Rotational mixing in low-mass stars II. Self-consistent models of Pop II RGB stars

Astronomy and Astrophysics

Volumn 453, Issue 1, 2006, Pages 261-278

  Palacios, A ^a   Charbonnel, C ^b,c   Talon, S ^d   Siess, L ^a  

^a UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

^b UNIVERSITÉ DE GENÈVE   (Switzerland)

^c IRAP   (France)

^d UNIVERSITÉ DE MONTRÉAL   (Canada)

Author keywords

Hydrodynamics; Stars: abundances; Stars: evolution; Stars: interiors; Stars: rotation; Turbulence

Indexed keywords

DIFFUSION; EVOLUTIONARY ALGORITHMS; GALAXIES; HYDRODYNAMICS; MATHEMATICAL MODELS; SERVICE LIFE; TURBULENCE;

STAR: EVOLUTION; STAR: INTERIORS; STAR: ROTATION; STARS: ABUNDANCES;

ASTROPHYSICS;

EID: 33745740697     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053065     Document Type: Article

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