Evolution and nucleosynthesis of extremely metal-poor and metal-free low- And intermediate-mass stars I. Stellar yield tables and the CEMPs

Astronomy and Astrophysics

Volumn 490, Issue 2, 2008, Pages 769-776

  Campbell, S W ^a,b   Lattanzio, J C ^b  

^a INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^b MONASH UNIVERSITY   (Australia)

Author keywords

Galaxy: halo; Stars: AGB and post AGB; Stars: evolution; Stars: interiors

Indexed keywords

ASTROPHYSICS; CHEMICAL ELEMENTS; CODES (SYMBOLS); DYNAMICS; ELECTROMAGNETIC PULSE; ELECTROMAGNETIC WAVES; FLUID DYNAMICS; HELIUM; HYDROGEN; INERT GASES; POLLUTION; SUN;

CHEMICAL COMPOSITIONS; CHEMICAL EVOLUTIONS; CONSISTENT; DIFFUSION APPROXIMATIONS; EARLY UNIVERSES; GALACTIC HALOS; GALAXY: HALO; HALO STARS; LARGE DATA SETS; LOW MASSES; MASS MODELS; MASS STARS; METALLICITIES; METALLICITY; MULTI-DIMENSIONAL; NUCLEAR BURNING; OBSERVED DATUM; POST-PROCESSING; SIGNIFICANT SURFACES; SPECTRAL OBSERVATIONS; STARS: AGB AND POST-AGB; STARS: EVOLUTION; STARS: INTERIORS; STELLAR EVOLUTIONS; STELLAR STRUCTURES; STRUCTURAL EVOLUTIONS; TO MANY;

STARS;

EID: 54549121559     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809597     Document Type: Article

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