Submitted to ApJ Preprint typeset using L ATEX style emulateapj v. 6/22/04 LITHIUM ISOTOPIC ABUNDANCES IN METAL-POOR HALO
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Francesca Primas | Verne V. Smith | David L. Lambert | Poul Erik Nissen | V. Smith | M. Asplund | F. Primas | D. Lambert | P. Nissen | Martin Asplund
[1] M. Asplund,et al. On OH line formation and oxygen abundances in metal-poor stars , 2001, astro-ph/0104071.
[2] L. Rebull,et al. Lithium Isotope Ratios in Halo Stars. III. , 1997 .
[3] Observatories of the Carnegie Institution of Washington,et al. Oxygen Abundances in Metal-poor Stars , 2003, astro-ph/0307063.
[4] D. Kiselman,et al. Line formation in solar granulation IV. (O I), O I and OH lines and the photospheric O abundance , 2003, astro-ph/0312290.
[5] Inelastic H+Li and H-+Li+ collisions and non-LTE Li I line formation in stellar atmospheres , 2003, astro-ph/0308170.
[6] R. Kurucz. ATLAS9 Stellar Atmosphere Programs and 2 km/s grid. , 1993 .
[7] T. Beers,et al. Extremely Metal-Poor Stars. II. Elemental Abundances and the Early Chemical Enrichment of The Galaxy , 1996 .
[8] V. Smith,et al. Isotopic Lithium Abundances in Nine Halo Stars , 1998 .
[9] G. Fontaine,et al. The lithium abundance - Constraints on stellar evolution , 1984 .
[10] Andreu Alibés,et al. Galactic Cosmic Rays from Superbubbles and the Abundances of Lithium, Beryllium, and Boron , 2002, astro-ph/0202097.
[11] H. Schmoranzer,et al. PRECISION LIFETIME MEASUREMENTS ON ALKALI ATOMS AND ON HELIUM BY BEAM-GAS-LASER SPECTROSCOPY , 1996 .
[12] D. Welty,et al. A High-Resolution Survey of Interstellar K I Absorption , 1996 .
[13] Bruce W. Carney,et al. A Survey of Proper-Motion Stars. XVI. Orbital Solutions for 171 Single-lined Spectroscopic Binaries , 2002 .
[14] A. Korn. Rectifying Échelle Spectra — A Comparison Between UVES, FEROS and FOCES , 2002 .
[15] COSMOLOGICAL COSMIC RAYS AND THE OBSERVED ^6Li PLATEAU IN METAL-POOR HALO STARS , 2004, astro-ph/0412426.
[16] M. Tambasco,et al. ENERGIES AND OSCILLATOR STRENGTHS FOR LITHIUMLIKE IONS , 1997 .
[17] Present status of primordial nucleosynthesis after WMAP: results from a new BBN code , 2003, astro-ph/0307213.
[18] S. Ryan,et al. Lithium Abundances in the Most Metal-deficient Stars , 1994 .
[19] T. Beers,et al. Rapid Rotation of Ultra-Li-depleted Halo Stars and Their Association with Blue Stragglers , 2002, astro-ph/0202369.
[20] Richard H. Cyburt. Primordial nucleosynthesis for the new cosmology: Determining uncertainties and examining concordance , 2004 .
[21] S. Vauclair. Lithium Nuclear Destruction in Stellar Outer Layers: A Consistent Theoretical View of the Characteristic Features Observed in Young and Old Stars , 1988 .
[22] Piercarlo Bonifacio,et al. The primordial lithium abundance , 1997 .
[23] O/Fe in metal-poor main sequence and subgiant stars ? , 2002, astro-ph/0205372.
[24] J. B. Laird,et al. A survey of proper motion stars. 12: an expanded sample , 1994 .
[25] J. Richer,et al. Models of Metal-poor Stars with Gravitational Settling and Radiative Accelerations. II. The Age of the Oldest Stars , 2001, astro-ph/0112113.
[26] D. Ivanova,et al. Non-LTE analysis of the formation of KI lines in the spectra of A-K stars , 2000 .
[27] Cosmic Ray Production of 6Li by Virialisation Shocks in the Early Milky Way , 2003, Publications of the Astronomical Society of Australia.
[28] P. Barklem,et al. Cross sections for low-energy inelastic H+Li collisions (9 pages) , 2003 .
[29] F. Primas,et al. The lithium content of the Galactic Halo stars , 2005 .
[30] T. Beers,et al. Beryllium Abundances in Halo Stars from Keck/HIRES Observations , 1999 .
[31] D. F. Gray,et al. The Observation and Analysis of Stellar Photospheres , 2021 .
[32] H. Spruit,et al. Li depletion in F stars by internal gravity waves , 1991 .
[33] J. Thorburn. The Primordial lithium abundance from extreme subdwarfs: New observations , 1993 .
