for 180 Red Giants in the Globular Cluster Omega Centauri (NGC 5139)
- Manganese trends in a sample of thin and thick disk stars. The origin of Mn
- Oxygen Abundances in Metal-Poor Stars
- A New Type of Extremely Metal Poor Star
- Chemical Inhomogeneities in the Milky Way Stellar Halo
- Heavy elements and chemical enrichment in globular clusters
- Disentangling the Galactic Halo with APOGEE: II. Chemical and Star Formation Histories for the Two Distinct Populations
- A Two Micron All-Sky Survey View of the Sagittarius Dwarf Galaxy: VI. s-Process and Titanium Abundance Variations Along the Sagittarius Stream
- The Chemical Composition of the Galactic Bulge and Implications for its Evolution
- High-Resolution Spectroscopy of the Planetary Host HD 13189: Highly-Evolved and Metal-Poor
- Sodium abundances in nearby disk stars
- Characterizing the High-Velocity Stars of RAVE: The Discovery of a Metal-Rich Halo Star Born in the Galactic Disk
- A comparison of the s- and r-process element evolution in local dwarf spheroidal galaxies and in the Milky Way
- Origins of the Thick Disk as Traced by the Alpha-Elements of Metal-Poor Giant Stars Selected from RAVE
- Chemical Abundances Of Three Metal-Poor Globular Clusters (NGC 6287, NGC 6293, And NGC 6541) In The Inner Halo
- A Unique Star in the Outer Halo of the Milky Way
- Statistical equilibrium of silicon in the atmospheres of metal-poor stars
- The Chemical Abundances of the Stellar Populations in the Leo I and Leo II dSph Galaxies
- Beryllium abundances in metal-poor stars
- An abundance study of red-giant-branch stars in the Hercules dwarf spheroidal galaxy
- Chemical Abundances of the Outer Halo Stars in the Milky Way
- Elemental Abundances in M31: A Comparative Analysis of Iron and Alpha Element Abundances in the Outer Disk, Giant Stellar Stream, and Inner Halo of M31
- Deep SDSS optical spectroscopy of distant halo stars II. Iron, calcium, and magnesium abundances
- Neutron Star Mergers Are the Dominant Source of the r-process in the Early Evolution of Dwarf Galaxies
- Beryllium in Disk and Halo Stars -- Evidence for a Beryllium Dispersion in Old Stars
- All quiet in the outer halo: chemical abundances in the globular cluster Pal 3
- The detailed chemical abundance patterns of accreted halo stars from the optical to infrared
- The chemical composition of globular clusters in the Local Group
- The fraction of first and second generation stars in globular clusters. I The case of NGC 6752
- Fluorine Abundances in the Milky Way Bulge
- The Gaia-ESO Survey: Carbon abundance in the Galactic thin and thick disks
- Insight Into the Formation of the Milky Way Through Cold Halo Substructure. II. The Elemental Abundances of ECHOS
- Chemical Compositions of Kinematically Selected Outer Halo Stars
- Chemical trends in the Galactic Halo with APOGEE data
- Reconstructing the Accretion History of the Galactic Stellar Halo from Chemical Abundance Ratio Distributions
- Chemical Abundances for the Outer Halo Cluster Pal 4 from Co-added High-Resolution Spectroscopy
- CD-62\degree1346: an extreme halo or hypervelocity CH~star?
- The Gaia-ESO Survey: Detailed Abundances in the Metal-poor Globular Cluster NGC 4372
- Early star formation in the Galaxy from beryllium and oxygen abundances
- Manganese Abundances in the Globular Cluster Omega Centauri
- What is the Milky Way outer halo made of? High resolution spectroscopy of distant red giants
- Radial Velocity and Metallicity of the Globular Cluster IC4499 Obtained with AAOmega
- A new algorithm for optimizing the wavelength coverage for spectroscopic studies: Spectral Wavelength Optimization Code (SWOC)
- Elemental abundances in M31: Individual and Coadded Spectroscopic [Fe/H] and [α/Fe] throughout the M31 Halo with SPLASH
- Beryllium in the Ultra-Lithium-Deficient,Metal-Poor Halo Dwarf, G186-26
- The 300km/s stellar stream near Segue 1: Insights From high-resolution spectroscopy of its brightest star
- G112-43/44: A metal-poor binary star with a unique chemical composition and kinematics like the Helmi streams
- Planetary companions around the metal-poor star HIP 11952
- Accretion of dust grains as a possible origin of metal-poor stars with low alpha/Fe ratios
- Triangulum-Andromeda overdensity: a region with a complex stellar population
- From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
- Second Parameter Globulars and Dwarf Spheroidals around the Local Group Massive Galaxies: What Can They Evidence?
- The Origin of the Metal-Poor Common Proper Motion Pair HD 134439/134440: Insights from New Elemental Abundances
- Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
- Chemical abundances of field halo stars -- Implications for the building blocks of the Milky Way
- The Stellar Population of the Thin Disk
- Complexity in small-scale dwarf spheroidal galaxies