The core helium flash revisited: II. Two and three-dimensional hydrodynamic simulations

Astronomy and Astrophysics

Volumn 501, Issue 2, 2009, Pages 659-677

  Mocak M ^a,b   Muller E ^a   Weiss, A ^a   Kifonidis, K ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b UNIVERSITÉ LIBRE DE BRUXELLES   (Belgium)

Author keywords

Convection; Hydrodynamics; Stars: evolution; Stars: interiors

Indexed keywords

AXISYMMETRIC FLOW; CONVECTION; CONVECTION ZONE; CONVECTIVE FLOW; CONVECTIVE VELOCITY; DYNAMIC TIME; EULERIAN HYDRODYNAMICS; HYDRODYNAMIC SIMULATION; MIXING LENGTH; NUMERICAL TECHNIQUES; SPATIAL SCALE; STARS: EVOLUTION; STARS: INTERIORS; TEMPERATURE GRADIENT; TEMPORAL EVOLUTION; THREE DIMENSIONAL SIMULATIONS; THREE-DIMENSIONAL MODEL; TURBULENT CONVECTION; TURBULENT ENTRAINMENT; TWO DIMENSIONAL MODEL; TWO-DIMENSIONAL HYDRODYNAMICS; TWO-DIMENSIONAL SIMULATIONS;

FLOW PATTERNS; FORECASTING; HEAT CONVECTION; HELIUM; HYDRODYNAMICS; RADIOACTIVITY; SIMULATORS; STARS; THREE DIMENSIONAL; THREE DIMENSIONAL COMPUTER GRAPHICS; TWO DIMENSIONAL;

FLUID DYNAMICS;

EID: 67650938299     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811414     Document Type: Article

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