[34] Solar neutrino constraints on the BBN production of Li , 2003, astro-ph/0312629.
[35] R. Rebolo,et al. Evidence for planet engulfment by the star HD82943 , 2001, Nature.
[36] M. Pinsonneault,et al. Evolutionary models of halo stars with rotation. II: Effects of metallicity on lithium depletion and possible implications for the primordial lithium abundance , 1992 .
[37] Kindler-Rohrborn,et al. In press , 1994, Molecular carcinogenesis.
[38] C. Proffitt,et al. Diffusion and mixing of lithium and helium in population II dwarfs , 1991 .
[39] S. Inoue,et al. Cosmic-Ray Production of 6Li by Structure Formation Shocks in the Early Milky Way: A Fossil Record of Dissipative Processes during Galaxy Formation , 2002, astro-ph/0201190.
[40] Big-Bang nucleosynthesis and hadronic decay of long-lived massive particles , 2004, astro-ph/0408426.
[41] G. Steigman. PRIMORDIAL NUCLEOSYNTHESIS: SUCCESSES AND CHALLENGES , 2005, astro-ph/0511534.
[42] Did something decay, evaporate, or annihilate during Big Bang nucleosynthesis? , 2004, astro-ph/0402344.
[43] The Spite Lithium Plateau: Ultrathin but Postprimordial , 1999, astro-ph/9903059.
[44] H. C. Stempels,et al. Detailed analysis of Balmer lines in cool dwarf stars , 2002, astro-ph/0201537.
[45] P. S. Barklem,et al. The broadening of Fe II lines by neutral hydrogen collisions , 2005 .
[46] S. Woosley,et al. The nu-process , 1990 .
[47] Robert F. Stein,et al. Simulations of Solar Granulation. I. General Properties , 1998 .
[48] Suzanne Talon,et al. Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars , 2005, Science.
[49] Sansonetti,et al. Measurements of the resonance lines of 6Li and 7Li by Doppler-free frequency-modulation spectroscopy. , 1995, Physical review. A, Atomic, molecular, and optical physics.
[50] Halo Star Lithium Depletion , 1998, astro-ph/9803073.
[51] Signatures of Convection in teh Spectrum of Procyon: Fundamental Parametrs and Iron Abundance , 2001, astro-ph/0111055.
[52] T. Beers,et al. He 1327-2326, an unevolved star with [Fe/H] < -5.0. I. A comprehensive abundance analysis , 2005, astro-ph/0509206.
[53] K. Covey,et al. A search for 6Li in stars with planets , 2002, astro-ph/0205268.
[54] G. Israelian,et al. Oxygen Abundances in Unevolved Metal-poor Stars from Near-Ultraviolet OH Lines , 1998, astro-ph/9806235.
[55] Bernard Delabre,et al. Design, construction, and performance of UVES, the echelle spectrograph for the UT2 Kueyen Telescope at the ESO Paranal Observatory , 2000, Astronomical Telescopes and Instrumentation.
[56] G. Herbig. APPARENT LITHIUM ISOTOPE RATIOS IN F5-G8 DWARFS , 1964 .
[57] C. Proffitt,et al. Pre-main-sequence depletion of Li-6 and Li-7 , 1989 .
[58] Ko NakamuraToshikazu Shigeyama. ROLES OF SUPERNOVA EJECTA IN NUCLEOSYNTHESIS OF THE LIGHT ELEMENTS Li, Be, AND B , 2004, astro-ph/0404293.
[59] Y. Yoshii,et al. A New Model for the Evolution of Light Elements in an Inhomogeneous Galactic Halo , 2000, astro-ph/0010108.
[60] J. W. Brault,et al. Lifetimes, transition probabilities, and level energies in Fe i , 1991 .
[61] M. Asplund,et al. Multi-level 3D non-LTE computations of lithium lines in the metal-poor halo stars HD 140283 and HD 84937 , 2003, astro-ph/0302406.
[62] F. Hoyle,et al. Galactic Cosmic Ray Origin of Li, Be and B in Stars , 1970, Nature.
[63] Jorge Melendez,et al. The effective temperature scale of FGK stars. I. Determination of temperatures and angular diameters with the infrared flux method , 2005 .
[64] D. Fabbian,et al. Effective temperatures and lithium abundances of halo turnoff stars , 2005, Proceedings of the International Astronomical Union.
[65] Atomic diffusion in metal-poor stars - II. Predictions for the Spite plateau , 2001, astro-ph/0104406.
[66] Andreas Kaufer,et al. High S/N, high resolution Image Slicer observations with UVES , 2003, SPIE Astronomical Telescopes + Instrumentation.
[67] Jacques Richer,et al. Implications of WMAP Observations on Li Abundance and Stellar Evolution Models , 2004 .
