Implications of O and Mg abundances in metal-poor halo stars for stellar iron yields

Astronomy and Astrophysics

Volumn 388, Issue 3, 2002, Pages 842-860

  Argast, D ^a   Samland, M ^a   Thielemann, F K ^a   Gerhard, O E ^a  

^a UNIVERSITY OF BASEL   (Switzerland)

Author keywords

Galaxy: abundances; Galaxy: halo; ISM: abundances; Nuclear reactions, nucleosynthesis, abundances; Stars: abundances

Indexed keywords

APPROXIMATION THEORY; CALCULATIONS; FUNCTIONS; GALAXIES; IRON; MAGNESIUM PRINTING PLATES; MATHEMATICAL MODELS; NUCLEAR PHYSICS; OXYGEN;

CHEMICAL EVOLUTION MODELS; HYPERNOVA; METAL-POOR HALO STARS; NUCLEOSYNTHESIS; STELLAR IRON YIELDS; SUPERNOVAE;

ASTROPHYSICS;

EID: 0036611947     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20020545     Document Type: Article

References (78)