Lithium abundances of halo dwarfs based on excitation temperatures: II. Non-local thermodynamic equilibrium

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Hosford, A ^a   Garcia Perez A E ^a   Collet, R ^b   Ryan, S G ^a   Norris, J E ^c   Olive, K A ^d  

^a UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^d University of Minnesota   (United States)

Author keywords

Early Universe; Galaxy: halo; Line: formation; Radiative transfer; Stars: abundances; Stars: atmospheres

Indexed keywords

EARLY UNIVERSE; GALAXY: HALO; LINE: FORMATION; STARS: ABUNDANCES; STARS: ATMOSPHERES;

BAYESIAN NETWORKS; CHEMICAL ELEMENTS; GALAXIES; LITHIUM; RADIATIVE TRANSFER; STARS; THERMODYNAMICS;

TEMPERATURE;

EID: 79952848340     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913693     Document Type: Article

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