Influence of two updated nuclear reaction rates on the evolution of low and intermediate mass stars (research note)

Astronomy and Astrophysics

Volumn 441, Issue 3, 2005, Pages 1129-1133

  Weiss, A ^a   Serenelli, A ^a,b   Kitsikis, A ^a   Schlattl, H ^a   Christensen Dalsgaard, J ^c  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b INSTITUTE FOR ADVANCED STUDY   (United States)

^c AARHUS UNIVERSITY   (Denmark)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: evolution; Stars: interiors

Indexed keywords

ALPHA PARTICLES; COMBUSTION; COMPOSITION; DATA REDUCTION; GALAXIES; METALS; SOLAR SYSTEM;

NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; STARS: EVOLUTION; STARS: INTERIORS;

ASTROPHYSICS;

EID: 26844466928     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053084     Document Type: Article

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