Lithium abundances of halo dwarfs based on excitation temperature I. Local thermodynamic equilibrium

Astronomy and Astrophysics

Volumn 493, Issue 2, 2009, Pages 601-612

  Hosford, A ^a   Ryan, S G ^a   Pérez, A E García ^a   Norris, J E ^b   Olive, K A ^c  

^a UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^b AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^c University of Minnesota   (United States)

Author keywords

Cosmology: early universe; Galaxy: halo; nuclear reactions, nucleosynthesis, abundances; Stars: abundances

Indexed keywords

CHEMICAL ELEMENTS; COSMOLOGY; GALAXIES; GEOMETRICAL OPTICS; METALS; NUCLEAR ENERGY; NUCLEAR PHYSICS; NUCLEAR REACTORS; STARS; TEMPERATURE; TEMPERATURE SCALES;

BARYON DENSITIES; COSMOLOGY: EARLY UNIVERSE; EFFECTIVE TEMPERATURES; ENERGY METHODS; EQUIVALENT WIDTHS; EXCITATION TEMPERATURES; GALAXY: HALO; HIPPARCOS; IONIZATION BALANCES; ISOCHRONES; LOCAL THERMODYNAMIC EQUILIBRIUMS; METAL-POOR STARS; METALLICITY; MICROTURBULENCE; NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; PHYSICAL PARAMETERS; SIGNAL TO NOISE; STARS: ABUNDANCES; TEMPERATURE SCALE; UNCERTAIN FACTORS; WILKINSON MICROWAVE ANISOTROPY PROBES;

LITHIUM;

EID: 59049096646     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810240     Document Type: Article

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