Convective overshooting and production of s-nuclei in massive stars during their core He-burning phase

Astronomy and Astrophysics

Volumn 524, Issue 2, 2010, Pages

  Pumo, M L ^a,b   Contino, G ^c   Bonanno, A ^b   Zappala R A ^c  

^a INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^c UNIVERSITY OF CATANIA   (Italy)

Author keywords

Convection; nuclear reactions, nucleosynthesis, abundances; stars: evolution; Stars: interiors

Indexed keywords

CONVECTION; F VALUES; INITIAL MASS; MASSIVE STARS; METALLICITIES; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; OVERALL EFFICIENCY; POST PROCESSING; RULE OF THUMB; S-PROCESS; STARS: EVOLUTION; STARS: INTERIORS; STELLAR EVOLUTIONS; STELLAR MODELS; STILL MISSING; Z VALUE;

BIOLOGY; CHEMICAL ELEMENTS; NUCLEAR ENERGY; NUCLEAR PHYSICS; NUCLEAR REACTORS;

STARS;

EID: 78649388141     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015518     Document Type: Article

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