[68] K. Butler,et al. The Solar Hydrogen Spectrum in Non-Local Thermodynamic Equilibrium , 2004 .
[69] Edward J. Wollack,et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters , 2003, astro-ph/0302209.
[70] N. Prantzos. The energetics, evolution, and stellar depletion of 6Li in the early Galaxy , 2005, astro-ph/0510122.
[71] S. Ryan,et al. Evolution of the Light Elements and the Cosmic-Ray Flux in the Galaxy , 1997 .
[72] R. Ramaty,et al. Light-Element Evolution and Cosmic-Ray Energetics , 1999, astro-ph/9909021.
[73] Paul Barklem,et al. A list of data for the broadening of metallic lines by neutral hydrogen collisions , 2000 .
[74] Primordial Lithium and Big Bang Nucleosynthesis. , 1999, The Astrophysical journal.
[75] Thomas G. Barnes,et al. Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis in honor of David L. Lambert , 2005 .
[76] V. Narayanan,et al. Stellar Mixing and the Primordial Lithium Abundance , 2001, astro-ph/0105439.
[77] G. Smith,et al. Oscillator strengths and collisional damping parameters for lines of neutral calcium , 1981 .
[78] The evolution of 6Li in standard cosmic-ray nucleosynthesis , 1998, astro-ph/9811183.
[79] Takeo Minezaki,et al. Nucleosynthetic signatures of the first stars , 2005, Nature.
[80] Gang Zhao,et al. On the Abundance of Potassium in Metal-Poor Stars , 2001, astro-ph/0110165.
[81] M. Bessell,et al. Nitrogen overabundances in Population II dwarfs , 1982 .
[82] R. Rebolo,et al. New measurement of the 6 Li= 7 Li isotopic ratio in the extra-solar planet host star HD 82943 and line blending in the Li 6708 Å region ? , 2003, astro-ph/0304358.
[83] J. Thorburn,et al. LITHIUM ISOTOPE RATIOS IN SIX HALO STARS , 1994 .
[85] V. Smith,et al. The 6Li/7Li ratio in the metal-poor halo dwarfs HD 19445 and HD 84937 , 1993 .
[86] F. Thevenin,et al. Stellar Iron Abundances: Non-LTE Effects , 1999, astro-ph/9906433.
[87] R. G. Gratton,et al. The O-Na and Mg-Al anticorrelations in turn-off and early subgiants in globular clusters , 2001 .
[88] V. Smith,et al. An Analysis of the K I λ7698 Line Profile in the Halo Turnoff Star HD 84937 and Its Implications for Lithium Isotopic Studies , 2001 .
[89] M. Asplund,et al. New light on stellar abundance analyses: Departures from LTE and homogeneity. , 2005 .
[90] Solving the discrepancy among the light elements abundances and WMAP , 2004, astro-ph/0402522.
[91] Updated Big Bang nucleosynthesis confronted to WMAP observations and to the abundance of light elements , 2003, astro-ph/0309480.
[92] S. Kawaler,et al. Lithium in halo stars from standard stellar evolution , 1990 .
[93] S. Vogt,et al. Oxygen in Unevolved Metal-Poor Stars from Keck Ultraviolet HIRES Spectra , 1999 .
[94] L. Pasquini,et al. Chemical abundances and mixing in stars in the milky way and its satellites : proceedings of the ESO-Arcetri Workshop held in Castiglione della Pescaia, Italy, 13-17 September, 2004 , 2006 .
[95] G. Starkman,et al. Is the Universe Closed by Baryons? Nucleosynthesis with a Late-decaying Massive Particle , 1988 .
[96] D. Alexander,et al. Models for Old, Metal-poor Stars with Enhanced α-Element Abundances. I. Evolutionary Tracks and ZAHB Loci; Observational Constraints , 2000 .
[97] Sulphur and zinc abundances in Galactic stars and damped Lyα systems , 2003, astro-ph/0311529.
[98] Ingemar Furenlid,et al. Solar flux atlas from 296 to 1300 nm , 1985 .
[99] Joseph Reader,et al. Wavelengths and Transition Probabilities for Atoms and Atomic Ions. Part I. Wavelengths. Part II. Transition Probabilities , 1980 .
[100] R. Ramaty,et al. Cosmic-Ray Acceleration from Supernova Ejecta in Superbubbles , 1998 .
[101] The effects of unstable particles on light-element abundances: Lithium versus deuterium and 3He , 2005, astro-ph/0503023.
[102] C. Stehlé,et al. Extensive tabulations of Stark broadened hydrogen line profiles , 1999 .
[103] Lithium–beryllium–boron: origin and evolution , 1999, astro-ph/9907171.
[104] A. Helmi,et al. Chemical Abundances and Mixing in Stars in the Milky Way and Its Satellites , 2006 .