Production and evolution of Li, Be, and B isotopes in the Galaxy

Astronomy and Astrophysics

Volumn 542, Issue , 2012, Pages

  Prantzos, N ^a  

^a INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

abundances; Cosmic rays; Galaxy: evolution; Nuclear reactions; nucleosynthesis; Stars: abundances

Indexed keywords

ABUNDANCES; ASYMPTOTIC GIANT BRANCH STARS; AVERAGE YIELD; CURRENT MODELS; FULLY-COUPLED; GALACTIC CHEMICAL EVOLUTIONS; GALACTIC COSMIC RAYS; GALACTIC EVOLUTION; GALAXY: EVOLUTION; ISOTOPIC ABUNDANCES; ISOTOPIC RATIOS; KEY FEATURE; LIGHT ELEMENTS; LOW-MASS; MASSIVE STARS; MILKY WAYS; RADIAL PROFILES; RED GIANTS; SECONDARY PROCESS; SELF-CONSISTENT CALCULATION; SOURCE COMPOSITION; STARS: ABUNDANCES; STELLAR NUCLEOSYNTHESIS; STELLAR SOURCES; THEORETICAL DEVELOPMENT;

COSMIC RAYS; GALAXIES; ISOTOPES; NUCLEAR REACTIONS; NUCLEOSYNTHESIS;

STARS;

EID: 84861975191     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219043     Document Type: Article

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