The impact of an updated 14N( p,γ)15O reaction rate on advanced evolutionary stages of low-mass stellar models

Astronomy and Astrophysics

Volumn 522, Issue 6, 2010, Pages

  Pietrinferni, A ^a   Cassisi, S ^a   Salaris, M ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^b LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

Author keywords

abundances; nuclear reactions; nucleosynthesis; stars: evolution; stars: interiors

Indexed keywords

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

CHEMICAL ELEMENTS; LUMINANCE; NUCLEAR ENERGY; NUCLEAR PHYSICS; NUCLEAR REACTORS; REACTION RATES;

STARS;

EID: 78149253482     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/2010150     Document Type: Article

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