Fluorine in carbon-enhanced metal-poor stars: A binary scenario

Astronomy and Astrophysics

Volumn 484, Issue 3, 2008, Pages

  Lugaro, M ^a,b   De Mink, S E ^a   Izzard, R G ^a   Campbell, S W ^b,c   Karakas, A I ^d   Cristallo, S ^e   Pols, O R ^a   Lattanzio, J C ^b   Straniero, O ^e   Gallino, R ^b,f   Beers, T C ^g  

^a UTRECHT UNIVERSITY   (Netherlands)

^b MONASH UNIVERSITY   (Australia)

^c INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

^d AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^e INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^f UNIVERSITY OF TURIN   (Italy)

^g MICHIGAN STATE UNIVERSITY   (United States)

Author keywords

Nuclear reactions, nucleosynthesis, abundances; Stars: abundances; Stars: AGB and post AGB; Stars: individual: HE 1305+0132

Indexed keywords

ASTROPHYSICS; CARBON; CHEMICAL ELEMENTS; FLUORINE; HELIUM; MASS TRANSFER; MICROFLUIDICS; ROTATION; STEEL ANALYSIS; UNCERTAINTY ANALYSIS;

(E ,3E) PROCESS; ASYMPTOTIC GIANT BRANCH (AGB); BINARY MODELS; CONVECTIVE BORDERS; CONVECTIVE ENVELOPE; GENERAL (CO); LOW-MASS; MASS LOSSES; MASSIVE STARS; METAL-POOR STARS; MODEL UNCERTAINTIES; POPULATION SYNTHESIS; STELLAR EVOLUTIONS;

STARS;

EID: 44849116271     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20079169     Document Type: Article

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