The production of short-lived radionuclides by new non-rotating and rotating Wolf-Rayet model stars

Astronomy and Astrophysics

Volumn 453, Issue 2, 2006, Pages 653-659

  Arnould, M ^a   Goriely, S ^a   Meynet, G ^b  

^a UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Solar system: formation; Stars: evolution; Stars: Wolf Rayet

Indexed keywords

ASTROPHYSICS; METEORITES; NUCLEAR PHYSICS; SOLAR SYSTEM; WIND EFFECTS;

ABUNDANCES; NUCLEAR REACTIONS; NUCLEOSYNTHESIS; SOLAR SYSTEM: FORMATION; STARS: EVOLUTION; STARS: WOLF-RAYET;

RADIOISOTOPES;

EID: 33745757172     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053966     Document Type: Article

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